AstroWeb: Ultraviolet Astronomy
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ASTRO Observatory
(ASTRO-1 and ASTRO-2)
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The ASTRO Observatory had three primary instruments: the Ultraviolet Imaging
Telescope (UIT), the Hopkins Ultraviolet Telescope (HUT) and the Wisconsin
Ultraviolet Photo-Polarimeter Experiment (WUPPE). The first Astro flight was on
December 2-11, 1990. The X-ray experiment Broad Band X-Ray Telescope
(BBXRT) was also part of the Astro-1 flight. The second
flight was on March 2-18, 1995.
- http://archive.stsci.edu/astro/
- Categories: telescope space ultraviolet
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Advanced Camera for Surveys
(ACS)
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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.
- http://adcam.pha.jhu.edu/
- Categories: telescope infrared optical space ultraviolet
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Array of Low Energy X-ray Imaging Sensors
(ALEXIS)
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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.
- http://alexis-www.lanl.gov/
- Categories: telescope high_energy space ultraviolet
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Astronomical Data Center
(ADC)
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The Astronomical Data Center (ADC), at NASA Goddard Space Flight
Center, Greenbelt, Maryland, is a cooperative effort between the National
Space Science Data Center (NSSDC)/ World Data Center A for
Rockets and Satellites (WDC-A-R&S) and its parent organization, the Space
Science Data Operations Office . Currently, the ADC archives hold
more than 670 catalogs of astrometry, photometry, spectroscopy, radio, and
other miscellaneous data for stellar and nonstellar objects. The data
were acquired through exchanges with the Centre de Donn'ees Astronomiques
de Strasbourg (CDS) , other astronomical data centers throughout the
world, and by direct contributions from the international astronomical community.
- http://adc.gsfc.nasa.gov/
- Categories: center high_energy infrared optical radio ultraviolet
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Atomic Line List
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The atomic line list is a compilation of approximately 855,000
allowed, intercombination and forbidden atomic transitions with wavelengths in the
range from 0.5 Å to 1000 µm. Its primary intention
is to allow the identification of observed atomic absorption or
emission features. The list is nearly complete for all ionization
stages of all elements up to zinc. Transition probabilities are
available for nearly 14% of the lines; they are mostly
derived from Opacity Project data.
- http://www.pa.uky.edu/~peter/atomic/
- Categories: physics center high_energy infrared optical ultraviolet
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Cassini-Huygens Mission to Saturn & Titan
(Cassini)
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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.
- http://saturn.jpl.nasa.gov/home/
- Categories: planetary center infrared optical particles radio space telescope ultraviolet
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INACTIVE LINK ? - 107 ---
Center for Extreme Ultraviolet Astrophysics
(CEA / EUVE)
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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.
- http://www.cea.berkeley.edu/
- Categories: telescope center space ultraviolet
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Extreme Ultraviolet Explorer (EUVE) Archive
(at STScI)
- http://archive.stsci.edu/euve/
- Categories: center ultraviolet
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Far Ultraviolet Spectroscopic Explorer
(FUSE French site)
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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). [in
French]
- http://www.iap.fr/Fuse/
- Categories: telescope space ultraviolet
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Far Ultraviolet Spectroscopic Explorer
(FUSE)
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The Far Ultraviolet Spectroscopic Explorer was launched on June 24,
1999; this satellite astronomy project is based at The Johns
Hopkins University. [also in French]
- http://fuse.pha.jhu.edu/
- Categories: telescope space ultraviolet
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GALaxy Evolution EXplorer
(GALEX)
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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.
- http://www.galex.caltech.edu/
- Categories: telescope space ultraviolet
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GSFC's Exploration of the Universe Division
(EUD)
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NASA-GSFC's Exploration of the Universe Division conducts and supports astroparticle
(gamma-ray and cosmic-ray), X-ray, gravitational-wave, observational cosmology, exoplanet and stellar
astrophysics research.
- http://universe.gsfc.nasa.gov/
- Categories: center high_energy infrared planetary space ultraviolet
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INACTIVE LINK ? - 94 ---
German Interferometer for Multi-channel Photometry and Astrometry
(DIVA)
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The 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.
