Enlaces a páginas de Observatorios y Telescopios:
AstroWeb: Observatories and Telescopes
1st High Energy Astrophysics Observatory
(HEAO 1. GSFC. NASA)
The first of NASA's three High Energy Astronomy Observatories, HEAO
1 was launched aboard an Atlas Centaur rocket on 12
August 1977 and operated until 9 January 1979. During that
time, it scanned the X-ray sky almost three times over
0.2 keV - 10 MeV, provided nearly constant monitoring of
X-ray sources near the ecliptic poles, as well as more
detailed studies of a number of objects through pointed observations.
2nd High Energy Astrophysics Observatory
(HEAO 2, renamed Einstein. GSFC. NASA)
The second High Energy Astronomy Observatory (HEAO-B) was launched into
an approximate 100-min low Earth orbit on 13 November 1978.
Renamed the Einstein Observatory, it operated (with one significant interruption)
until April 1981 and made over 5,000 targeted observations.
A Broad-Band Imaging X-ray All-Sky Survey
ABRIXAS is a small satellite mission which was planned to
observe the X-ray sky in the energy band 0.5-10 keV.
The mission failed shortly after launch in Spring 1999.
AREA31 Radio Observatory
A31RO is a privately owned astronomical radio observatory operated by
the Interstellar Electromagnetics Institute/L'institut Electromagnetiques Interstellaires under cooperative agreement with
the AREA31 Research Facility.
It is located near Shelburne,
Ontario, Canada, about 1-1/2 hrs drive NW of Toronto. The
Project TARGET microwave SETI program (since 1985), previously conducted at
the Hay River Radio Observatory and also the Algonquin Radio
Observatory is the primary initiative.
ATNF - Australia Telescope Compact Array
The Paul Wild Observatory, near Narrabri, is part of the
Australia Telescope National Facility (ATNF), and operated by the CSIRO;
the Officer-in-Charge is Dr Graham Nelson. The Narrabri site contains
the Australia Telescope Compact Array, which consists of five antennas
located along a 3-km railtrack, and a 6th antenna 3
km further to the west.
ATNF - Australia Telescope National Facility
CSIRO's Australia Telescope National Facility (ATNF) is an organisation that
supports and undertakes research in radio astronomy. It operates the
Australia Telescope, the collective name for a set of radio
telescopes in New South Wales. These telescopes are used, individually
or together, to study objects in the Universe ranging from
the remains of dead stars to entire galaxies.
ATNF - Mopra Antenna
The Mopra 22-m antenna is part of the Australia Telescope
National Facility (ATNF), operated by the CSIRO. It is intended
for use in conjunction with other AT antennas (the six
22-m dishes at Narrabri, and the 64-m Parkes dish) to
form the Long Baseline Array. Like the Parkes antenna, it
is also used for single-dish operation; mm-wavelength receivers are to
be installed soon.
ATNF - Parkes Observatory
The CSIRO Australia Telescope National Facility operates a group of
radio telescopes collectively known as the Australia Telescope. The ATNF
Parkes Observatory consists of a 64m telescope which is used
as an independent instrument, and networked with other Australian and
international radio telescopes for VLBI.
Active Magnetospheric Particle Tracer Explorers
Advanced Camera for Surveys
The Advanced Camera for Surveys (ACS) will be installed in
the Hubble Space Telescope (HST) during a Space Shuttle mission
scheduled in 2000. ACS will increase the discovery efficiency of
the HST by a factor of ten. ACS will consist
of three electronic cameras and a complement of filters and
dispersers that detect light from the ultraviolet at 1200 angstroms
to the near infrared at 10,000 angstroms.
Advanced Fiber-Optic Echelle
A Spectrograph for Precise Stellar Radial Velocity Measurements.
Advanced Satellite for Cosmology and Astrophysics
ASCA (formerly named Astro-D) is Japan's fourth cosmic X-ray astronomy
mission, and the second for which the United States is
providing part of the scientific payload. The satellite was successfully
launched February 20, 1993.
Air Force Maui Optical Station
Information about the Air Force Maui Optical Station (AMOS), located
on Maui, Hawaii. This is a dual-use facility, supporting both
US government agencies as well as the civilian community. Assets
include visible and IR sensors, and a 3.67 meter telescope
The Anglo-Australian Observatory operates the Anglo-Australian and UK Schmidt
Telescopes at Siding Spring, Australia, and a laboratory on the
same campus as the ATNF in the Sydney Suburb of
Antarctic Muon and Neutrino Detector Array
Antarctic Submillimeter Telescope and Remote Observatory
AST/RO is a 1.7m diameter telescope for submillimeter-wave astronomy and
aeronomy at Amundsen-Scott South Pole Station.
Apache Point Observatory
APO is privately owned and operated by the Astrophysical Research
Consortium. Located near Sunspot, New Mexico, the observatory consists of
a 3.5-meter telescope, the 2.5-meter Sloan Digital Sky Survey telescope,
and two smaller telescopes.
Arecibo Observatory - National Astronomy and Ionosphere Center
(The New Greek Telescope)
The New Greek Telescope project of the AI-NOA for
the 2.3m Ritchey-Chretien telescope, funded by the European Commission and
the General Secretariat for Research and Technology of the Hellenic
Ministry of Development.
Array of Low Energy X-ray Imaging Sensors
ALEXIS' X-ray telescopes feature curved mirrors whose multilayer coatings reflect
and focus low-energy X-rays or extreme ultraviolet light the way
optical telescopes focus visible light. The satellite and payloads were
funded by the Department of Energy and built by Los Alamos National Laboratory in collaboration with Sandia National Laboratory
and the University of California-Space Sciences Lab. The Launch was
provided by the Air Force Space Test Program on a
Pegasus Booster on April 25, 1993. The mission is entirely
controlled from a small groundstation at LANL.
Association Sciences et Techniques Jeunesse - Secteur Astronomie
(Astro-2. MSFC. NASA)
Astro-2 is a high-tech observatory flying for 16 days in
the payload bay of the Space Shuttle Endeavour during the
STS-67 mission. The Astro-2 instruments allow astronomers to view stars,
galaxies, planets and quasars in ultraviolet light, which is invisible
to our eye
Atacama Large Millimeter Array - ESO Web site
The Atacama Large Millimeter Array (ALMA) is the new name
for the merger of the major millimeter array projects into
one global project: the European Large Southern Array (LSA), the
U.S. Millimeter Array (MMA), and possibly the Japanese Large Millimeter
and Submillimeter Array (LMSA). This will be the largest ground-based
astronomy project of the next decade after VLT/VLTI, and, together
with the Next Generation Space Telescope (NGST), one of the
two major new facilities for world astronomy coming into operation
by the end of the next decade.
Atacama Large Millimeter Array - NRAO Web site
The Atacama Large Millimeter Array (ALMA) is a millimeter wavelength
telescope. The U.S. side of the project is run by
the National Radio Astronomy Observatory (NRAO), operated by Associated Universities,
Inc., under cooperative agreement with the National Science Foundation (NSF).
The European side of the project is a collaboration between
the European Southern Observatory (ESO), the Centre National de la
Recherche Scientifique, the Max-Planck-Gesellschaft, the Netherlands Foundation for Research in
Astronomy and Nederlandse Onderzoekschool Voor Astronomie, and the United Kingdom
Particle Physics and Astronomy Research Council.
Automated Patrol Telescope
The Automated Patrol Telescope (APT) is a wide-field CCD imaging
telescope, which is operated by the University of New South
Wales at Siding Spring Observatory, Australia.
Links to Automated telescopes on the Internet.
The X-ray astronomy satellite BeppoSAX (Satellite per Astronomia X "Beppo"
in honor of Giuseppe Occhialini) is a project of the
Italian Space Agency (ASI) with participation of the Netherlands
Agency for Aerospace Programs (NIVR).
In the framework of
past and future X-ray missions BeppoSAX stands out for its
wide spectral coverage, ranging from 0.1 to over 200 keV.
The sensitivity of the scientific payload allows the detailed study
over the entire energy band of sources as weak as
about 1/20 of 3C273. This opens new perspectives in the
study of broad band X-ray spectra and variability of cosmic
Berkeley Illinois Maryland Association
(BIMA - Hat Creek)
BIMA is a consortium consisting of the The University of
California at Berkeley, The University of Illinois at Urbana and
The University of Maryland at College Park which operates and
maintains a millimeter-wave radio interferometer at Hat Creek, California.
Big Bear Solar Observatory
This site contains daily images from our solar optical telescope
at Big Bear, California. Fulldisk images for the current month.
H-alpha, white light, and Ca-II K-line images are generally available
for every observing day; Ca-II K-line fulldisk archive; H-alpha fulldisk
archive; White light fulldisk archive; Current high-resolution region images; Programs
to read FITS images on IBM PCs and Macintoshes.
Big Ear Radio Observatory
(Ohio State University)
Big Ear is a Kraus-type radio telescope which covers an
area larger than three football fields. The telescope is famous
for discovering some of the most distant known objects in
the universe, and the longest-running SETI (Search for ExtraTerrestrial Intelligence)
Birmingham Solar Oscillations Network
The current status of the Birmingham Solar Oscillations Network -
a global network for helioseismology. Additionally some recent results and
publications are available. [site under reconstruction]
Broad Band X-ray Telescope
(BBXRT. GSFC. NASA)
The Broad Band X-ray Telescope (BBXRT) was flown on the
space shuttle Columbia (STS-35) on 1990 December 2-December 11, as
part of the ASTRO-1 payload. The flight of BBXRT marked
the first opportunity for performing X-ray observations over a broad
energy range (0.3-12 keV) with a moderate energy resolution (typically
90 eV and 150 eV at 1 and 6 keV,
Broadcast from Carl Sagan Observatory
Live broadcast of solar observation from Observatorio "Carl Sagan", Universidad
de Sonora, Mexico, from Monday to Saturday, 15 to 22
hrs UTC, weather permit.
Brown University - Observatories
Bucknell University Observatory
Byurakan Astrophysical Observatory
CERN Hybrid Oscillation Research apparatUS
The Center for High Angular Resolution Astronomy (CHARA) Array will
consist of five 1-m aperture telescopes (with an eventual goal
of seven) in a Y-shaped array contained within a 400m
diameter circle. This configuration will provide high resolution interferometry in
the visible spectral region as well as the K spectral
band (2.2 micron), with a limiting resolution of 0.2 milliarcsec
in the visible.
COROT - Asterosismology and Search for Exoplanets
A space mission of the French Space Agency (CNES), with
a launch planned in 2004. COROT stands for COnvection ROtation
and planetary Transits.
COsmic Background Explorer
Cagliari Astronomical Observatory
(International Latitude Station)
The Cagliari Astronomical Observatory was established as International Latitude Astronomical
Station of Carloforte in 1899, a small town of the
sardinian island of S. Pietro. It has been, for about
80 years, one of the five international stations devoted to
study the Earth rotation and polar motion. Observations with the
zenital telescope were carried out, except in the period of
the second world's war. Starting from 1978, the headquarters were
moved to Punta Sa Menta, a site 15 km far
from Cagliari which has the same latitude of the Carloforte
station. (Satellite Laser Ranging, Astrophysics, Planetary Dynamics, Time Laboratory, Data
Calar Alto Observatory
(Centro Astronomico Hispano-Aleman)
The German-Spanish Astronomical Center at Calar Alto is located in
the Sierra de Los Filabres in Southern Spain. It operates
four telescopes with apertures from 1.2m to 3.5m as well
as a Schmidt reflector. A 1.5m-telescope is operated under the
control of the Observatory of Madrid.
Caltech Submillimeter Observatory
The Caltech Submillimeter Observatory (CSO) is a cutting-edge facility for
astronomical research and instrumentation development. It consists of a 10.4-meter
diameter Leighton radio dish situated in a compact dome near
the summit of Mauna Kea, Hawaii.
Cambridge Optical Aperture Synthesis Telescope
Cambridge Ryle Telescope
Canada France Hawaii Telescope
CFHT is a joint facility of the National Research Council
of Canada, the Centre National de la Recherche Scientifique of
France, and the University of Hawaii. The CFH observatory hosts
a world-class, 3.6 meter optical/infrared telescope. The observatory is located
atop the summit of Mauna Kea, a 4200 meter, dormant
volcano located on the island of Hawaii. The CFH Telescope
became operational in 1979.
