Radio Astronomy

A List Supernova Pages on the WWW
Links to a growing list of WWW pages concerning all aspects of research on supernova and supernova remnants. Observations and theory; all types of supernovae; research groups and individual researchers.
Academia Sinica's Institute of Astronomy and Astrophysics ( ASIAA )
ASIAA is a research institute founded in 1993 at Taipei, Taiwan, Public of CHINA to study the universe and its constituents observationally and theoretically. ASIAA's initial emphasis is on radio astronomy. ASIAA has joined the Berkeley-Illinois-Maryland millimeter Array (BIMA) as a 10% partner sinice 1994. ASIAA is adding two elements to Smithsonian Astrophysical Observatory's Sub-Mn-Array (SMA) (the SMART project) to become a 15% partner of this frontier facility which is to be completed before the year 2000.
Arecibo Observatory - National Astronomy and Ionosphere Center ( NAIC )
Astronomical Dep. of University Of Thessaloniki
ATNF - Australia Telescope Compact Array ( ATCA, Narrabri )
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 - Mopra Antenna ( ATNF Mopra )
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 ( ATNF Parkes )
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.
ATNF Parkes 21cm Multibeam Survey
The Parkes 64-m telescope is commencing an HI Southern Sky and Zone of Avoidance survey in 1996. The survey will cover redshifts up to 0.04, and be sensitive to objects with HI mass between 10^6 and 10^10 solar masses, depending on distance. This will be the first extensive "blind" survey of the 21cm extragalactic sky.
Australia Telescope National Facility ( ATNF )
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.
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.
Caltech Millimeter Array
Caltech Submillimeter Observatory ( CSO )
A single-dish submillimeter telescope on Mauna Kea Hawaii operated by Caltech for the astronomy community under contract from the NSF
Cambridge LFST
Cambridge Ryle Telescope
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.
CSIRO - Australia Telescope National Facility ( CSIRO - ATNF )
Gopher , Anonymous ftp
CSIRO - Radiophysics Laboratory ( CSIRO - RP )
This server is operated by the CSIRO Australia Telescope National Facility and CSIRO Division of Radiophysics, located in Sydney, Australia. The Parkes Radio Observatory is also operated by ATNF. The top-level menu contains: ATNF Site Guides and General Information, The ATNF FTP Server - Documentation (See the README file first), The ATNF FTP Server - Parkes Catalogue '90, The ATNF FTP Server - Parkes, MIT, NRAO Survey, The ATNF FTP Server - COMRAD database.

There is also an FTP server , with contents: Various AIPS tasks and support routines for the processing of Australia Telescope data; Observing proposals and documentation related to the use and operation of the Australia Telescope, including vistors guides to all the ATNF sites; The Karma package (library and applications for Signal and Image Processing; A spectral line reduction package which can read a number of formats including those used by the Parkes 64m telescope; Another spectral line reduction package specifically for the reduction of spectral line data from the Parkes 64m telescope; - README

Daily Martian Weather Report
The Daily Martian Weather Report is produced by the Mars Global Surveyor Radio Science Team (MGS RST). When the MGS mapping sequence begins, the page will contain a daily weather report for the planet Mars based on radio occultation measurements of the temperature and pressure profiles of the Martian atmosphere. Currently, the site contains information about the MGS mission and the Radio Science Team, the radio occultation technique for study of planetary atmospheres, profiles of the atmosphere of Venus acquired during occultations of the Magellan spacecraft, and information for K-12 educators interested in e-mail communications between their classes and members of the MGS RST.
Deep Space Network - Goldstone Deep Space Station
Dominion Radio Astrophysical Observatory [English] ( DRAO )
DRAO is a national facility operated by the Herzberg Institute of Astrophysics of the National Research Council of Canada. The synthesis telescope is particularly suited to comprehensive studies of the interstellar medium, extended Galactic nebulae and star-forming regions, and of nearby galaxies. The other instruments are a 26-m paraboloid and a solar flux monitoring system. Observing proposals are welcome from all interested astronomers.
Effelsberg Radio Telescope ( MPIfR )
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.
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 Establishments.
ETH Institute of Astronomy ( ETH Zurich )
Welcome to the Institute of Astronomy at ETH Zurich. There are three groups, working on different topics, namely: The Optical Solar Astrophysics Group The Stellar Astrophysics Group The Radio Astronomy Group
European Incoherent SCATtter
Faint Images of the Radio Sky at Twenty-centimeters ( VLA FIRST )
FIRST -- Faint Images of the Radio Sky at Twenty-cm -- is a project designed to produce the radio equivalent of the Palomar Observatory Sky Survey over 10,000 square degrees of the North Galactic Cap. Using the NRAO Very Large Array (VLA) and an automated mapping pipeline, we produce images with 1.8" pixels, a typical rms of 150 Jy, and a resolution of 5" . At the 0.75 mJy source detection threshold, there are ~110 sources per square degree, ~35% of which have resolved structure on scales from 2-30" .
Five College Radio Astronomy Observatory ( FCRAO )
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.