- http://www.ari.uni-heidelberg.de/diva/
- Categories: telescope infrared optical space ultraviolet
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Hubble Space Telescope
(HST)
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The Hubble Space Telescope is a cooperative program of the
European Space Agency (ESA) and the National Aeronautics and Space
Administration (NASA) to operate a long-lived space-based observatory for the
benefit of the international astronomical community. To accomplish this goal
and protect the spacecraft against instrument and equipment failures, NASA
had always planned on regular servicing missions. Hubble has special
grapple fixtures, 76 handholds, and stabilized in all three axes.
HST is a 2.4-meter reflecting telescope which was deployed in
low-Earth orbit (600 kilometers) by the crew of the space
shuttle Discovery (STS-31) on 25 April 1990. HST's current complement
of science instruments include three cameras, two spectrographs, and fine
guidance sensors (primarily used for astrometric observations). Because of HST's
location above the Earth's atmosphere, these science instruments can produce
high resolution images of astronomical objects. Ground-based telescopes can seldom
provide resolution better than 1.0 arc-seconds, except momentarily under the
very best observing conditions. HST's resolution is about 10 times
better, or 0.1 arc-seconds.
- http://www.stsci.edu/hst/
- Categories: telescope infrared optical space ultraviolet
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IUE Archive
(MAST)
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The International Ultraviolet Explorer (IUE) performed spectrophotometry at high (0.1-0.3
Å) and low (6-7 Å) resolution between 1150 Å and
3200 Å.
Over 104,000 ultraviolet spectra were obtained with
IUE between January 26, 1978, and September 30, 1996.
This is part of the Multimission Archive at STScI.
- http://archive.stsci.edu/iue/
- Categories: center ultraviolet
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INACTIVE LINK ? - 182 ---
IUE Newly Extracted Spectra
(INES)
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This data server provides access to IUE Final Archive data,
processed with the INES system. It was developed by the
ESA IUE project at VILSPA and is maintained and
distributed by ESA and LAEFF, the Principal Centre for
INES data. LAEFF is part of the Space Science Division
of INTA.
- http://ines.laeff.esa.es/ines/
- Categories: center ultraviolet
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Image Reduction and Analysis Facility
(IRAF)
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The main IRAF distribution includes a good selection of programs
for general image processing and graphics, plus a large number
of programs for the reduction and analysis of optical and
IR astronomy data (the "NOAO" packages). Other external or layered
packages are available for applications such as data acquisition or
handling data from other observatories and wavelength regimes such as
the Hubble Space Telescope (optical), EUVE (extreme ultra-violet), or ROSAT
and AXAF (X-ray). These external packages are distributed separately from
the main IRAF distribution but can be easily installed. The
IRAF system also includes a complete programming environment for scientific
applications, which includes a programmable Command Language scripting facility, the
IMFORT Fortran/C programming interface, and the full SPP/VOS programming environment
in which the portable IRAF system and all applications are
written.
- http://iraf.noao.edu/
- Categories: software high_energy infrared optical ultraviolet
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INACTIVE LINK ? - 174 ---
International Ultraviolet Explorer
(IUE)
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The International Ultraviolet Explorer (IUE) satellite was launched on the
26th of January 1978 and transferred into a geosynchronous orbit
over the Atlantic Ocean. The mission ended on September 30,
1996.
- http://www.vilspa.esa.es/iue/iue.html
- Categories: center space ultraviolet
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Large Binocular Telescope Observatory
(LBT)
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The Large Binocular Telescope (LBT) is a collaboration between Arizona
(25%), Italy (25%, represented by the Arcetri Astrophysical Observatory in
Florence), Research Corporation (12.5%), the Ohio State University (12.5%), and
Germany (25%, represented by the LBT Beteiligungsgesellschaft).
The goal
of the LBT project is to construct and exploit 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.
- http://lbto.org/
- Categories: telescope infrared optical ultraviolet
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Lausanne - General Catalogue of Photometric Data
(GCPD)
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The General Catalogue of Photometric Data (GCPD) built at the
Institute of Astronomy of the University of Lausanne contains photometric
data for about 200000 stars from some 75 different systems,
taken from about 3300 papers. The WWW server allows to
query the database ad retrieve any data from any photometric
system. Searching the references by authors' names and keywords from
the titles offers a possibility to retrieve the data from
each of the 3300 papers directly.