There is a Mirror
copy of the Web site at CDS.
A CFHT page at CADC has information about the
CFHT archive, CCDs, proposal template and manuals.
Canada France Hawaii Telescope (ftp)
Canadian Automatic Small Telescope for Orbital Research
(CASTOR Satellite Tracking Project)
The Canadian Automatic Small Telescopes for Orbital Research project, based
at the Royal Military College of Canada, uses small optical
telescopes to track medium to high earth orbit satellites such
as Russian, Molniya satellites.
Carlsberg Meridian Telescope
The Carlsberg Meridian Telescope (formerly the Carlsberg Automatic Meridian Circle)
is located on La Palma and is dedicated to carrying
out high-precision optical astrometry.
Carnegie Institution Observatories
Case Western Reserve University - Nassau Station Robotic Telescope
Cassini Mission to Saturn
(UltraViolet Imaging Spectrograph, UVIS)
Saturn and Titan will be the destination for the Cassini
mission, a project under joint development by NASA, the
European Space Agency and the Italian Space Agency.
The U.S. portion of the mission is managed for NASA
by the Jet Propulsion Laboratory.
Catania Astrophysical Observatory
Daily solar images (chromosphere and photosphere).
Cecil and Ida Green Piñon Flat Observatory
Center for Astrophysical Research in Antarctica
Center for Extreme Ultraviolet Astrophysics
(CEA / EUVE)
The Center for Extreme Ultraviolet Astrophysics (CEA) opened in September,
1990. CEA represents the culmination of twenty years of research
and student training in the field of EUV astronomy brought
to focus by the launch of NASA's research mission, the
University of California at Berkeley Extreme Ultraviolet Explorer (EUVE), on
June 7, 1992.
Centro de Investigaciones de Astronomia
The National observatory CIDA (Merida, Venezuela) hosts the biggest telescopes
of the earth equatorial belt: schmidt, reflector, refractor, astrograph.
Observatorio nacional están ubicados los telescopios astronómicos más importantes de
Venezuela y de la zona ecuatorial terrestre.
Cerro Tololo Interamerican Observatory
Cerro Tololo Interamerican Observatory is a complex of astronomical telescopes
and instruments located approximately 80 km to the East of
La Serena, Chile at an altitude of 2200 Meters.
is operated by the Association of Universities for Research
in Astronomy Inc. (AURA), under a cooperative agreement with the
National Science Foundation as part of the National
Optical Astronomy Observatories.
CfA 1.2 m Millimeter-Wave Telescope
The 1.2 meter Millimeter-Wave Telescope at the Harvard- Smithsonian Center
for Astrophysics and its twin instrument at CTIO in Chile
have been studying the distribution and properties of molecular clouds
in our Galaxy and its nearest neighbours for over 20
Chandra X-ray Observatory
The Chandra X-ray Observatory is the U.S. follow-on to the
Einstein Observatory. Chandra was formerly known as AXAF, the Advanced
X-ray Astrophysics Facility, but renamed by NASA in December, 1998.
The Chandra spacecraft carries a high resolution mirror, two imaging
detectors, and two sets of transmission gratings.
Cherenkov Array at Themis
Homepage of the CAT (Cherenkov Array at Themis) imager. This
is an atmospheric Cherenkov imaging telescope for detection of high-energy
gamma rays (>200 GeV), sited in the French Pyrenees.
Chicago Air Shower Array
The Chicago Air Shower Array (CASA) is a very large
array of scintillation counters located in Utah, fifty miles southwest
of Salt Lake City. CASA has been operating since 1992
in coincidence with a second array, the Michigan Anti (MIA),
is made of 2500 square meters of buried muon detectors.
CASA is the most sensitive experiment built to date in
the study of gamma-ray and cosmic ray interactions at energies
above 100 TeV (10^14 electron-Volts). Research topics on data from
this experiment cover a wide variety of physics issues, including
the search for gamma-rays from extragalactic sources (quasars and gamma-ray
bursts), the study of diffuse gamma-ray emission from the Galactic
plane, and a measurement of the cosmic ray composition in
the poorly understood region from 100 to 100,000 TeV.
Cincinnati Observatory Center
The Cincinnati Observatory Center is the first and oldest observatory
in the United States. It has been founded in 1842.
It hosts a 12-inch Merz und Mahler refractor and a
16-inch Alvan Clark refractor, each with a beautifully restored tube,
mount, and mechanical clock drive.
Collaboration between Australia and Nippon for a Gamma Ray Observatory in the Outback
The project uses two gamma ray telescopes at a dark
site 15 km from Woomera, a small town 500 km
north of Adelaide.
Complejo Astronómico El Leoncito
The Complejo Astronómico El Leoncito is an astronomical facility operated
under agreement between the Consejo Nacional de Investigaciones Científicas y
Técnicas de la República Argentina and the Universities of La
Plata, Córdoba and San Juan.
Its main telescope is a
2.15 meter reflector, equipped with direct CCD camera, spectrographs, a
photopolarimeter and other instruments. It is located at 2552 meters
above the sea level, in a high quality astronomical site
in the mountains of Calingasta, 240 km away from the
city of San Juan (Argentina).
The use of this facility
is open to the national and international astronomical community.
Compton Gamma-Ray Observatory
(CGRO. GSFC. NASA)
The Compton Gamma Ray Observatory is the second of NASA's
Great Observatories. Compton, at 17 tons, the heaviest astrophysical payload
ever flown, was launched on April 5, 1991 aboard the
space shuttle Atlantis. Compton has four instruments that cover an
unprecedented six decades of the electromagnetic spectrum, from 30 keV
to 30 GeV.
Compton/GRO Observatory Science Support Center/Guest Observer
Query the Library Database; Archive Data Selector; Archive Data Selector
Demonstrator; Trouble Report Generator; Access the GRONEWS Bulletin Board
The Constellation X-ray Mission (formerly HTXS) is a Next Generation
X-ray Observatory dedicated to observations at high spectral resolution, providing
as much as a factor of 100 increase in sensitivity
over currently planned high resolution X-ray spectroscopy missions.
Cosmic Anisotropy Telescope
The CAT is a three-element interferometer for cosmic microwave background
observations at 13 to 17 GHz.
Cracow - Solar radio emission in dm wavelength
Continuous observations of solar radio emission in decimeter wavelength have
been maintained in Cracow since 1957. Beginning from January 1995
we provide the reduced data on-line. The new instrument for
solar radio observations is under construction. It is to start
its operation in May, 1995.
Curtis Schmidt Telescope
The Curtis Schmidt telescope is a 0.61/.91 meter diameter Schmidt
telescope located at the Cerro Tololo InterAmerican Observatory, about
500 km north of Santiago, Chile. This telescope was originally
installed at the University of Michigan's Portage Lake Observatory in
1950, and moved to the much clearer skies of north
central Chile in 1966. Two thirds of the time on
this telescope is available to US and Chilean astronomers, with
the remaining one third reserved for astronomers from the Dept. of Astronomy at the University of Michigan.
Danish telescopes around the world
Dark Matter Telescope
The Dark Matter Telescope is a proposed 8.4 meter, 3-degree-field,
synoptic survey telescope.
(Space IR Interferometry Mission)
Darwin is a proposal for a European infrared
interferometer in space. Its first aim is to detect Earth-like
planets around nearby stars, and then to search for a
signature of life, ozone in an atmosphere. It could also
be used as a general-purpose infrared observatory.
was proposed to the European Space Agency (ESA) for
a Cornerstone Mission in its Horizon 2000 Plus plan. In
October 1995, ESA decided to study such an infrared interferometer
as an option for its Interferometer Cornerstone. The Darwin
and Edison teams have combined to promote
the selection by ESA of this option. The Darwin
advocacy team members are also members of the
International Working Group on Space Interferometry , a pressure group
for this type of mission. Final selection on cost, science
and technology grounds will be made around 2000, for a
launch in the period 2009 - 2017.
David Dunlap Observatory, University of Toronto
The David Dunlap Observatory is located in Richmond Hill, Canada.
As part of the University of Toronto's Department of Astronomy
it operates optical telescopes for research, the largest being a
1.88m telescope. DDO is also a centre for student training
and public education.
Deep Space Network - Goldstone Deep Space Station
The NASA Deep Space Network - or DSN - is
an international network of antennas that supports interplanetary spacecraft missions
and radio and radar astronomy observations for the exploration of
the solar system and the universe. The network also supports
some Earth-orbiting missions, including emergency support of the Shuttle Space
Deep Undersea Muon and Neutrino Detection
Directory tree of information about the DUMAND project, designed to
serve the needs of the experimenters, as well as to
make information about DUMAND progress available to the broader scientific
Deutsches Interferometer fuer Vielkanalphotometrie und Astrometrie
DIVA is a small astronomy satellite, planned for launch in
2004. It is aimed to measure positions, proper motions and
parallaxes, brightness and color of at least 30 million stars.
This amount and the high precision is unreached so
far by any predecessor mission. In a sense it is
a pathfinder mission for the technology of upcoming cornerstone missions
in the ESA Horizon 2000+ and the NASA Origins programmes
like GAIA, DARWIN, LISA, SIM etc.
Dutch Open Telescope
Innovative new optical solar telescope at the Roque de los
Muchachos Observatory on La Palma (Canary Islands). The DOT provides
extended sequences of solar images in various wavelengths with high
angular resolution (0.2 arcsec).
ESA - Villafranca Satellite Tracking Station
(ESA - VILSPA: IUE, ISO)
General information on the ESA Satellite Tracking Station and on
the projects supported at Villafranca: IUE, Marecs and ISO (in
the near future). The service includes links to other ESA
The Eddington mission was proposed in early 2000 to ESA
in response to the ``Call for mission proposals for two
flexi-missions''. The proposal was submitted by an international scientific team
led by I.W. Roxburgh (Astronomy Unit, QMW, Univ. of London,
UK), J. Christensen-Dalsgaard (University of Aarhus, Denmark) and F. Favata
(ESA/ESTEC). The mission has two complementary scientific aims, to produce
the data on stellar oscillations necessary for understanding the interior
structure and evolution of stars, and to detect and characterize
habitable planets around other stars.
Effelsberg Radio Telescope
The Max-Planck-Institut für Radioastronomie (MPIfR) operates the world's largest movable
radio telescope, a 100-m single-dish near Effelsberg, 40 km south
of Bonn, Germany.
The second of NASA's three High Energy Astrophysical Observatories, HEAO
2, renamed Einstein after launch, was the first fully imaging
X-ray telescope put into space. The few arcsecond angular resolution,
the field-of-view of tens of arcminutes, and a sensitivity several
100 times greater than any mission before it provided, for
the first time, the capability to image extended objects, diffuse
emission, and to detect faint sources. It was also the
first X-ray NASA mission to have a Guest Observer program.
Overall, it was a key mission in X-ray astronomy and
its scientific outcome completely changed the view of the X-ray
Estación de Observación Solar-Observatorio
The Astronomy Area of CIF-US (Center for Research on Physics/Universidad
de Sonora, Hermosillo Sonora, Mexico), operates EOS (Estacion de Observacion
Solar/Solar Observational Station)and OCS (Observatorio "Carl Sagan"), the only two
solar observatories in the country with an observational program of
active regions at the continuum, and H-Alpha and Calcium lines,
through a two-heliostat system and a 15 cm refractor telescope.
Live broadcast of solar observations through ASTRO-USON WebTV with the
new 14 cm Maksutov-H-Alpha telescope.
European Northern Observatory
The Instituto de Astrofísica de Canarias (IAC) and its Observatories
(the Observatorio de Teide, on Tenerife, and the Observatorio del
Roque de los Muchachos, on La Palma) make up a
Spanish research and observational centre, which, since 1979, has been
open to the international scientific community and effectively constitute the
European Northern Observatory (ENO).
European Southern Observatory
ESO, the European Southern Observatory, is a multinational organisation of
eight European member states. It operates astronomical observatories in Chile
and has its headquarters in Munich, Germany.
