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Astronomical acronyms

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At the 2012 General Assembly of the International Astronomical Union (IAU; the international body for professional astronomy), the organising committee of IAU Commission 5 (Data and Information) requested the creation of a list of Astronomical Acronyms on Wikipedia. This list of acronyms and initials is not definitive but reflects current usage amongst professional astronomers.

Contents

1

  • 1RXS First ROSAT X-ray Survey
  • 2

  • 2MASS 2 Micron All Sky Survey
  • A

  • AAS American Astronomical Society – the primary association of professional astronomers in the United States
  • ACE Advanced Composition Explorer
  • ADS The Smithsonian Astrophysical Observatory/NASA astrophysics data system, an on-line database of almost all astronomical publications
  • AGC Arecibo general catalog
  • AGN active galactic nucleus – the nucleus of a galaxy that contains an active massive black hole
  • AIPS Astronomical Image Processing System – a widely used software package used for processing radio astronomy data
  • AMANDA Antarctic Muon And Neutrino Detector Array – a neutrino telescope located at a depth of 1.5 – 1.9 km below the ice in Antarctica.
  • AMBER Astronomical Multi-Beam Recombiner – a near-infrared interferometric instrument at VLTI
  • ARCADE Absolute Radiometer for Cosmology, Astrophysics, and Diffuse Emission – a balloon satellite experiment to measure the heating of the Universe by the first stars and galaxies after the big bang.
  • ASAS All Sky Automated Survey
  • ASKAP Australian Square Kilometre Array Pathfinder – a next-generation radio telescope under construction in Western Australia. It differs from previous radio-telescopes in having many pixels at the focus of each antenna.
  • ATCA Australia Telescope Compact Array, a radio telescope in Australia operated by CSIRO.
  • ATLAS Australia Telescope Large Area Survey – a deep radio astronomical sky survey of two SWIRE fields covering a total of about 7 square degrees of sky.
  • AU Astronomical Unit - a unit of length, roughly the distance from the Earth to the Sun.
  • B

  • BICEP2 Background Imaging of Cosmic Extragalactic Polarization 2
  • BLAST Balloon-borne Large Aperture Submillimeter Telescope – a submillimeter telescope that hangs from a high-altitude balloon, operated by a multi-university consortium headed by the University of Pennsylvania
  • BOOMERanG Balloon Observations Of Millimetric Extragalactic Radiation and Geophysics
  • C

  • CANGAROO Collaboration between Australian and Nippon for a Gamma Ray Observatory in the Outback - a very high energy cosmic gamma ray observatory, located on the Woomera Prohibited Area in South Australia.
  • CARA Centre for Astrophysical Research in Antarctica - an organisation that operates an observatory at the South Pole, including several different telescopes from different research groups.
  • CARMA Combined Array for Research in Millimeter-wave Astronomy - an array of millimetre-wave telescopes located near Owens Valley, California
  • CCAFS Cape Canaveral Air Force Station, an air force base in Florida where NASA launches satellites from.
  • CCD Charge Coupled Device - a device for the movement of electrical charge.
  • CDFS Chandra Deep Field South - a deep field surveyed by many telescopes at different wavelengths, first selected for deep field observations by the Chandra X-ray Observatory
  • CDM Cold dark matter is a hypothetical form of dark matter thought to account for 80% of matter in the Universe.
  • CDS Centre de données astronomiques de Strasbourg – a major astronomical data centre
  • CFHT Canada-France-Hawaii Telescope
  • CHIPSat Cosmic Hot Interstellar Plasma Spectrometer satellite
  • CINDI Coupled Ion-Neutral Dynamics Investigation
  • CMB Cosmic microwave background radiation thermal radiation filling the observable universe almost uniformly
  • CME – coronal mass ejection
  • COSMOS The Cosmic Evolution Survey a deep field surveyed by many telescopes at different wavelengths, first selected as a Hubble Space Telescope Treasury Project to survey a two square degree equatorial field with the Advanced Camera for Surveys (ACS).
  • CRRES Combined Release and Radiation Effects Satellite
  • CSS Catalina Sky Survey
  • CV – cataclysmic variable, a type of active star
  • D

  • DEC Declination
  • DSN Deep Space Network - network of large antennas and communication facilities.
  • DM dark matter – the unidentified non-baryonic matter responsible for 80% of matter in the Universe.
  • DSS Digitized Sky Survey
  • E