- http://obswww.unige.ch/gcpd/gcpd.html
- Categories: center bibliography infrared optical ultraviolet
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Libraries of stellar spectra
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Libraries of stellar spectra (late-type stars) by Montes et al.,
Other Libraries of stellar spectra. MK (Morgan-Keenan) Spectral Classification. Other
related links.
Maintained by David Montes, Departamento de Astrofísica,
Universidad Complutense de Madrid.
- http://www.ucm.es/info/Astrof/invest/actividad/spectra.html
- Categories: center infrared optical ultraviolet
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Multi-Experiment Data Operations Center for SOHO
(MEDOC)
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MEDOC (Multi-Experiment Data Operations Center for SOHO) is designed to
meet the needs of European SOHO Investigators who wish to
work together on the data analysis and the preparation of
joint observations using SOHO instruments and also European solar ground-based
Observatories. This European Centre complements the SOHO facilities (Experiment
Operations Facility, Experiment Analysis Facility, U.S. SOHO Archive
) located in GSFC (NASA).
- http://www.medoc-ias.u-psud.fr/
- Categories: center optical particles solar space ultraviolet
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Multimission Archive at STScI
(MAST)
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The Multimission Archive at STScI is being developed to support
a variety of astronomical data archives, with the primary focus
on scientifically related data sets in the optical, ultraviolet, and
near-infrared parts of the spectrum.
- http://archive.stsci.edu/mast.html
- Categories: center infrared optical ultraviolet
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NASA National Space Science Data Center
(NSSDC)
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The primary responsibility of the NSSDC is to further the
use of NASA spaceflight mission data. The NSSDC also provides
data from some ground-based and non-NASA sources which are considered
to be important adjuncts to the NASA space-based data. The
Data Center maintains and distributes documentation, indexes and catalogs about
the data in its archives, and similar information about important
space mission datasets maintained by other institutions. The
NSSDC's Astronomy and Astrophysics Home Page offers information about online
data and services, including access to a WAIS-searchable index of
more than 700 astronomical catalogs; high-level project descriptions for such
projects as ASCA, ROSAT, EUVE, HST, and COBE; and links
to many other popular astronomy and astrophysics resources.
- http://nssdc.gsfc.nasa.gov/
- Categories: center high_energy infrared optical particles radio ultraviolet
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NASA/IPAC Extragalactic Database
(NED)
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Research tool providing access to a broad range of published
extragalactic data. NED is continuously being updated and augmented. It
is the systematic merger of major catalogs of extragalactic objects
covering all wavelengths, and of object lists appearing in the
refereed literature.
NED contains about 800,000 objects, along with
names, redshifts, positions, bibliographic references, photometric measurements, and notes. The
Web interface of NED started recently serving images of objects
at various wavelengths.
- http://nedwww.ipac.caltech.edu/
- Categories: center abstracts bibliography high_energy infrared optical radio ultraviolet
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NCSA Astronomy Digital Image Library
(NCSA ADIL)
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The purpose of the NCSA Astronomy Digital Image Library is
to collect fully processed astronomical images in FITS format format
and make them available to the research community and the
general public via the World Wide Web. The collection contains
images from research observatories all over the world and taken
at all wavebands.
- http://imagelib.ncsa.uiuc.edu/imagelib.html
- Categories: library center education high_energy infrared optical pictures radio ultraviolet
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OAO-3 (Copernicus) Archive
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The Copernicus satellite, otherwise known as the Orbiting Astronomical Observatory
3 (OAO-3), obtained high resolution far- (900-1560 Å) and near-
(1650-3150 Å) ultraviolet spectra of 551 objects, primarily bright stars,
from 1972 to 1981.
This is part of the
Multimission Archive at STsCI (MAST).
- http://archive.stsci.edu/copernicus/
- Categories: center space ultraviolet
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PDS Imaging Node
(PDSIMG)
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The Imaging Node of the Planetary Data System is the
curator of NASA's primary digital image collections from past, present,
and future planetary missions. The node provides to the NASA
planetary science community the digital image archives, necessary ancillary datasets,
software tools, and technical expertise necessary to fully utilize the
vast collection of digital planetary imagery.