European VLBI Network
The European VLBI network (EVN) home page includes general information
on the EVN, including contact adresses around the network, Call
for Proposals, the EVN PC page, EVN and global VLBI
scheduling, VLBINFO account, EVN experiment feedback facility, Network monitoring reports
and other technical documents, the EVN Newsletter archive and a
description of the type of science that can be investigated
with the EVN array.
European X-ray Observatory
(EXOSAT at GSFC. NASA)
The European Space Agency's X-ray Observatory, EXOSAT, was operational from
May 1983 to April 1986. During that time, EXOSAT made
1780 observations of a wide variety of objects, including active
galactic nuclei, stellar coronae, cataclysmic variables, white dwarfs, X-ray binaries,
clusters of galaxies, and supernova remnants.
European X-ray Observatory
(EXOSAT at ESTEC, ESA)
The Exosat satellite was operational from May 1983 until April
1986 and in that time made 1780 observations in the
X-ray band of most classes of astronomical object. The payload
consisted of three instruments that produced spectra, images and light
curves in various energy bands.
Exploration of Neighboring Planetary Systems
NASA's plan for the Exploration of Neighboring Planetary Systems (ExNPS)
consists of a long term program of continuous scientific discovery
and technological development leading ultimately to the detection and characterization
of Earth-like planets around nearby stars.
(NASA Small Explorer Program)
The NASA Fast Auroral Snapshot Explorer (FAST) Satellite is designed
to investigate the plasma physics of the auroral phenomena which
occur around both poles of the earth.
FOcal Reducer/low dispersion Spectrograph
(FORS, ESO VLT)
The two FORS instruments are designed as all-dioptric focal reducers
for the ESO Very Large Telescope. They are capable of
doing : direct imaging , long slit grism spectroscopy ,
multi object grism spectroscopy , polarimetry (FORS1), medium dispersion echelle
grism spectroscopy (FORS2), and all sensible combinations of these modes
(e.g. imaging- or spectropolarimetry) in the wavelength range from 330nm
FUEGOS - Multi-Object Area Spectrograph
The FUEGOS instrument stands for Fibre Unit for Extra-Galactic Optical
Spectroscopy and will be capable of performing Multi-object spectroscopy and
Area spectroscopy in the 370nm to 900nm wavelength range and
with two resolving powers, 17000 and 7500.
(French site, IAP, Paris)
[in French] Site of the French team contributing to Far
Ultraviolet Spectroscopic Explorer (FUSE).
FUSE est un satellite observatoire
de la NASA dédié à la spectroscopie haute résolution dans
le domaine ultraviolet. Ce programme est realisé en coopération avec
l'Agence Spatiale Canadienne et le Centre National d'Etudes Spatiales (CNES).
Far Ultraviolet Spectroscopic Explorer
Information on the Far Ultraviolet Spectroscopic Explorer, a satellite astronomy
project based at The Johns Hopkins University
Fiber Linked Unit for Optical Recombination
One of the three recombination instruments of IOTA interferometer.
Fibre Large Area Multi Element Spectrograph
(FLAMES, ESO VLT)
FLAMES is a Fibre Facility for the ESO VLT. It
includes an high and intermediate resolution optical spectrograph (GIRAFFE), with
its own fibre system.
Five College Radio Astronomy Observatory
The FCRAO was founded in 1969 by the University of
Massachusetts, together with Amherst College, Hampshire College, Mount Holyoke College
and Smith College. The original low frequency telescope was superseded
in 1976 by a 14-m diameter radome-enclosed antenna for use
at high radio frequencies (mm wavelengths), built primarily to study
the physics and chemistry of interstellar clouds, circumstellar envelopes, planetary
atmospheres, and comets.
Francois-Xavier Bagnoud Observatory
The François-Xavier Bagnoud Observatory, located above the village of St-Luc
in the Swiss Alps, stands at an altitude of 2200
metres. It is intended not only for the experienced amateur
wishing to produce work of a quasi-professional quality, but also
for the use of schools and for simple visitors. curious.
Equipped with numerous instruments (60 cm reflecting telescope with
CCD camera, 20 cm refracting telescope, coelostat, 16 cm coronagraph)
it may be used day or night.
Fred Lawrence Whipple Gamma-Ray Telescopes
Full-sky Astrometric Mapping Explorer
FAME is an astrometric satellite designed to determine with unprecedented
accuracy the positions, distances, and motions of 40 million stars
within our galactic neighborhood. It is a collaborative effort between
the U.S. Naval Observatory (USNO) and several other institutions. FAME
will measure stellar positions to less than 50 microarcseconds. It
is a NASA MIDEX mission scheduled for launch in 2004.
Galactic Exoplanet Survey Telescope
Galaxy Evolution Explorer
A Space Ultraviolet imaging and spectroscopic mission that will map
the global history and probe the causes of star formation
over the redshift range 0 < z < 2.
Gamma-Ray Astronomy with COMPTEL
Local project documentation and utilities as well as collaboration-wide information
sources are maintained by the MPE COMPTEL people for: COMPTEL
Data Reduction Group work: documents, scientific results and utilities used
by the data analysts, the processing team and the scientists.
COMPASS software system work : technical and management documents, used
and maintained by the MPE software team. the local computing
environment : documents on system configuration, maintained by the MPE/RZG
software team. MPE - COMPTEL People Matters: the weekly activity
list individual 'home pages'
Gamma-ray Large Area Space Telescope
The GLAST Mission is under study for flight in the
first decade of the next century. GLAST is a next
generation high-energy gamma-ray observatory designed for making observations of celestial
gamma-ray sources in the energy band extending from 10 MeV
to more than 100 GeV.
Gemini - U.K. Support Group
The U.K. GEMINI Support Group based at Oxford University, England
is aimed at supporting the U.K. astronomer community in the
use of the GEMINI 8m Telescopes. This site is the
main source of information on the telescopes themselves, their instrument
compliment, applying for observing time, observing with the GEMINI telecopes
and post-observing data reduction/analysis for U.K. researchers.
Gemini 8m Telescopes
The Gemini 8m Telescopes Project is an international project to
build two infrared-optimized telescopes. One telescope will be located on
Mauna Kea, Hawaii; the other will be on Cerro Pachon,
Gemini Multiobject Spectrographs
There will be one GMOS for each of the two
GEMINI 8-m telescopes ( UK mirror ) which are due
for completion in 1998 and 2000. They will provide a
versatile low/medium resolution spectroscopic capability which will exploit the excellent
image quality delivered by the telescopes at optical and near-infrared
Astro-C, renamed Ginga (Japanese for 'galaxy'), was launched from the
Kagoshima Space Center on 5 February 1987. The primary instrument
for observations was the Large Area Counter (LAC). Ginga was
the third Japanese X-ray astronomy mission, following Hakucho and Tenma.
Ginga reentered the Earth's atmosphere on 1 November 1991.
INACTIVE LINK ? - 18 ---
Gloabal Astrometric Interferometer for Astrophysics
GAIA is a preliminary concept for a second space astrometry
mission (after HIPPARCOS), recently recommended within the context of ESA's
Horizon 2000 Plus long-term scientific programme. It is aimed at
the broadest possible astrophysical exploitation of optical interferometry using a
modest baseline length.
Global Oscillation Network Group
Goddard High Resolution Spectrograph Investigation Definition Team
The GHRS is one of four axial instruments on the
Hubble Space Telescope and is designed to obtain UV spectra
over a wide range of resolutions. This page was set
up as a reference source for team members and other
users of the instrument.
Gran Telescopio CANARIAS
The Gran Telescopio CANARIAS (GTC), is a high performance segmented
10-meter telescope to be installed in one of the best
sites of the Northern Hemisphere: the Roque de los Muchachos
Observatory (La Palma, Canary Islands, Spain). First light is planed
The GTC project is a Spanish initiative,
led by the IAC (Instituto de Astrofísica de Canarias)
with the aim of becoming an international project. GRANTECAN
has undertaken the construction of this telescope.
Grand Interferometre a 2 Telescopes
Optical Interferometer, Plateau du Calern, Departement Fresnel, Observatoire de la
Côte d'Azur, France [in French].
The National Radio Astronomy Observatory in Green Bank (West Virginia)
is a facility of the National Science Foundation operated under
cooperative agreement by Associated Universities, Inc.
Grove Creek Observatory, Australia
Grove Creek Observatory in NSW Australia, specializes in CCD imaging
and research. Accomodation is available for visiting amateur astronomers.
Guillermo Haro Observatory
Hard Labor Creek Observatory
Hartebeesthoek Radio Astronomy Observatory
Hat Creek Radio Observatory
High Energy Astrophysics Observatories
(HEASARC. GSFC. NASA)
Comprehensive list of satellites with high energy astrophysics instrumentation. Includes
images from these missions.
High Energy Solar Spectroscopic Imager
Studying the Fundamental Aspects of Solar Flares.
High Energy Transient Explorer
The High Energy Transient Explorer is a small scientific satellite
designed to detect and localize gamma-ray bursts.
High Energy X-ray Timing Experiment
The High Energy X-ray Timing Experiment is one of 3
common-user instruments on board the Rossi X-ray Timing Explorer (RXTE)
which was launched on 1995 December 30. The HEXTE is
sensitive to X-rays from 15 to 250 keV and is
able to time-tag photons in this energy range to 8
High Resolution Fly's Eye Cosmic Ray Detector
The HiRes detector - an atmospheric fluorescence detector: HiRes currently
consists of two sites on top of two mountains separated
by 13km in western Utah.
High Resolution Fly's Eye Cosmic Ray Detector
The HiRes detector - an atmospheric fluorescence detector: HiRes currently
consists of two sites on top of two mountains separated
by 13km in western Utah.
High-Resolution Near-Infrared Camera
(CONICA, ESO VLT)
The high-resolution near-IR camera CONICA covers the infrared wavelength range
from 1 µm to 5 µm. It is installed at
the Nasmyth B focus of the VLT Unit Telescope 1
to operate in conjunction with the Nasmyth Adaptive Optics System
(NAOS). CONICA is designed to exploit the adaptively corrected telescope
image at wavelengths longwards of 2 µm. Speckle interferometry can
be performed, primarily at the shorter wavelengths.
Hilal, Islam, Astronomy, and Cyberspace
(Crescent Moon Sighting)
This website provides Monthly Crescent Moon Sighting information for many
locations around the world. This provides the basis for a
Hobby Eberly Telescope
The Hobby-Eberly telescope (HET) is a new 9 meter telescope,
built at the University of Texas McDonald Observatory near
Ft. Davis Texas as a result of an international collaboration
between the University of Texas at Austin, The
Pennsylvania State University and Stanford University in the United
States and Ludwig-Maximilians-Universitaet Muenchen, and Goerg-August-Universitaet Goettingen. The
HET has been tailored for spectroscopy, and in particular, fiber-coupled
Hopkins Ultraviolet Telescope
Astronomers at the Johns Hopkins University designed the Hopkins Ultraviolet
Telescope (HUT) to explore the far- and extreme-ultraviolet portions of
the electromagnetic spectrum. HUT has a 36-inch primary mirror which
collects ultraviolet light for a prime-focus spectrograph. The spectrograph disperses
light in the 825 to 1850 Angstrom wavelength range with
a resolution of 3 Angstroms
Hubble Space Telescope
(HST - from CADC)
Also, there is a page from ST-ECF .
IAC / Observatorio Roque de los Muchachos
IAC / Observatorio del Teide
IPS Radio & Space Services
IPS is a unit of the Australian Government Department of
Administrative Services and provides the Australian radio propagation and space
environment services. Includes: Sydney Regional Warning Centre; Culgoora Solar Observatory;
Learmonth Solar Observatory; Prediction Services; Consultancy Services
Infra-Red Space Interferometer DARWIN
(IRSI / DARWIN)
The `InfraRed Space Interferometry Mission' DARWIN (IRSI or DARWIN) is
a cornerstone mission in the ESA `Horizon 2000+' science plan.
The goals for this space mission is for the first
time to detect terrestial planets in orbit around other stars
than our Sun.
Infra-Red Telescope Facility
The IRTF is a 3.0 meter telescope optimized for use
in the infrared. It was first built to support the
Voyager missions to Jupiter. It is now the National facility
for infrared astronomy providing continued support to planetary and deep
Also contains an Anonymous FTP
site: Manuals, Forms, Instrument information, Software tools.