Green Bank
Hartebeesthoek Radio Astronomy Observatory ( HartRAO )
Hat Creek Radio Observatory ( UMD )
Haystack Observatory
Institut de Radio Astronomie Millimétrique ( IRAM )
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). The three IRAM sites are:
IPS Radio & Space Services ( IPS )
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
James Clerk Maxwell Telescope ( JCMT )
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 (see HIA JCMT pages) 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 ( Peru )
Joint Astronomy Centre ( Hilo, Hawaii )
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 .
JPL Space Very Long Baseline Interferometry Project ( VSOP )
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.
Korea Astronomy Observatory
Large Millimeter and Submillimeter Array Project ( LMSA Project )
Large Millimeter Wavelength Telescope ( LMT, Mexico )
also see Large Millimeter Wavelength Telescope (LMT, Massachusetts)
Max-Planck-Institut für Radioastronomie ( MPIfR, Bonn )
Colloquium schedule (KOLLOQUIUMSPLANUNG -- Diese Planungsdatei ist LAN-öffentlich und über Internet zugänglich via 'anonymes ftp')
Metsähovi 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 Mets=E4hovi, 40 km west of Helsinki, Finland. The Cassegrain telescope system can be used at frequencies 10 - 230 GHz (wavelengths 3 cm - 1.8 mm).
Millimeter Array project ( MMA )
Millstone Hill Observatory ( MHO, Haystack )
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.
Mount Pleasant Radio Observatory ( Tasmania )
Mullard Radio Astronomy Observatory ( MRAO )
The Mullard Radio Astronomy Observatory is part of the Cavendish Laboratory, the Physics Department of the University of Cambridge. Current research interests include: the cosmic microwave background (Sunyaev-Zeldovich and primordial fluctuations), radio galaxies (hot-spots, spectral ageing), ultra-luminous infra-red galaxies, star formation in galaxies, low-frequency radio surveys, mm and sub-mm instrumentation, mm and sub-mm astronomy (star formation and outflows, interferometry, the Galactic Centre), the interplanetary medium, supernova remnants, optical aperture synthesis, and maximum entropy techniques.
Multi-Element Radio Linked Interferometer Network ( MERLIN - Jodrell Bank )
Multiwavelength Atlas of Galaxies
A Multiwavelength Atlas of Galaxies is presented as an educational tool for high school students. Optical, X-ray, Far-Infrared and Radio images are shown for a variety of nearby galaxies. Text describing the physical mechanisms of the different types of radiation, and their astronomical sources is supplied.
NASA SCAN
WAIS index to abstracts from NASA's Selected Current Space Aeronautics (SCAN) abstract service
Nation River Observatory
National Radio Astronomy Observatory ( NRAO )
The NRAO is a facility operated by Associated Universities, Inc. under cooperative agreement with the National Science Foundation.
NRAO/VLA Information System -- Maintenance Report summaries (Open and to be Repaired); Official VLA, VLBA and VLBI NUG Schedules; General Info for Visitors to NRAO (New Mexico); VLA Specific Information; VLBA Specific Information; Weather Information
NRAO-Charlottesville ( Headquarters ; there is also an anonFTP server .
NRAO-Socorro (Array Operations Center)
NRAO-Tucson
NRAO-VLA (Very Large Array)
NRAO-VLBA (Very Long Baseline Array)
NRAO-Green Bank (140-foot, GBT, OVLBI)
Nobeyama Radio Observatory, NAOJ ( NRO )
Information regarding the 45-m Telescope, the Millimeter Array(NMA), the Large Millimeter and Submillimeter Array (LMSA) project, and much more.
Noto VLBI Station
NRAO 12m
NRAO Arizona Operations ( NRAO-TUC )
The National Radio Astronomy Observatory Arizona Operations is the center for the following NRAO activities: (1) 12 Meter Telescope and (2) Millimeter Array Development Activities.
NRAO Charlottesville ( NRAO-CV )
This web page contains links to these items, among others: AIPS (Astronomical Image Processing System), AIPS++, NRAO Headquarters, The Central Development Lab, and the main NRAO Library.
Nuffield Radio Astronomy Laboratories
The NRAL home page is located at Jodrell Bank, and provides information about the research carried out by the members of the University of Manchester's Radio Atronomy Group. It also provides details of the Laboratories' main instrument, MERLIN, including details for applying for time, observing schedules, and user's guide.
Onsala Space Observatory ( OSO )
OSO is the Swedish National Facility for Radio Astronomy.
Orbiting Very Long Baseline Interferometry ( OVLBI )
Owens Valley Radio Observatory ( OVRO )
Postage Stamp Server for NVSS Radio Sky Survey ( NVSS Postage Stamp Server )
This Web page allows the user to obtain "postage stamp" FITS images of selected, small fields from the NRAO/VLA Sky Survey (NVSS). Either 1950 or 2000 positions are supported as are a number of projective geometries. This survey is being done with the National Radio Astronomy Observatory's Very Large Array telescope at a wavelength of 20 cm (1.4 GHz) and is producing images of the sky north of declination -40 deg with a resolution of 45". Both total intensity and linear polarization is being imaged. This project began in September 1993 and the main body of observations will be finished in the Summer of 1996. Results are being made available as they are produced.