- http://pds-imaging.jpl.nasa.gov/
- Categories: center education infosys infrared optical pictures planetary software space ultraviolet
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PDS Imaging Node's Planetary Image Atlas
(PDSIMG Atlas)
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The Atlas is designed to be a single interface through
which you can search for, display, and download full resolution
data for all planetary missions. It will eventually replace individual
existing browsers. Until that time, links to the individual browsers
are provided from this central location. Current missions included in
the Atlas are: 2001 Mars Odyssey, Mars Global Surveyor, Magellan,
Clementine, Viking, Mars Pathfinder, Voyager, and Galileo.
- http://pds-imaging.jpl.nasa.gov/Atlas/
- Categories: center infrared optical pictures planetary space ultraviolet
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POLAR Spacecraft
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Exloring through the Solar Cycle. Instruments: Plasma Waves Investigation (PWI), Magnetic
Fields Experiment (MFE), Toroidal Imaging Mass-Angle Spectrograph (TIMAS), Electric Fields Investigation (EFI), Thermal
Ion Dynamics Experiment (TIDE), Ultraviolet Imager (UVI), Visible Imaging System (VIS), Polar Ionospheric
X-Ray Imaging Experiment (PIXIE), Charge and Mass Magnetosperic Ion Composition Experiment
(CAMMICE), Comprehensive Energetic-Particle Pitch-Angle Distribution - Source/Loss Cone Energetic Particle Spectrometer
(CEPPAD/SEPS), Hot Plasma Analyzer (HYDRA).
- http://istp.gsfc.nasa.gov/istp/polar/
- Categories: telescope high_energy optical particles space ultraviolet
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Padova database of stellar evolutionary tracks and isochrones
- http://pleiadi.pd.astro.it/
- Categories: center infrared optical ultraviolet
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Planetary Data System
(PDS)
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The PDS archives and distributes scientific data from NASA planetary
missions, astronomical observations, and laboratory measurements. The PDS is sponsored
by NASA's Office of Space Science. Its purpose is to
ensure the long-term usability of NASA data and to stimulate
advanced research. PDS is continually upgrading and updating its archives,
to better serve the needs of its user communities.
- http://pds.jpl.nasa.gov/index.html
- Categories: center high_energy infrared optical particles radio ultraviolet
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SOlar and Heliospheric Observatory
(SOHO)
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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
scientists.
- http://sohowww.nascom.nasa.gov/
- Categories: telescope optical particles solar space ultraviolet
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Solar Data Analysis Center
(SDAC)
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The SDAC at NASA Goddard Space Flight Center serves current
solar ground- and spaced-based imagery, text, figures, maps, and tables
of NASA eclipse bulletins, solar flare data from the Compton
GRO BATSE experiment and the Yohkoh spacecraft, and science operations
planning information for the SOHO Science Working Team.... and more
to come.
- http://umbra.nascom.nasa.gov/sdac.html
- Categories: center high_energy infrared optical particles pictures solar space ultraviolet
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Solar Extreme-ultraviolet Rocket Telescope and Spectrograph
(SERTS)
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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.
- http://serts.gsfc.nasa.gov/
- Categories: telescope solar space ultraviolet
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Solar UV Atlas from HRTS
(HRTS data)
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Through the generosity of Dr. Pål Brekke of the University
of Oslo, the High Resolution Spectrograph and Telescope (HRTS) ultraviolet
solar atlas is now available on the Web. Click here
for more information.
- http://umbra.nascom.nasa.gov/uv_atlas/atlas.html
- Categories: center pictures software solar space ultraviolet
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Solar-Terrestrial Physics Home Page
(STP)
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Solar-Terrestrial Physics Division of the National Geophysical Data Center home
page. Includes several various STP disciplines within the Center: geomagnetism, Iononosphere, Solar and Upper
Atmosphere, and two satellite programs: GOES and DMSP.
DMSP is a two satellite constellation of near-polar orbiting, sun-synchronous
satellites monitoring meteorological, oceanographic and solar-terrestrial physics environments. NGDC maintains
an archive of all data recorded on DMSP satellites as
relayed to NGDC by Air Force Global Weather Central. Data
from March 1992 to March 1994, are considered to be
experimental. After March 1994, the system should be fully operational.