Infrared Array Camera for the Space Infrared Telescope Facility
The Space Infrared Telescope Facility (SIRTF) contains three focal
plane instruments, one of which is the Infrared Array Camera
(IRAC). IRAC is a four-channel camera that provides simultaneous 5.12
x 5.12 arcmin images at 3.6, 4.5, 5.8, and 8
Infrared Space Observatory
The Infrared Space Observatory (ISO) is an ESA (European Space
Agency) mission with the participation of ISAS (Japan) and NASA
(USA). This WWW server is maintained at the ISO Data
Centre, which is based at Villafranca, Madrid, and is part
of the Astrophysics Division of the Space Science Department.
Infrared Space Observatory U.S. Support Center
U.S. science support center for observers using the Infrared Space
Observatory (ISO), a fully approved and funded project of the
European Space Agency (ESA).
Infrared Spectrometer And Array Camera
(ISAAC, ESO VLT)
ISAAC covers the wavelength range 1-5µm and is designed primarily
for: 'wide' (2.5x2.5') field imaging and long slit low &
medium resolution spectroscopy.
Infrared and Optical Telescope Array
Institut de Radio Astronomie Millimétrique
IRAM is an international institute for research in millimeter astronomy,
cofunded by the CNRS (Centre National de la Recherche Scientifique,
France), the MPG (Max Planck Gesellschaft, Germany), and since September
1990 the IGN (Instituto Geografico Nacional, Spain).
IRAM sites are: Grenoble, France : the IRAM headquarters, Laboratories
(the SIS junction lab the backend group, the receiver group
; Plateau de Bure, France : the interferometer of four
15-m antennas ; Granada, Spain : the Granada laboratories, the
30-m telescope located on Pico Veleta.
Institute of Astronomy, Bulgaria
Institute of Astronomy, Bulgaria (IABG) and National Astronomical Observatory "Rozhen".
Instituto Argentino de Radioastronomia
Información sobre las características del Instituto Argentino de Radioastronomía, sus
facilidades instrumentales, tareas de investigación y desarrollo en curso, personal
científico y técnico y actividades de extensión.
Instituto Nacional de Astrofísica, Óptica y Electrónica. Astrophysics Department
Information on the Large Millimeter Telescope an about the Cananea
Interferometry Center of Excellence
The Interferometry Center of Excellence (ICE), at JPL, has been
established to ensure the development and maintenance of a leading
edge capability in optical and near-infrared interferometric astrometry and imaging.
International Gamma-Ray Astrophysics Laboratory
(INTEGRAL. ESTEC. ESA)
Technical status of Integral. The mission utilises the service module
(bus) under development for the ESA XMM project. Integral
will be launched in 2001. The mission is conceived as
an observatory led by ESA with contributions from Russia and
International Interference Mitigation (for Radio Astronomy)
This Web site is a meeting place for anyone interested
in the technical problems of making radio astronomical measurements in
the presence of other radio signals. Postings on this site
are from scientists and engineers around the world on subjects
such as suppression of RFI from electronic devices, measurement of
the electromagnetic environment, and techniques for separating weak cosmic signals
from other radiation in the radio spectrum.
International Liquid Mirror Telescope Project
International Ultraviolet Explorer
The International Ultraviolet Explorer (IUE) satellite was launched on the
26th of January 1978 by a Thor-Delta rocket from Cape
Kennedy and transferred into a geosynchronous orbit over the Atlantic
Ocean. Information on the project is available at:
Iowa Robotic Observatory
A Consortium consisting of faculty from the Regents Universities of
the State of Iowa (University of Iowa, Iowa State University,
and University of Northern Iowa) manages this fully robotic Observatory
for undergraduate teaching and research in astronomy and related fields.
The Iowa Robotic Observatory (IRO) consists of a fully computerized
telescope and enclosure, a large format imaging CCD camera and
The Winer Mobile Observatory is providing a
site in southeastern Arizona to maintain and operate the telescope.
Iowa Robotic Telescopes Facilities
The University of Iowa Physics and Astronomy Department maintains
these pages as a guide to our suite of robotic,
autonomous tasking telescopes. In addition to using these instruments for
teaching and faculty and student research, limited observing time is
made available to anyone with an interest in Astronomy and
a valid observing request.
Isaac Newton Group - La Palma
The Issac Newton Group consists of three telescopes, the 4.2
metre William Herschel Telescope, the 2.5 metre Isaac Newton Telescope,
and the 1 metre Jacobus Kapteyn Telescope. They are situated
at the Observatorio del Roque de los Muchachos, on the
island of La Palma in the Canary Islands, and are
operated by the Royal Observatories of the UK. This resource
contains documentation for many of the major instruments, details of
how to apply for time, brief descriptions of the telescopes,
details and status of the service programme, current telescope schedules,
weather information for La Palma, and pointers to other institutions
which share the site.
The site is mirrored at
http://www.ast.cam.ac.uk/ING/ for faster access to UK users.
James Clerk Maxwell Telescope
The 15-m JCMT is situated close to the summit of
Mauna Kea, Hawaii, and is the largest submillmetre facility in
the world. It is owned and operated by the UK,
Canada and the Netherlands on behalf of astronomers worldwide. Its
home page contains information about the site, the antenna and
the instrumentation, as well as a description of the JCMT-CSO
interferometer, and details of the various time allocation processes.
Jicamarca Radio Observatory
Radar studies of the ionosphere and upper atmosphere.
Jodrell Bank Observatory
(University of Manchester)
Jodrell Bank Observatory is part of the University of Manchester's
Department of Physics and Astronomy. The Laboratories are home to
the Lovell Telescope and the MERLIN & VLBI National Facility
which is operated by the University on behalf of PPARC.
Joint Astronomy Centre
The Joint Astronomy Centre incorporates the 15m James Clerk Maxwell
Telescope (JCMT) and the 3.8m United Kingdom Infrared Telescope (UKIRT)
on the 4200m summit of Mauna Kea along with the
Centre's Hawaii headquarters in Hilo. The facility is operated by
the Royal Observatory, Edinburgh on behalf of the Science and
Engineering Research Council of the United Kingdom, the Nederlandse Organisatie
Voor Wetenschappelijk Onderzoek and the National Research Council of Canada.
Joint Institute for VLBI in Europe / European VLBI Network
(JIVE / EVN)
The European VLBI Network (EVN) was formed in 1980 by
a consortium of five of the major radio astronomy institutes
in Europe (the European Consortium for VLBI). Since 1980, the
EVN and the Consortium has grown to include 9 institutes
with 12 telescopes in 8 western European countries as well
as associated institutes with telescopes in Poland, Russia, Ukraine and
China. Proposals for additional telescopes in Spain and Italy are
under consideration, and furthermore, the EVN can be linked to
the 7-element Jodrell Bank MERLIN interferometer in the UK and
to the US Very Long Baseline Array (VLBA) to create
a " global network" . In 1993 the Joint Institute
for VLBI in Europe (JIVE) was created, with the Netherlands
Foundation for Research in Astronomy (Dwingeloo) acting as the host
institute. It will provide both scientific user support and a
correlator facility. Very Long Baseline Interferometry (VLBI) achieves ultra-high angular
resolution and is a multi-disciplinary technique e.g. imaging of extragalactic
radio sources, geodesy and astrometry. See EVN-TWG Meeting
. There is also an EVN anonFTP directory
at JB .
Kanzelhoehe Solar Observatory
The Kanzelhoehe Solar Observatory is operated by the Institute of
Geophysics, Astrophysics and Meteorology (IGAM) of the University of Graz,
Austria. It is located near Villach, close to the Italian
and Slovenian border. Operated continuously and devoted also to Solar
surveillance since its foundation in 1943 it houses a rich
archive of observations.
Kiepenheuer-Institut für Sonnenphysik
The Kiepenheuer-Institut is a research institution of the German state
of Baden-Wuerttemberg, dedicated to the study of the Sun. It
is located in Freiburg, Germany, and operates solar observing facilities
at the Observatorio del Teide, Tenerife, Spain.
Kitt Peak National Observatory
There is also an anonymous ftp
Kitt Peak Observing Information
Koelner Observatorium fuer SubMillimeter Astronomie
The 3-m KOSMA telescope at Gornergrat (Switzerland) is operated by
the I. Physikalisches Institut (Cologne, Germany). It can be used
for observations between 210 and 820 GHz.
Kuiper Airborne Observatory
The Observing Station of the Uppsala Observatory.
The Large Binocular Telescope (LBT) is a collaboration between the
University of Arizona, the Italian astronomical community, which is represented
by the Arcetri Astrophysical Observatory in Florence, and the Research
Corporation in Tucson. The goal of the LBT project is
to construct a binocular telescope consisting of two 8.4-meter mirrors
on a common mount. This telescope will be equivalent in
light-gathering power to a single 11.8-meter instrument. Because of its
binocular arrangement, the telescope will have a resolving power (ultimate
image sharpness) corresponding to a 23-meter telescope.
LECS Instrument on BeppoSAX
(SAX, ESTEC, ESA)
SAX is devoted to systematic, integrated and comprehensive studies of
galactic and extragalactic X-ray sources in the energy band 0.1
- 200 keV; the observational goal to be addressed is
to continue and expand upon previous spectral and timing observations
of celestial sources in those areas for which the existing
information is missing or inadequate and will remain uncovered in
the foreseable future.
La Silla - ESO Facilities
Lake Afton Public Observatory
(Wichita State University)
Large Angle and Spectrographic Coronagraph for SOHO
This instrument monitors the solar corona above the Sun's limb
in a similar way as we perceive the corona during
a solar eclipse. It produces images of the corona in
the visible spectrum and with distance off the Sun's center
ranging from 1.1 to 32 solar radii.
Large Millimeter Telescope / Gran Telescopio Milimétrico
The Large Millimeter Telescope is a bi-national project sponsored by
both U.S. and Mexican governments and institutions to build the
largest single-dish millimeter-wavelength radio telescope ontop of the mountain Cerro
La Negra near Puebla in Mexico. The telescope is currently
under construction with a rough completion date near 2003.
Large Millimeter and Submillimeter Array Project
Laser Guide Star Adaptive Optics
The focus of the Laser Guide Star Adaptive Optics Program
at Lawrence Livermore National Laboratory (LLNL) is the development of
integrated adaptive optics (AO) and sodium-layer laser guide star (LGS)
systems for use on large astronomical telescopes.
Laser Interferometer Gravitational-Wave Observatory
Leonardo da VINCI - Interferometry
VINCI is the VLT INnterferometer Commissionning Instrument, a collaboration of
ESO, DESPA (Observatoire de Paris), MPE and OMP. It combines
the light coming from two telescopes using single-mode fluoride glass
Limber Observatory is a private observatory and residence in the
Texas Hill Country near San Antonio, specializing in optical polarimetry
of early emission line stars.
Liquid Mirrors at Université Laval
Liquid Mirror (LM) technology is being developed at Université Laval.
A f/1.2, 2.5 meter diameter, mercury mirror is being extensively
tested in our testing tower. We are also exploring the
use of gallium eutectics as reflecting liquids. The design of
novel optical correctors to increase the accessible field of view
of liquid mirrors up to 45 degrees is also addressed.
Liverpool John Moores University, Astrophysics Research Institute
(ARI, Liverpool JMU)
Details of the research and teaching interests of the group,
as well as information on the Liverpool Telescope project
- a fully-robotic 2m telescope to be situated at the
Observatorio del Roque de los Muchachos, La Palma.
well as the Astrophysics degree-course with Liverpool University, we also
have an innovative distance learning course.
Tools and informations for observers at the 152 cm Loiano
Telescope of Bologna Astronomical Observatory. Tools include a web form
for submitting proposals. Informations on road map, weather and accomodations
Loiano Telescopes - Bologna
INACTIVE LINK ? - 18 ---
Low Energy Gamma-Ray Imager
LEGRI is a payload for the first mission of the
Spanish MINISAT platform. The objective of LEGRI is
to demonstrate the viability of HgI2 detectors for space astronomy,
providing imaging and spectroscopical capabilities in the 10-100 keV range.