  • EGS Extended Groth Strip – a deep field surveyed by many telescopes at different wavelengths
  • EGRET Energetic Gamma Ray Experiment Telescope - a Gamma-ray telescope mounted on board NASA's Compton Gamma-Ray Observatory
  • ELAIS ESO Large-area infrared survey – a survey which named three deep fields (ELAIS-North, ELAIS-South1, ELAIS-South2) which are used for deep sky surveys
  • ELF Extremely Luminous Far-infrared Galaxy, a synonym for Ultra-Luminous infrared galaxy - a galaxy which emits more than 1012 solar luminosities in the far-infrared part of the electromagnetic spectrum.
  • EMU Evolutionary Map of the Universe – a planned radio survey of the sky which will use the new ASKAP radio telescope to make a radio survey of the sky, producing a catalogue of 70 million galaxies.
  • ESA European Space Agency
  • ESO European Southern Observatory
  • EVN European VLBI Network – a collaboration of the major radio astronomical institutes in Europe, Asia and South Africa to perform high angular resolution observations of cosmic radio sources.
  • F

  • FITS Flexible Image Transport System
  • FORTE Fast On-orbit Rapid Recording of Transient Events
  • FOV Field of View - the extent of the observable world that is seen at any given moment.
  • G

  • GALEX GALaxy Evolution eXplorer
  • GALEXASC GALaxy Evolution eXplorer all-sky catalog
  • GBT Green Bank Telescope – the world's largest fully steerable radio telescope operated by the National Radio Astronomy Observatory at Green Bank, West Virginia, US.
  • GMRT Giant Metrewave Radio Telescope
  • GOLD Global-scale Observations of the Limb and Disk
  • GOODS Great Observatories Origins Deep Survey
  • H

  • HCG Hickson Compact Group
  • HD Henry Draper Catalogue
  • HDF Hubble Deep Field - a deep field surveyed by many telescopes at different wavelengths, first selected for deep field observations by the Hubble Space Telescope
  • HDFS Hubble Deep Field South - a deep field surveyed by many telescopes at different wavelengths, first selected for deep field observations by the Hubble Space Telescope
  • HIP Hipparcos satellite
  • HLIRG Hyper-Luminous infrared galaxy - a galaxy which emits more than 1013 solar luminosities in the far-infrared part of the electromagnetic spectrum.
  • HET Hobby-Eberly Telescope
  • HOPS The H2O southern Galactic Plane Survey
  • HST Hubble Space Telescope
  • I

  • IAU International Astronomical Union
  • IC Index Catalog, a secondary catalog to the New General Catalogue
  • IMAGE Imager for Magnetopause-to-Aurora Global Exploration
  • IMBH Intermediate-mass black hole
  • IRAM Institut de radioastronomie millimétrique
  • IRAS Infrared Astronomical Satellite
  • ISON International Scientific Optical Network
  • J

  • JBO Jodrell Bank Observatory A radio observatory in England. Part of The University of Manchester.
  • JIVE Joint Institute for VLBI in Europe
  • JPL Jet Propulsion Laboratory
  • L

  • LCDM or ΛCDM Lambda – cold dark matter – a cosmological model in which the universe contains a cosmological constant, denoted by Lambda, and cold dark matter. It is frequently referred to as the standard model of Big Bang cosmology.
  • LINEAR LIncoln Near-Earth Asteroid Research
  • LIRG Luminous infrared galaxy - a galaxy which emits more than 1011 solar luminosities in the far-infrared part of the electromagnetic spectrum.
  • LMC Large Magellanic Cloud
  • LOAN Longitude of ascending node
  • LOFAR The LOFAR low-frequency synthesis array, based in the Netherlands
  • LONEOS Lowell Observatory Near-Earth-Object Search
  • LSST Large Synoptic Survey Telescope
  • M

  • MACHO Massive Compact Halo Objects – a class of objects once hypothesised to be the cause of Dark Matter
  • MALT Millimetre Astronomy Legacy Team – including MALT90 and MALT45
  • MAVEN Mars Atmosphere and Volatile EvolutioN
  • MBH – massive black hole
  • MCG Morphological Catalogue of Galaxies
  • MERLIN Multi Element Radio Linked Interferometer. A seven-telescope radio interferometer – maximum baseline ~200 km – operated from Jodrell Bank Observatory
  • MESSENGER MErcury Surface, Space ENvironment, GEochemistry and Ranging
  • MIDI MID-Infrared instrument. A mid-infrared instrument of the VLTI
  • MMS Magnetospheric Multiscale Mission
  • MPC Minor Planet Center
  • MRK Markarian galaxies
  • MSL Mars Science Laboratory
  • MUSYC Multi-wavelength survey by Yale-Chile
  • N