- http://www.ngdc.noaa.gov/stp/stp.html
- Categories: center dept high_energy infrared optical particles radio solar space ultraviolet
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Southern African Large Telescope Project
(SALT)
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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.
- http://www.salt.ac.za/
- Categories: telescope infrared optical ultraviolet
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Space Telescope - European Coordinating Facility
(ST-ECF)
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The ST-ECF was established in 1984 jointly by the European
Space Agency and the European Southern Observatory and is located
at the ESO headquarters at Garching near Munich. The ST-ECF
supports the European astromical community in exploiting the research opportunities
provided by the earth-orbiting Hubble Space Telescope. The ST-ECF provides
detailed technical information about the HST and its science instruments,
supports European astronomers in the preparation of HST observing proposals,
coordinates the development of computer software tuned to the specific
data analysis needs of HST users, operates and maintains an
archive of all the scientific data collected by HST, and
acts as a European centre for associated meetings and workshops.
In all of these duties the ST-ECF staff maintains close
contacts with the Space Telescope Science Institute (STScI) in Baltimore,
which is charged with the scientific operation of the HST
observatory.
HST Archive at CADC.
- http://www.stecf.org/
- Categories: center infrared optical space ultraviolet
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Space Telescope Science Institute
(STScI)
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STScI is responsible for the scientific operations of the Hubble
Space Telescope (HST). STScI is operated by Associated Universities for
Research in Astronomy (AURA) under contract to NASA.
- http://www.stsci.edu/
- Categories: dept center infrared library optical software space survey ultraviolet
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Standard Objects For Astronomy
(SOFA)
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Site with links to Standard Object Resources classified according to
observing techniques and wavelength domains. Created by Patrice Corporon; now
maintained by Shashikiran Ganesh and Anatoly Miroshnichenko. (Indian mirror;
US mirror)
- http://sofa.sarovar.org/
- Categories: other_astronomy center high_energy infrared optical radio ultraviolet
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Swift Gamma Ray Burst Mission
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Swift is a three-telescope space observatory (gamma-ray telescope, X-ray telescope,
and ultraviolet/optical telescope) for studying gamma ray bursts. Scheduled launch:
October 7, 2004.
- http://swift.gsfc.nasa.gov/
- Categories: telescope high_energy optical space ultraviolet
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Synthetic Spectra of B Main-Sequence Stars from 3000 - 10000
(Landessternwarte Heidelberg-Königstuhl)
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This Web page provides a simple interactive tool for line
identification in B stars along the main sequence. The calculation
makes use of the atomic line list of Kurucz &
Bell (1995). For one of six possible effective temperatures between
10000 and 35000 K and an arbitrary wavelength range between
3000 and 10000 Å a normalized synthetic spectrum is displayed
on-line. The output consists of a gif image (~10 kB)
or a gzipped postscript file (~30 kB).
- http://www.lsw.uni-heidelberg.de/cgi-bin/websynspec.cgi
- Categories: center infrared optical ultraviolet
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Transition Region And Coronal Explorer
(TRACE)
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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.
- http://vestige.lmsal.com/TRACE/
- Categories: telescope optical solar ultraviolet
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Ultraviolet Imaging Telescope
(UIT - Archives at STScI MAST)
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The Ultraviolet Imaging Telescope (UIT) was one of three ultraviolet
telescopes on the ASTRO-1 mission flown on the space shuttle
Columbia during 2-10 December 1990. The same three instruments were
later flown on the space shuttle Endeavour from 3-17 March
1995, as part of the ASTRO-2 mission. Exposures were obtained
on 70-mm photographic film in the 1200-3300 Å range using
broadband filters and later digitized using a Perkin-Elmer microdensitometer. Image
resolution was 3" over a 40' field of view. Overall,
UIT-1 obtained 821 exposures of 66 targets, and UIT-2 obtained
758 images of 193 targets.
- http://archive.stsci.edu/uit/
- Categories: telescope space ultraviolet
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Wisconsin Ultraviolet Photo-Polarimeter Experiment
(WUPPE)
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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.
- http://www.sal.wisc.edu/WUPPE/
- Categories: telescope space ultraviolet
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This page was updated on: Fri 07 Dec 07