Low Frequency Array
e Low Frequency Array (LOFAR) is a radio telescope that
will operate at the lowest frequencies that are accessible from
earth. The current plan is that LOFAR will work in
the range from 10-240 MHz. The telescope is being developed
by ASTRON, based in Dwingeloo (the Netherlands), the Naval Research Laboratory in Washington DC (USA) and MIT
Haystack Observatory (USA).
MDM Observatory was founded by the University of
Michigan, Dartmouth College, and the Massachusetts Institute
of Technology. Current operating partners include Michigan, Dartmouth,
MIT, Ohio State University, and Columbia University.
The Observatory is located on the southwest ridge of the
Kitt Peak National Observatory near Tucson, AZ. It
operates two telescopes: the 2.4-m Hiltner telescope and the 1.3-m
MONOPTEC's Fixed Shutter Dome
MONOPTEC licenses the Fixed Shutter Dome, an enabling technology in
observatory enclosures and satellite laser ranging systems. Four FSD's now
reside in Tokyo, Japan, as part of the Keystone Project.
MOnitoring X-ray Experiment
The MOnitoring X-ray Experiment (MOXE) is an X-ray all-sky monitor
to be launched on the Russian Spectrum-X-Gamma satellite. It will
monitor several hundred X-ray sources on a daily basis, and
will be the first instrument to monitor the complete X-ray
sky simultaneously. MOXE is built by Los Alamos Nat Lab,
Goddard Space Flight Center and Space Research Institute (Moscow).
Magellan Mission to Venus
NASA's Magellan spacecraft made a dramatic conclusion to its highly
successful mission at Venus when it is commanded to plunge
into the planet's dense atmosphere Tuesday, October 11, 1994. During
its four years in orbit around Earth's sister planet, the
spacecraft has radar-mapped 98 percent of the surface and collected
high-resolution gravity data of Venus. The purpose of the crash
landing is to gain data on the planet's atmosphere and
on the performance of the spacecraft as it descends. Up-to-date
status reports will be available from this WWW page, which
also offers Venus images and other highlights from the mission.
The Maidanak Foundation is dedicated to supporting the scientific teams
currently running the Mt. Maidanak Observatory, and to provide funding
for key scientific equipment.
Mauna Kea Observatories
INACTIVE LINK ? - 21 ---
Mauritius Radio Telescope
MRT is a southern sky survey telescope, which is making
a complimentary survey to 6C (southern sky) and observing selected
southern sky pulsars. See UK and original MRT
(University of Texas, Austin)
McDonald Observatory is located 450 miles west of Austin, Texas,
in the Davis Mountains. At present, there are three operating
telescopes: 2.7-meter, 2.1-meter, and .76-meter reflectors. The Observatory is equipped
with a wide range of state-of-the-art instrumentation for imaging and
spectroscopy in the optical and infrared, and it boasts one
of the first and most productive lunar ranging stations.
Mees Solar Observatory
Metsahovi Radio Research Station
The Metsähovi Radio Research Station, a separate research institute of
the Helsinki University of Technology since May 1988, operates a
14 m diameter radome enclosed radio telescope at Metsähovi, 40
km west of Helsinki, Finland. The Cassegrain telescope system can
be used at frequencies 10 - 230 GHz (wavelengths 3
cm - 1.8 mm).
Michelle: A mid-infrared spectrometer and imager for the UKIRT and Gemini telescopes
Michigan State's Telescope Initative
Outreach efforts to merge astronomy research and non-science education.
Microvariability and Oscillations of Stars
MOST is Canada's first space science microsatellite and its first
optical space telescope project, aiming for launch in late 2001.
MOST is designed to measure (as its acronym implies) Microvariability
& Oscillations of STars in broadband light with a precision
of a few micromagnitudes over timescales from minutes to days.
The resulting eigenfrequency data will be used primarily for stellar
seismology, to probe the structure and ages of Sun-like stars,
magnetic stars, Wolf-Rayet stars and halo subdwarfs. The subdwarfs are
expected to yield age estimates which would place a meaningful
lower limit on the age of the Universe. MOST should
also be capable of confirming the presence of giant extrasolar
planets identified in Doppler surveys.
Microwave Anisotropy Probe
NASA has selected MAP has one of the next MIDEX
missions. It will map the microwave background fluctuations over the
whole sky and provide insights into the formation of galaxies
and the basic parameters of cosmology.
Mid-InfraRed Large Imager
MIRLIN is a 128 x 128 pixel, 7 - 25
micrometer infrared astronomical camera built at JPL by a team
led by Dr. Michael Ressler and used on the Palomar
5 meter (200 inch) telescope, the NASA Infrared Telescope Facility
3 meter telescope, and the Keck II 10 meter telescope.
Midcourse Space Experiment
The MSX observatory is a Ballistic Missile Defense Organization project
which offers major benefits for both the defense and civilian
sectors. It was launched on a Delta II vehicle on
April 24, 1996, into a 900 km, polar, near-Sun synchronous
orbit. The spacecraft featured an advanced multispectral image capability to
gather data on test targets and space background phenomena.
The infrared sensors operated at 11 to 12 degrees Kelvin
by employing a solid hydrogen cryostat. The IR instruments span
the range 4.2 - 26 microns. The focal plane array
consists of five bands and the radiometer beam-size is more
than 25 times smaller than IRAS. As a result, much
greater spatial resolution than anything currently available has been obtained.
The cryogen phase of the mission ended on 26 February
1997. During the ten month cryogen phase of the mission
over 200 Giga Bytes of data on Celestial Backgrounds were
See the MSX Celestial Backgrounds Team
Home Page for additional details.
Millstone Hill Observatory
The Millstone Hill Observatory, located in Westford Massachusetts, is a
broad-based atmospheric sciences research facility owned and operated by the
Massachusetts Institute of Technology. The Atmospheric Sciences Group, which staffs
and manages the observatory, is a part of M.I.T's Haystack
Observatory, a basic research organization whose focus is radio wave
and radar science, instrumentation and techniques. The following resources may
be of interest. EISCAT is a particularly good source of
data and useful information. See, for example, incoherent scatter radar
and magnetosphere Millstone Hill Observatory: Information, data, etc., including real-time
radar status and data when the radar is operating. EISCAT:
European Incoherent Scatter Association. NCAR: National Center for Atmospheric Research.
NSF: National Science Foundation Gopher server. NASA: National Aeronautics and
Space Administration. NGDC: National Geophysical Data Center.
Mississippi State University - Howell Observatory
Molonglo Observatory Synthesis Telescope
The MOST consists of two cylindrical paraboloids, 778m x 12m,
separated by 15m and aligned East-West. A line feed system
of 7744 circular dipoles collects the signal and feeds 176
preamplifiers and 88 IF amplifiers. The telescope is steered by
mechanical rotation of the cylindrical paraboloids about their long axis,
and by phasing the feed elements along the arms. The
resulting `alt-alt' system can follow a field for +/- 6
hours (necessary for a complete synthesis with an East-West array)
only if the field is south of declination -30 degrees.
For fields near this limit the signal-to-noise ratio is considerably
lower for the first and last hour or so due
to the lower gain of the system at large `meridian
Monterey Institute for Research in Astronomy
The Monterey Institute for Research in Astronomy is a non-profit
astronomical observatory, founded in 1972 and dedicated to research and
education in astronomy.
Mount Evans Meyer-Womble Observatory
Mt.Evans Meyer-Womble Observatory, elev. 4,303 meters, in the Colorado Rockies.
Dual 0.7 meter R-C telescopes, optical and mid-infrared instrumentation. Summer
access. Collaborations invited.
Mount Graham International Observatory
The Mt. Graham International Observatory is located on Mt. Graham
near Safford , Arizona. Two telescopes are now in operation,
the Vatican Observatory/Arizona 1.8m Lennon telescope(VATT) and the 10m
diameter Heinrich Hertz Submillimeter Telescope (SMT), a joint project
of Arizona and the Max-Planck-Institut für Radioastronomie, Germany.
Mount Laguna Observatory
Mount Pleasant Radio Observatory
Mount Suhora Observatory
(Cracow Pedagogical University)
The Mt.Suhora Observatory is a part of Astronomy Department at
the Pedagogical University in Cracow, Poland. It is located in
Gorce mountain, near Koninki village, 60 km south-east of Cracow.
The scientific staff of 9 people works on photometry
of variable stars.
Mount Wilson Observatory
The mountain is host to several ongoing observing projects using
the onsite facilities. The observatory has two primary nighttime telescopes:
the 60-inch telescope, built in 1908 is home to the
HK Project and the Atmospheric Compensation Experiment; and the 100-inch
(Hooker) telescope, built in 1917, which is available to the
scientific community. Two solar observatories, the 60-foot tower telescope (operated
by USC), and the 150-foot tower telescope (operated by UCLA)
maintain long-term exploration of the magnetic activity behavior of the
Sun. There are also two interferometers onsite: the Infrared Spatial
Interferometer (ISI, operated by U.C. Berkeley), and the NRL Optical
Interferometer. The Telescopes in Education (TIE) Project operates a 24"
telescope, as well as the Snow Solar Telescope (built in
1904). Finally, a fully-robotic 32-inch Automatic Photoeletric Telescope (APT) is
operated by Tennessee State University.
Multi-Element Radio Linked Interferometer Network
(MERLIN - Jodrell Bank)
Multiband Imaging Photometer for SIRTF
The Multiband Imaging Photometer for SIRTF (MIPS) is a far-infrared
photometer, scheduled for launch into a solar orbit in December,
2001. It is one of three instruments that will fly
Multiple Mirror Telescope Observatory (1)
Multiple Mirror Telescope Observatory (2)
NFO's Automatic Radio Linked Telescope
Observatory associated with Western New Mexico University in Silver
City, NM (USA).
The Near Infrared Camera and Multi-Object Spectrometer (NICMOS) is a
second-generation instrument to be installed on the Hubble Space Telescope
(HST) during the February 13, 1997 on-orbit servicing mission. NICMOS
will provide infrared imaging and spectroscopic observations of astronomical targets
between 0.8-2.5 microns.
The Nançay Radio Observatory is a scientific department (the Unite
Scientifique de Nançay) of the Paris Observatory, and it is
also associated to the CNRS (the French National Scientific
Nasmyth Adaptive Optics System
(NAOS, ESO VLT)
Nation River Observatory
National Astronomical Observatory of Spain
OAN is a 200 year old institution devoted to research
in astronomy that operates several observatories. The Yebes Observatory is
the site of a mm-wave 14m telescope devoted to spectroscopy
and VLBI. A 1.5m optical telescope is located at the
Calar Alto Observatory. The OAN is also the Spanish partner
of IRAM, which runs a 30m mm-wave telescope and a
5x15m mm-wave interferometer.
National Centre for Radio Astrophysics
National Centre for Radio Astrophysics is the leading centre in
India for reseach in radio astronomy. It operates the Giant
Metrewave Radio Telescope(GMRT), one of the most powerful radio telescopes
in the world for radio astronomy at metre wavelengths.
National Laboratory for Astrophysics
LNA is an Institute of the National Council for Scientific
and Technological Development (CNPq). At present, LNA supports 3 telescopes:
the 1.6-m Ritchey-Chretien and coudé, the 0.6-m Cassegrain and the
0.6-m telescope of the University of São Paulo.
National Schools' Observatory
The National Schools' Observatory is a major web-based resource that
allows UK schools to use world-class astronomical telescopes sited all
around the world.
Using the resources and software developed by
the Observatory, students can prepare and carry out their own
astronomical research and share in the excitement of discovery.
National Solar Observatory
Synoptic Solar Magnetograms
National Solar Observatory / Sacramento Peak, Sunspot, NM
National Undergraduate Research Observatory
The National Undergraduate Research Observatory (NURO) at Lowell Observatory and
Northern Arizona University is a 0.8m telescope located on Anderson
Mesa south of Flagstaff, Arizona. NURO is a consortium of
Universities and small colleges to provide a research grade telescope
for undergraduate research and education.
Near-Earth Asteroid Tracking
NEAT is an autonomous celestial observatory located at the USAF/Ground-based
Electro-Optical Deep Space Surveillance (GEODSS) site on Haleakala, Maui, Hawaii.