Princeton University - Pulsar Group
The home page of the pulsar research group in the department of physics of Princeton University, this site includes pointers to the home pages of group members, a collection of pulsar related resources and pointers to our supported data analysis software (including TEMPO), and links to radio astronomy observatories and related sites.
Radio Pulsar Resources
A unified collection of information and pointers of interest to radio pulsar researchers. Resources include pointers to group and individual home pages, radio telescope home pages and telescope schedules, and pulsar related preprints and reprints.
Radio télescope millimetrique POM2 [French]
SERENDIP
The UC Berkeley SETI Program, SERENDIP (Search for Extraterrestrial Radio Emissions from Nearby Developed Intelligent Populations) is an ongoing scientific research effort aimed at detecting radio signals from extraterrestrial civilizations. The project is the world's only " piggyback" SETI system, operating alongside simultaneously conducted conventional radio astronomy observations. SERENDIP is currently piggybacking on the 1,000-foot dish at Arecibo Observatory in Puerto Rico, the largest radio telescope in the world.
SETI Institute Home Page ( SETI )
The SETI Institute (the Search for Extraterrestrial Intelligence) serves as an institutional home for scientific and educational projects relevant to the nature, distribution, and prevalence of life in the universe. The largest research effort is Project Phoenix, the privately-funded continuation of the Targeted Search portion of NASA's High Resolution Microwave Survey. Two other projects of interest are the Life in the Universe (LITU) Curriculum Project and the Flight Opportunities for Science Teacher EnRichment (FOSTER) Project. LITU develops supplementary science curriculum material for grades 3 through 9. FOSTER allows science teachers to experience the excitement of research on NASA's Kuiper Airborne Observatory (KAO).
SETI League
The SETI League believes that receipt of electromagnetic signals of intelligent origin from beyond our planet will change forever our view of humanity's place in the cosmos. Our mission it to organize and coordinate people interested in the Search for Extra-Terrestrial Intelligence in the hope of receiving such signals.
Southern Columbia Millimeter Telescope ( 1.2 Meter )
Space Sciences Laboratory ( Berkeley )
HEAD The High Energy Astrophysics Division of the American Astronomical Society. SPRG The Space Physics Research Group. SERENDIP The Search for Extraterrestrial Radio Emissions from Nearby Developed Intelligent Populations. HOU The Hands-On Universe Program. COBE The Cosmic Background Explorer. EAG The Experimental Astrophysics Group. ISI The Infrared Spatial Interferometer Group. CEA The Center for Extreme Ultraviolet Astrophysics. ORFEUS The Orbiting Retrievable Far and Extreme Ultraviolet Spectrometers and The Berkeley Spectrometer.
Submillimeter Array ( SMA )
Submillimeter Telescope Observatory ( SMTO )
Taeduk Radio Astronomy Observatory ( TRAO )
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.
The Cosmic Anisotropy Telescope
The CAT is a three-element interferometer for cosmic microwave background observations at 13 to 17 GHz.
Torun Radio Astronomy Observatory ( TRAO )
Torun Radio Astronomy Observatory (TRAO) is an educational and research facility to study the Universe by means of radio waves. The Observatory is a part of the Faculty of Physics and Astronomy of Nicolaus Copernicus University.
Universitity of Groningen - Kapteyn Astronomical Institute
There is also a Gopher server. Includes Dutch Astronomy Services
University of Calgary Radio Astronomy Laboratory
University of California, Berkeley - Astronomy Department ( UCB-Astronomy )
The UCB Astronomy Home Page contains general information about the department. We maintain links for faculty, staff, post docs and students so that they may make papers, images, and other information available. Also included are an e-mail directory for the department, and links to related institutions.
University of Georgia, Dept of Physics and Astronomy
Astronomy at UGA
University of Manchester. Radioastronomy Group ( UK )
University of Melbourne - School of Physics: Astrophysics Group
Ventspils International Radioastronomy Centre ( VIRC )
The Ventspils 32-m antenna is the biggest in the Baltics.
Very Large Array ( VLA )
Very Long Baseline Array ( VLBA )
VLBI Antenna at Fortaleza, Brazil
Westerbork Synthesis Radio Telescope ( WSRT - NFRA )
Zurich Solar Radio Spectrometer
The Radio Astronomy Group (RAG) of ETH in Zurich, Switzerland recorded solar radio spectrograms with an analog spectrometer called Daedalus(1974-1993) in the range of 100-1000 MHz. Its observation list can be accessed directly. Two digital spectrometers, IKARUS (1978--1985) and PHOENIX (1988 to the present), cover a range from 100--1000 MHz and 0.1--3 GHz, respectively. Their observation list contains references to frequency programs indicating what frequency was observed. More information can be obtained from a RAG member.
Updated on 96/9/16 8:38 GMT by Sergio Paoli spaoli@fcaglp.fcaglp.unlp.edu.ar