  • NASA National Aeronautics and Space Administration
  • NEAT Near-Earth Asteroid Tracking
  • NED NASA/IPAC Extragalactic Database
  • NEOWISE Near-Earth Object WISE
  • NGC New General Catalogue
  • NGS-POSS National Geographic Society – Palomar Observatory Sky Survey
  • NOAO National Optical Astronomy Observatory – one of the major optical observatory organisations in the USA
  • NRAO National Radio Astronomy Observatory – the premier radio observatory in the US
  • NRAL Nuffield Radio Astronomy Laboratory – the former name for Jodrell Bank Observatory
  • NuSTAR Nuclear Spectroscopic Telescope Array
  • NVSS NRAO VLA Sky Survey A major survey of the sky produced in 1998 using the VLA radio telescope
  • O

  • OSIRIS-REx Origins Spectral Interpretation Resource Identification Security Regolith Explorer
  • P

  • Pan-STARRS Panoramic Survey Telescope And Rapid Response System
  • PGC Principal Galaxies Catalogue
  • POSSUM Polarisation Sky Survey of the Universe's Magnetism – a polarisation survey to be conducted with the new ASKAP radio telescope
  • PRIMUS The Prism Multi-Object Survey – a large [spectroscopic survey] of several deep fields
  • PSR Pulsar
  • R

  • RA Right ascension
  • RASS ROSAT all-sky survey
  • ROSAT Röntgensatellit, German for 'X-ray satellite'
  • RXTE Rossi X-ray Timing Explorer
  • S

  • S82 Stripe 82
  • SAO Smithsonian Astrophysical Observatory
  • SDO Scattered disc object
  • SDO Solar Dynamics Observatory
  • SDSS Sloan Digital Sky Survey
  • SETI Search for extraterrestrial intelligence
  • SKA Square Kilometre Array – a next-generation radio telescope to be built in Australia and South Africa
  • SMBH – super-massive black hole
  • SMC Small Magellanic Cloud
  • SMM Solar Maximum Mission
  • SOHO SOlar and Heliospheric Observatory
  • SONEAR Southern Observatory for Near Earth Asteroids Research
  • SOLO Solar Orbiter
  • STEREO Solar TErrestrial RElations Observatory
  • SWIRE Spitzer Widefield Infrared Extragalactic Survey – a large deep survey carried out with the Spitzer space telescope
  • T

  • TABLEAUX International Conference on Automated Reasoning with Analytic Tableaux and Related Methods
  • TCC Theory of Cryptography Conference
  • THEMIS Time History of Events and Macroscale Interactions during Substorms
  • TNO Trans-Neptunian object
  • TPHOLs Theorem Proving in Higher-Order Logics
  • TRACE Transition Region and Coronal Explorer
  • U

  • UAI Union Astronomique Internationale – the French name for the International Astronomical Union, and one of its two official names
  • UGC Uppsala General Catalogue
  • UKIDSS UKIRT Infrared Deep Sky Survey
  • UKIRT United Kingdom Infrared Telescope
  • ULIRG Ultra-Luminous infrared galaxy - a galaxy which emits more than 1012 solar luminosities in the far-infrared part of the electromagnetic spectrum.
  • ULX Ultraluminous X-ray source
  • UZC Updated Zwicky Catalogue
  • V

  • VISTA Visible and Infrared Survey Telescope for Astronomy a 4-m diameter telescope operated by the European Southern Observatory, and located in Chile.
  • VIPERS VIMOS Public Extragalactic Redshift Survey an ESO Large Program to map galaxies over an unprecedented volume of the z~1 Universe
  • VLA Very Large Array – a large radio telescope located in Socorro, New Mexico, operated by the National Radio Astronomy Observatory
  • VLBI very long baseline interferometry – a technique used in Radio astronomy involving the use of radio telescopes separated by hundreds or thousands of km.
  • VLT Very Large Telescope – one of the world's largest telescopes, operated by the European Southern Observatory
  • VV Vorontsov-Vel'yaminov Interacting Galaxies
  • VVDS VIMOS-VLT Deep Survey
  • W

  • WALLABY WALLABY is a survey of neutral hydrogen in galaxies to be conducted with the new ASKAP radio telescope
  • WD White dwarf
  • WIMP Weakly interacting massive particle – a class of objects hypothesised to be the cause of Dark Matter
  • WIRE Wide Field Infrared Explorer
  • WISE Wide-field Infrared Survey Explorer
  • WMAP Wilkinson Microwave Anisotropy Probe
  • WSRT Westerbork Synthesis Radio Telescope
  • X

  • XMM X-ray Multi-Mirror Mission
  • Z

  • ZOA Zone of Avoidance
  • References

    Astronomical acronyms Wikipedia


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