It is designed to complete a comprehensive search of the
sky for near-Earth asteroids and comets.
Neutrino Oscillation MAgnetic Detector
Nomad (Neutrino Oscillation MAgnetic Detector) is CERN experiment WA96. The
experiment searches for the oscillation nu_mu -> nu_tau in the
CERN wide-band neutrino beam. It aims at detecting tau-neutrino charged-current
interactions by observing the production of the tau lepton through
its various decay modes by means of kinematical criteria.
New Radio Telescope Technologies Laboratory
NRRT Lab. of JSEC "Astronomy" in St.Petersburg, Russia. Current research:
Antenna testing and research, development of new antenna technologies for
radio telescopes including multielement feed arrays, MMIC focal receiver arrays,
active phased arrays for radio telescopes. Development, investigation and introduction
of new observation modes at RATAN-600 radio telescope.
Next Generation Space Telescope
The Next Generation Space Telescope (NGST) is a critical component
of NASA's Origins Program. It will be a telescope of
aperture greater than 4m, radiatively cooled to 30 - 60
deg.K, permitting extremely deep exposures at near infrared wavelengths with
a 10 year life. A key requirement is to break
the HST cost paradigm through the use of new technology
and management methods. This site is designed to serve as
the starting point for finding online NGST Study documentation.
There is also a public home page at NASA,
and a European site at ST-ECF.
Next Generation Space Telescope listservs
This URL takes you to a WWW page where you
can subscribe to a number of listservs devoted to the
Next Generation Space Telescope project. You may subscribe to any
of them. Posting is restricted. Right now, these are used
as ways to inform the community about progress in the
project. The web site contains links for feedback to the
project team members.
Nobeyama Radio Observatory, NAOJ
Information regarding the 45-m Telescope, the Millimeter Array(NMA), the Large
Millimeter and Submillimeter Array (LMSA) project, and much more.
Nordic Optical Telescope
(NOT, La Palma)
Noto VLBI Station
Oak Ridge Observatory
The Observatoire Midi-Pyrénées (OMP) is an Observatoire des Sciences de
l'Univers placed under the administrative supervison of both the Institute
des Sciences de l'Univers (INSU) of the French National Center
for Scientific Research (CNRS) and the Ministry of Research, Technology
and Education. It has laboratories located on the Rangueuil campus
of Université Paul Sabatier in Toulouse (UPS), in Bagnères, Lannemezan
and on the summit of Pic du Midi de Bigorre.
Observatoire de Haute-Provence
The Observatoire de Haute-Provence (OHP) is an optical observatory in
southeast France offering small and medium-sized observing facilities to astronomers
in France, Europe and abroad. Includes information about instruments and
Observatoire du Mont Megantic
The Centre de recherche Observatoire du mont Mégantic (OMM) is
an inter-university collaborative organisation which brings together researchers from Université
de Montréal, Université Laval, with axis centred on the télescope
du mont Mégantic (TMM).
The Centre unites most of
the professional researchers working in astronomy and astrophysics in Québec.
Observatoire du Mont Mégantic
Observatorio Astronómico Nacional
The Observatorio Astronómico Nacional (OAN) operates 3 telescopes (2.1m, 1.5m,
and 0.84m) up in the mountains of the Sierra San
Pedro Martir of Baja California. The observatory offices and workshops
are located in Ensenada, B.C. overlooking the Pacific ocean. OAN
is a part of the Instituto de Astronomía of the
Universidad Nacional Autónoma de México.
Observatorio Nacional, Brazil
(Rio de Janeiro)
Observatorium Hoher List
The Wide Field Imager for the VST at Paranal.
Onsala Space Observatory
OSO is the Swedish National Facility for Radio Astronomy.
Optical Correctors for Liquid Mirror Telescopes
One of the often cited limitations of liquid mirror telescopes
pertains to the small region of sky which they can
observe. Because the aberrations of a parabola increase rapidly with
field angle, classical corrector designs cannot yield subarcsecond images for
angles significantly greater than one degree. To access larger fields,
innovative corrector designs must be explored.
In these pages we
discuss the Optical Design and Testing of a family of
two-mirror correctors to compensate the aberrations of a fixed parabolic
mirror observing at a large angle from the zenith.
Orbiting Very Long Baseline Interferometry
Owens Valley Radio Observatory
Planck is the third Medium-Sized Mission (M3) of ESA's Horizon
2000 Scientific Programme. It is designed to image the anisotropies
of the Cosmic Background Radiation Field over the whole sky,
with unprecedented sensitivity and angular resolution. Planck will provide a
major source of information relevant to several cosmological and astrophysical
issues, such as testing theories of the early universe and
the origin of cosmic structure.
Planck was formerly called
COBRAS/SAMBA. After the mission was selected and approved, it was
renamed in honor of the German scientist Max Planck (1858-1947),
Nobel Prize for Physics in 1918.
Palomar Testbed Interferometer
Public Observatory located in Deleware, Ohio, USA. Offers public programs
almost every weekend. Owned and operated by the Ohio Wesleyan
Perugia University Astronomical Observatory
Articles, data, researches, and new developments at Perugia University Astronomical
Pine Mountain Observatory
(University of Oregon)
Pushchino Radioastronomy Observatory (PRAO)
Pushchino Radioastronomy Observatory of Astro Space Center of P.N.Lebedev Physical
Institute (PRAO ASC LPI).
Roentgen Satellite (X-ray satellite) operated by the Max-Planck-Institut
für Extraterrestrische Physik (MPE), Garching, Germany.
ROSAT Guest Observer Facility
The ROSAT Science Data Center (RSDC) is responsible for execution
of the guest investigator program, including such activities as providing
assistance in the preparation of proposals, the receiving, processing, and
distributing ROSAT pointed data, and providing facilities for the scientific
analysis of these data.
(ROSAT at GSFC. NASA)
ROSAT, the ROentgen SATellite, is an X-ray observatory developed through
a cooperative program between the Germany, the United States, and
the United Kingdom. The satellite was designed and is operated
by Germany, and was launched by the United States on
June 1, 1990.
RXTE Guest Observer Facility
Radio Ice Cherenkov Experiment
A prototype ultra-high energy neutrino detector/obervatory located at the South
Pole. RICE consists of an array of radio antennas buried
deep in the ice which detect coherent Cherenkov emission from
electromagnetic cascades produced as a by product of ultra-high energy
RadioAstron is a project led by the Astro Space Center
of the Lebedev Physical Institute in Moscow, Russia, that will
put a 10-meter radio telescope into a high elliptical orbit
in order to make VLBI observations in conjunction with radio
telescopes on the ground. It is part of the Spectrum
series of spacecraft, also including Spectrum X-Gamma and Spectrum-UV.
Robotic Lunar Observatory
The Robotic Lunar Observatory (ROLO) is dedicated to studying one
of the remaining unknowns of the Moon: what is its
precise brightness? ROLO is currently part of the NASA Earth
Observing Spacecraft Mission. The concept of the project is that
the Moon will be observed repeatedly, and data gathered, so
that we can predict the brightness of the Moon to
better than two percent. Then, spacecraft orbiting the Earth can
look at the Moon as part of a calibration sequence
to get an absolute brightness reference.
Robotic Optical Transient Search Experiment
ROTSE is an experimental program to search for astrophysical optical
transients on time scales of a fraction of a second
to a few hours. This is an area of astronomical
science that has been relatively unexplored until now. The primary
incentive for this research is to find the optical counterparts
of gamma-ray bursts (GRBs). Two sets of instruments are now
under construction: ROTSE-I, a 4-fold camera array using telephoto lenses
to cover a 16 degree by 16 degree field of
view and ROTSE-II, a pair of 0.45 meter aperture telescopes
to cover a 2 degree by 2 degree field of
view. The expected sensitivities of these two systems is expected
to be m_v ~ 15 and 18 respectively.
Rossi X-Ray Timing Explorer Project
The Rossi X-ray Timing Explorer is designed to facilitate the
study of time variability in the emission of X-ray sources
with moderate spectral resolution.
Royal Observatory, Edinburgh
This site offers information about the extensive activities of the
Royal Observatory, Edinburgh, a PPARC establishment responsible for building common-user
IR and sub-mm instrumentation and managing telescope sites and data
archive resources, as well as the UK Schmidt Telescope and
the SuperCOSMOS measuring machine. The ROE site also has links
to, or acts as the home page for:
and much more
Institute for Astronomy, University of Edinburgh;
- latest research
- the Crawford library;
- the ROE Visitor Centre;
- the UKIRT data archive;
- Public Understanding of Science;
- ROE Photolabs;
- Teacher Research Inititive
SAtellite for Measurement of cosmological Background Anisotropies
SAMBA will use bolometers to survey the sky in the
0.3-6mm wavelength range. The project has been selected by ESA
for a merging with the COBRAS proposal, which gives the
COBRAS/SAMBA mission, now named PLANCK.
STellar Astrophysics & Research on Exoplanets
STARE (STellar Astrophysics & Research on Exoplanets) uses precise time-series
photometry to search for extrasolar giant planets transiting their parent
stars. An important byproduct of STARE will be an unusually
complete survey of variable stars within its selected fields-of-view.
SUBARU astronomical observatory
Japan national optical-infrared telescope at the summit of Mauna Kea.
The site includes astrophotographs from Subaru.
Santiago de Compostela - Astronomical Observatory Ramón María Aller
(Amateur High Speed Stellar Photometry)
Schaller Observatory is dedicated to high speed stellar photometry and
optical SETI. The site describes the observatory, computer controlled telescope.
photomultiplier tube detector, amplifiers, filters, data acquisition and FFT analysis.
Schmidt telescope at Observatoire de la Cote d'Azur
The Telescope is located at the "Observatoire de Calern", above
the city of Grasse.
Equipped with a 2K CCD
camera, it is mainly used for the OCA-DLR Asteroid Survey
program. It is also used for geostationnaary Space Debris detection
and GRB optical counterparts follow ups.
SciTech Astronomical Research
(STAR Research Telescopes)
Design and manufacture specialized and general purpose telescopes and instrumentation
for research and education.
NASA's Small Explorer (SMEX) program provides frequent flight opportunities for
highly focused and relatively inexpensive science missions.
Soft X-Ray Telescope onboard Yohkoh Satellite, ISAS, Japan
(description at LMSAL, USA)
Yohkoh (" Sunbeam" in Japanese) is a satellite of the
Japanese Institute of Space and Astronautical Science (ISAS) dedicated to
high-energy observations of the Sun, specifically of flares and other
Solar Extreme-ultraviolet Rocket Telescope and Spectrograph
The Solar Extreme-ultraviolet Rocket Telescope and Spectrograph (SERTS) instrument obtains
spatially resolved spectra and spectroheliograms over a wide range of
extreme ultraviolet (EUV) wavelengths characteristic of temperatures between 5x10^4-3x10^7K, providing
information about the Sun's corona and upper transition region. Wavelength
coverage is 170-450A with spectral resolution near 10000, spatial resolution
as good as 5arcsec, and relative photometric accuracy within +/-
20% over most of its range. This page contains links
to information about the instrument, a solar EUV line list
between 170 and 450 A from the SERTS-89 flight, and
a list of SERTS-related publications. Soon to be added is
information about upcoming launches. Also included are links to other
WWW servers relevant to solar astronomers.
Solar Group of RATAN-600
The group provides Solar Radio Monitoring on RATAN-600. Observations are
performed with a high spatial, one - dimensional resolution scan
near UT 9-00 at 30-40 wavelengths in the range from
1.67 cm up to 32 cm with left (LCP) and
right (RCP) circular polarization.
There are FITS and GIF
data archives available from May 1997.
Solar Tower Atmospheric Cherenkov Effect Experiment
STACEE is a new experiment for detecting gamma-rays with energies
from 20 to 300 GeV, corresponding to the last unopened
window in the electromagnetic spectrum. STACEE will use a the
heliostats available at a large solar power facility to collect
Cherenkov light that results from gamma-ray air showers. STACEE is
currently under development and should be operational sometime in 1997
Solar and Heliospheric Observatory
The SOHO project is being carried out by the European
Space Agency (ESA) and the US National Aeronautics and Space
Administration (NASA) as a cooperative effort between the two agencies
in the framework of the Solar Terrestrial Science Program (STSP).
SOHO was launched on December 2, 1995. The SOHO
spacecraft was built in Europe by an industry team led
by Matra, and instruments were provided by European and American
South African Astronomical Observatory
The South African Astronomical Observatory (SAAO) is the National Facility
for optical/infrared astronomy in South Africa. Its prime function is
to further fundamental research in astronomy and astrophysics at a
national and international level through the provision and use of
a world-class astronomical facility.
Southeastern Association for Research in Astronomy
The SARA telescope consortium operates the 0.9 meter SARA optical
telescope on Kitt Peak.
Southern African Large Telescope
SALT, a 9-m class southern hemisphere twin of the Hobby-Eberly
Telescope (HET) in Texas, to be built at the Sutherland
observing station of the South African Astronomical Observatory.
Southern Columbia Millimeter Telescope
Space Infrared Telescope Facility
The Space InfraRed Telescope Facility (SIRTF), the fourth and final
element in NASA's family of "Great Observatories", has entered development.
SIRTF consists of a 0.85-meter telescope and three cryogenically-cooled science
instruments capable of performing imaging and spectroscopy in the 3
- 180 micron wavelength range. Incorporating the latest in large-format
infrared detector arrays, SIRTF offers orders-of-magnitude improvements in capability over
existing programs. While SIRTF's mission lifetime requirement remains 2.5 years,
recent programmatic and engineering developments have brought a 5-year cryogenic
mission within reach. A fast-track development schedule will lead to
a launch in December 2001. SIRTF represents an important scientific
and technical bridge to NASA's new Origins program.
Space Infrared Telescope Facility (SIRTF) - Infrared Spectrograph
The Infrared Spectrograph (IRS) is one of three instruments to
be flown in the Space Infrared Telescope Facility (SIRTF).
Space Interferometry Mission
SIM will be NASA's first space interferometer designed specifically for
measuring the position of stars. SIM will utilize multiple telescopes
placed along a 10-meter (33-foot) structure.
Special Astrophysical Observatory of Russian Academy of Sciences
SAO is Russia's main centre for ground-based space research. The
Observatory is located in the South of Russia, in the
Caucasus mountains of Karachaevo-Cherkesia. The basic instruments of the Observatory
are the 6-meter optical telescope BTA (Big Alt-azimuth Telescope) and
the 600-meter radio telescope RATAN-600.
SPECTRUM UV is planned as a general purpose ultraviolet observatory.
Phase A study activities are supported by the Space Agencies
of Russia, Ukraine, Italy and Germany. Spectrum UV is planned
to be launched round the turn of the century.
Spectrum-X-Gamma Coordination facility
(SXG. University of Harvard)
Spectrum-X-Gamma (SXG) is an international high-energy astrophysics observatory which is
being built under the leadership of the Russian Space Research
Institute (IKI). The US SXG CF supports the US astronomical
community in obtaining information about SXG, proposing for and making
SXG observations, and performing archival research using the SXG archive
Square Kilometer Array Interferometer radio telescope project
This site provides information about the world-wide efforts to develop
the next generation of radio telescope.
Square Kilometre Array
(SKA - Australian contribution)
A web resource covering SKA scientific and engineering developments. Contains
access to reports, meetings announcements, discussions of SKA issues, links
to SKA related research.
Stardial:an autonomous astronomical camera on the World Wide Web
Stardial delivers images of the night sky nearly in real-time
to the world wide web. It is used primarily for
educational purposes. Its archive consists of images taken at 15
minute (sidereal) intervals since July 1996. The survey covers from
0 to -8 degrees declination to 12th magnitude. Highlights and
possible classroom assignments are described.
A space mission that will fly close to a comet
and, for the first time ever, bring cometary material back
Stephen F. Austin State University Observatory
Facilities, research, and personnel of the SFASU Observatory.
The Steward Observatory Home Page provides information on the academic
and research activities of the University of Arizona Department of
Astronomy as well as information on the facilities of Steward
Stratospheric Observatory For Infrared Astronomy
The Stratospheric Observatory For Infrared Astronomy (SOFIA) will be a
2.5 meter, optical/infrared/sub-millimeter telescope mounted in a Boeing 747, to
be used for many basic astronomical observations performed at stratospheric
altitudes. The Facility will accommodate installation of different focal plane
instruments, with in-flight accessibility, provided by investigators selected from the
international science community. The Facility objective is to have an
operational lifetime in excess of 20 years.
Subaru Telescope at Hilo
The SUBARU is an 8.3-m diameter new-generation telescope being constructed
and to be operated by the National Astronomical Observatory, under
the Ministry of Education of Japan.
The Submillimeter Array (SMA), now under construction near the summit
of Mauna Kea, was conceived as an
exploratory instrument for high angular resolution observations at submillimeter wavelengths
(1.3 to 0.3 mm).
Submillimeter Polarimeter for Antarctic Remote Observing
Mapping Interstellar Magnetic Fields from the South Pole.
Submillimeter Receiver Laboratory
Submillimeter Telescope Observatory
The Submillimeter Telescope Observatory (SMTO) is operated as a joint
facility for the University of Arizona's Steward Observatory and the
Max-Planck-Institut für Radioastronomie (Bonn). The SMTO is located on Emerald
Peak of Mt. Graham, approximately 75 miles north-east of Tucson,
Submillimeter Wave Astronomy Satellite
SWAS, the Submillimeter Wave Astronomy Satellite, is a pathfinding mission
for studying the chemical composition of interstellar galactic clouds to
help determine the process of star formation.
Submillimetre Common-User Bolometer
Array for the James Clerk Maxwell Telescope
SCUBA is a bolometer camera for the James Clerk Maxwell
Telescope operating at submillimetre and millimetre wavelengths.
Sudbury Neutrino Observatory
(SNO at Queen's University)
SNO is an astronomical neutrino observatory that is being built
below ground in the deepest section of INCO Limited's Creighton
Mine near Sudbury, Ontario. SNO is an international collaboration of
scientists from Canada, USA and UK. Information services are available
Super-Kamiokande is a joint Japan-US collaboration to construct the world's
largest underground neutrino observatory.
Junction Detector Research
Such devices promise to yield the near-ideal astronomical photon-counting detector
in which not just the location, but also the energy
of each photon is recorded at extremely high efficiency. STJ
detectors have previously been considered mainly for X-ray astronomy applications,
but recent theoretical and laboratory research in the division has
led to a dramatic breakthrough in extending the technique to
visible and UV wavelengths where energy discrimination up until now
has had to rely on filters or low efficiency dispersive
Swedish-ESO SUbmillimetre Telescope
Swift Gamma Ray Burst Explorer
Swift is a three-telescoipe space observatory (gamma-ray telescope, X-ray telescope,
and ultraviolet/optical telescope) for studying gamma ray bursts. It is
a NASA MIDEX mission selected for launch in 2003.
Sydney University Molonglo Sky Survey
SUMSS is a deep radio survey of the entire sky
south of declination -30 degrees, made using the Molonglo Observatory
Synthesis Telescope, operating at 843MHz and recording right-circular polarization.
SUMSS matches (approximately) the resolution and depth of the NRAO-VLA
Sky Survey (NVSS). The principal data products are mosaics which
cover a 4x4 degree square on the sky. The centres
of the mosaics mirror the NVSS centres in the north.
The resolution is 45" x 45"/sin(dec), and the rms noise
limit varies from 1.3 to 2mJy/beam (lower toward the south
The survey began in March 1997 and
will take eight years to complete. SUMSS is suported by
funding from the Australian Research Council.
The primary reference
for a description of the survey is: Bock, D.,
Large, M. and Sadler, E.
THEMIS - Heliographic Telescope for the Study of the Magnetism and Instabilities on the Sun
THEMIS (Télescope Héliographique pour l'Etude du Magnétisme et des Instabilités
Solaires) is a new generation Franco-Italian solar telescope built by
INSU/CNRS (France) and CNR (Italy). The main
scientific goal for which it has been designed is the
accurate determination of the vector magnetic field.
Taeduk Radio Astronomy Observatory
Taeduk Radio Astronomy Observatory (TRAO) is part of the Korea
Astronomy Observatory, which is operated under a cooperative agreement with
the Ministry of Science and Technology.
Telescope Array Project
A project of ground-based detector for Astrophysics.
Telescope a Action Rapide pour les Objets Transitoires
TAROT is an automatic, autonomous observatory whose first objective is
the real-time detection of optical transient counterparts of cosmic gamma
Telescopio Infrarosso del Gornergrat
Italian national 1.5m telescope optimized for infrared observations, operated by
Telescopio Nazionale Galileo - Italian National Telescope Galileo
(TNG, La Palma)
The Telescopio Nazionale Galileo is the national facility of the
Italian astronomical community, set in the Canary island of La
Palma (Spain). The Astronomical Observatory of Padova had the
responsibility of its construction through the TNG Project Office.
Tennessee State University 2-m Automatic Spectroscopic Telescope Project
This site details development of an 80-inch automatic telescope that
Tennessee State University is developing for high-dispersion spectroscopy. It includes
engineering reports and extensive pictures of the instrument.
Terrestrial Planet Finder
(Origins of Stars, Planets, and Life)
The Terrestrial Planet Finder (TPF) is a key element of
NASA Origins Program. It will study all aspects of planets:
from their formation and development in disks of dust and
gas around newly forming stars to the presence and features
of those planets orbiting the nearest stars; from the numbers
at various sizes, and places to their suitability as an
abode for life. By combining the high sensitivity of space
telescopes with the sharply detailed pictures from an interferometer, TPF
will be able to reduce the glare of parent stars
by a factor of more than one hundred-thousand to see
planetary systems as far away as 50 light years.
Thueringer Landessternwarte Tautenburg
The observatory is running a 2m telescope which can be
used in three different optical configurations: Schmidt telescope Cassegrain telescope
Torun Radio Astronomy Observatory
Torun Radio Astronomy Observatory (TRAO), now part of Torun Centre
for Astronomy is an educational and research facility of the
Nicolaus Copernicus University, Faculty of Astronomy and Physics, Torun, Poland.
The Observatory main instrument is 32m modern design radio telescope
usable up to 50 GHz. Presently equipped with cooled receivers
for L and C bands is used extensively for VLBI,
pulsar timing and spectroscopy. Since April 1998 Torun is the
full member of the EVN.
Transition Region And Coronal Explorer
TRACE will enable solar physicists to study the connections between
fine-scale magnetic fields and the associated plasma structures on the
Sun in a quantitative way by observing the photosphere, transition
region, and corona.
U.S. Space Very Long Baseline Interferometry Project
(U.S. Space VLBI)
This project supports the VSOP (VLBI Space Observatory Programme) mission
led by the Institute of Space and Astronautical Science in
Japan, and the RadioAstron mission led by the Astro Space
Center of the Lebedev Physical Institute in Russia. VSOP is
scheduled for launch in September 1996, while RadioAstron is scheduled
for launch in 1997. Each mission involves an orbiting 8-10
meter radio telescope dedicated to astronomical radio interferometry experiments using
baselines formed between the spacecraft and a number of ground
radio telescopes. A variety of information is now on line,
describing the JPL Project, each of the space missions, and
the science goals of the missions.
UK Infra-Red Telescope
UK Schmidt Telescope
The initial task of the UKST was to construct a
photographic survey of the entire southern sky. The telescope still
takes some 700 plates a year - about half for
current surveys and the remainder taken at the request of
research astronomers around the world. To date the UKST has
taken over 17,000 plates, the plates are stored in the
Plate Library at the Royal Observatory, Edinburgh (ROE) and represent
a huge source of data for the astronomical community. Some
300 active research programmes make use of UKST plate material.
Many plates are copied in the ROE Photolabs and sold
as Sky Atlases or Teaching Packages. In addition to its
photographic role the UKST also has a multi-object fibre spectroscopy
system known as FLAIR. e-mail firstname.lastname@example.org
UK Schmidt Telescope - Anglo-Australian Observatory
(UKST / AAO)
Uhuru was the first earth-orbiting mission dedicated entirely to celestial
X-ray astronomy. It was launched on 12 December 1970 into
an orbit of about 560 km apogee, 520 km perigee,
3 degrees inclination, with a period of 96 minutes. The
mission ended in March 1973.
INACTIVE LINK ? - 40 ---
Ultraviolet Imaging Telescope
(UIT. GSFC. NASA)
The UIT is a 38-cm Ritchey-Chretien telescope equipped for ultraviolet
filter and grating imagery over a 40 arcminute field of
view. It contains two detector systems: one in the far
UV and one in the near UV. The UIT flew
onboard the Space Shuttle Columbia as part of the Astro
1 payload. The UIT's second flight took place in 1995
onboard the Space Shuttle Endeavor as part of the Astro
The Ulysses Mission is the first spacecraft to explore interplanetary
space at high solar latitudes. Ulysses is a joint endeavor
of the European Space Agency (ESA) and the National Aeronautics
and Space Administration (NASA) of the USA. Instruments include: Magnetometer
(VHM/FGM), Solar Wind Plasma Experiment (SWOOPS), Solar Wind Ion Composition
Instrument (SWICS), Unified Radio and Plasma Wave Instrument (URAP), Energetic
Particle Instrument (EPAC), Low-Energy Ion and Electron Experiment (HISCALE), Cosmic
Ray and Solar Particle Instrument (COSPIN), Solar X-ray and Cosmic
Gamma-Ray Burst Instrument (GRB)
University of Bradford - Robotic Telescope
The engineering in astronomy Team in the Department of
Industrial Technology are currently working on low-cost fully-robotic telescopes.
University of California Observatories - Lick Observatory (WWW)
Lick Observatory Anonymous ftp
University of California, Irvine, Observatory
The University of California, Irvine, Observatory is located on campus.
It consists of a computer-controlled telescope with a 24-inch primary
mirror and numerous other portable telescopes. The instruments on the
primary telescope include CCD cameras and a spectrograph. The Observatory
is used primarily for undergraduate astronomy classes. In addition, Visitor
Nights open to the general public are held quarterly, and
special tours for community groups can be arranged.
University of Denver Astronomy
Mt.Evans Meyer-Womble Observatory located at 14,124 feet above sea level,
on Mt.Evans in the Front Range of Colorado, used for
infrared astronomy research.
University of Hawaii IfA: 2.2m Telescope
University of Louisville - Moore Observatory
Moore Observatory is located in the Horner Wildlife Sanctuary near
Louisville, KY. A computer-controlled 0.5 meter telescope, fiber optically coupled
spectrograph, and wide field spectral imaging camera are used there
to investigate physical processes in comets and low surface brightness
emission nebulae. This resource describes the observatory and its environs,
and provides a link to astrophysics research at the University
University of Toronto Southern Observatory
UTSO operates the 60cm Helen Sawyer Hogg Telescope located on
Cerro Las Campanas in north-central Chile. This homepage provides information
useful to potential users and others interested in our facility.
The VIRMOS project aims to deliver 2 spectrographs for the
ESO- VLT . VIMOS is a visible imaging spectrograph with
outstanding multiplex capabilities, allowing to take spectra of more than
800 objects simultaneously (10 arcsec slits), or spectroscopy of all
objects in a 1x1 arcmin2 area. NIRMOS is a near-infrared
imaging spectrograph with a multiplex of 180 (10 arcsec slits),
and allows spectroscopy of all objects in a 30x30 arcsec2
area. Together VIMOS and NIRMOS allow to get spectroscopy from
0.37 to 1.8 microns, with unsurpassed efficiency for large surveys.
VLBI Antenna at Radio-Observatorio Espacial do Nordeste
Site of Fortaleza, Brazil.
VLBI Space Observatory Programme
The VSOP (VLBI Space Observatory Programme) mission is led by
the Institute of Space and Astronautical Science, in collaboration with
the National Astronomical Observatory of Japan. The first VSOP satellite
was successfully launched 12 February 1997 on the new ISAS
M-V rocket from the Kagoshima Space Center. The satellite, renamed
HALCA after its successful launch, sucessfully deployed an 8 meter
diameter radio telescope in orbit on 27 & 28 February
1997. HALCA is in an elliptical Earth orbit, with an
apogee height of 21,000km and a perigee height of 560km,
which enables VLBI (Very Long Baseline Interferometry) observations on baselines
up to three times longer than those acheivable on Earth.
VLT Mid Infrared Imager Spectrometer
(VISIR, ESO VLT)
VLT Survey Telescope
The VST project is a cooperation between the European Southern
Observatory (ESO) and the Capodimonte Astronomical Observatory (OAC) for the
study, design and construction of a wide field alt-az telescope
of 2.6 m aperture, specialized for high quality astronomical imaging
to be installed and operated on Cerro Paranal, next to
ESO's Very Large Telescope (VLT).
Ventspils International Radioastronomy Centre
The Ventspils 32-m antenna is the biggest in the Baltics.
The main purpose of the VIRAC is to take part
in observations at high angular resolution of faint sources of
cosmic natural and artificial radiation in order to accumulate observational
data for fundamental and practical research programmes in radioastronomy, astrophysics,
cosmology, geophysics, geodynamics, geodesy, co-ordinate-time service and other.
Very Large Array
Very Large Telescope Project
ESO is building what will be the World's largest optical
telescope array, The Very Large telescope (VLT).
Very Large Telescope will consist of four 8-meter telescopes which
can work independently or in combined mode. In this latter
mode the VLT provides the total light collecting power of
a 16 meter single telescope, making it the largest optical
telescope in the world. The four 8-m telescopes supplemented with
3 auxilliary 1 m telescopes may also be used in
interferometric mode providing high angular resolution imaging. The useful wavelength
range extends from the near UV up to 25 microns
in the infrared.
Very Long Baseline Array
Very Small Array
The Very Small Array is an interferometer array designed to
make images of the cosmic microwave background (CMB) radiation on
angular scales around one degree. The VSA consists of an
array of 14 small antennas, working at a frequency in
the range 26-36 GHz, and will be sited at the
Teide Observatory in Tenerife.
The purpose of the Virgo interferometer is to detect arrival
of gravitational waves on earth from astronomical sources.
Visible and Infrared Survey Telescope for Astronomy
VISTA is the Visible and Infrared Telescope for Astronomy: a
4-m Wide Field Survey telescope for the Southern Hemisphere, being
built at Cerro Paranal, close to ESO VLT, by a
consortium of 18 UK universities.
Vulcan Camera Project
The Vulcan Camera Project, sponsored by NASA Ames Research Center,
is designed to detect transits of large extrasolar planets using
differential photometry. Vulcan uses a 15cm aperture refactor at Lick
Observatory to image a wide field in which ~6000 stars
are monitored for two months, in a search for the
~1% transit signal expect from a 51 Pegasi-type planet. Vulcan
is a ground-based test-bed for the proposed Kepler Mission to
detect Earth-sized exoplanets.
WAVES : The Radio and Plasma Wave Investigation on the WIND Spacecraft
WAVES radio astronomy instrument on the ISTP-Wind spacecraft.
WFCAM - Wide Field Camera
WFCAM is an IR wide field camera for the UK
Infrared Telescope on Mauna Kea. WFCAM will be operational as
an IR imaging survey instrument in late 2002. The camera
has been designed to maximize survey speed at J, H
and K while retaining excellent image quality.
WIYN, from Indiana University
INACTIVE LINK ? - 20 ---
Warren Rupp Observatory
Astronomical Research, Digital Imaging, Comet Search, Planetary observation, Deep sky
photography, Education. 31" F7 Telescope with computer drive in 35ft
dome. Lots of nice facilities. CCD stuff, Chemical photography. Free
access to qualified student, university, profesionals and amateurs.
Westerbork Synthesis Radio Telescope
(WSRT - NFRA)
The Westerbork Synthesis Radio Telescope is a linear 3 kilometer
array located near the village of Westerbork in the North-East
of the Netherlands. The WSRT consists of fourteen 25m dishes
along a perfect east-west line. By combining these fourteen elements
one can synthesize a radio telescope with a diameter of
Whole Earth Blazar Telescope
The WEB Telescope (WEBT) is a network of optical observers
who in concert have the capability to obtain continuous, high-temporal-density,
optical monitoring of blazars.
Whole Earth Telescope
(WET, site of University of Texas at Austin)
The Whole Earth Telescope (WET) is a collaboration of astronomers
who observe variable stars (white dwarfs and Delta Scuti stars)
and cataclysmic variables Typically twice a year, we coordinate a
global time-series photometry campaign at ~10 observatories worldwide such that
our target objects are visible from the night side of
the planet 24 hours a day
Whole Earth Telescope
In 1986, astronomers from the University of Texas established a
world--wide network of cooperating astronomical observatories to obtain uninterrupted time--series
measurements of variable stars. The technological goal was to resolve
the multi-periodic oscillations observed in these objects into their individual
components; the scientific goal was to construct accurate theoretical models
of the target objects, constrained by their observed behavior, from
which their fundamental astrophysical parameters could be derived. This approach
has been extremely successful, and has placed the fledgling science
of stellar seismology at the forefront of stellar astrophysics.
Wide Field Infrared Explorer
This is the website for NASA's Wide Field Infrared Explorer
(WIRE). The primary purpose of WIRE was a four month
infrared survey of the universe, focusing specifically on starburst galaxies
and luminous protogalaxies.
On 29 Mar 1999, the WIRE
mission has been declared a loss.
Wilcox Solar Observatory
The Wilcox Solar Observatory began daily observations of the Sun's
global magnetic field in May 1975, with the goal of
understanding changes in the Sun and how those changes affect
the Earth; this is now called space weather. Now low-resolution
maps are also made of the Sun's magnetic field each
day, as are observations of solar surface motions. The observatory
is located in the foothills just west of the Stanford
Robotic observatory for small telescopes located in southeastern Arizona hosting
telescopes from other institutions for a fee. See our Web
site for details. Our own scientific interests are NEO's and
minor planet astrometry and photometry.
Wisconsin Ultraviolet Photo-Polarimeter Experiment
The Wisconsin Ultraviolet Photo-Polarimeter Experiment (WUPPE) was a pioneering effort
to explore polarization and photometry in the ultraviolet (UV) spectrum.
It was the first and most comprehensive effort to exploit
the unique powers of polarimetry at wavelengths not visible on
Earth. The instrument was designed and built at the University
of Wisconsin Space Astronomy Laboratory in the 1980's. WUPPE flew
on two NASA Space Shuttle missions: ASTRO-1 and ASTRO-2.
Wolfgang-Amadeus, The University of Vienna Twin Automatic Photoelectric Telescope
We operate two robotic 75-cm telescopes for photoelectric photometry at
Fairborn Observatory in the Sonoran desert near Tucson, Arizona. Not
only are the telescopes automatic, but the observatory itself is
automatic. A site-control computer monitors weather sensors, operates the observatory
roof, and provides a nightly report to the observatory staff,
who are located in Vienna, Austria.
Wyoming Infrared Observatory
X-Ray Timing Explorer
The Rossi X-ray Timing Explorer is a Goddard mission which
was launched on December 30th, 1995. RXTE is designed to
facilitate the study of time variability in the emission of
X-ray sources with moderate spectral resolution. Time scales from microseconds
to months are covered in an instantaneous spectral range from
2 to 250 keV. It is designed for a required
lifetime of two years, with a goal of five years.
The European Space Agency's X-ray Multi-Mirror satellite is the most
powerful X-ray telescope ever placed in orbit. It has an
unprecedented sensitivity and the mission will help solve many cosmic
mysteries, ranging from enigmatic black holes to the formation of
XMM-Newton Science Operations Centre
ESA s X-ray Multi Mirror mission XMM-Newtion is the second
Cornerstone in ESA's Long Term Scientific Programme. With a large
collecting area of its mirrors and the high sensitivity of
its cameras, XMM-Newton is expected to increase radically our understanding
of high-energy sources - clues to a mysterious past, and
keys to understanding the future of the Universe.
(University of Chicago)
Yerkes Observatory in Williams Bay Wisconsin hosts the 40" refractor,
a 41" reflector, a 24" Boller & Chivens reflector, a
10" educational telescope, and support facilities. The 41" telescope is
used for research including adaptive optics studies.
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