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2MASS

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(Redirected from2MASX)
Astronomical survey of the whole sky in the infrared
2MASS
Alternative namesTwo Micron All-Sky Survey
Websitewww.ipac.caltech.edu/2mass/
 Related media on Commons
2MASSJ-band image. Thebrown dwarf2MASS J17111353+2326333 is highlighted.

TheTwo Micron All-Sky Survey, or2MASS, was anastronomical survey of the whole sky ininfrared light.[1] It took place between 1997 and 2001, in two different locations: at the U.S.Fred Lawrence Whipple Observatory on Mount Hopkins, Arizona, and at theCerro Tololo Inter-American Observatory in Chile, each using a 1.3-meter telescope for theNorthern and Southern Hemisphere, respectively.[2] It was conducted in theshort-wavelength infrared at three distinctfrequency bands (J,H, andK) near 2micrometres, from which thephotometric survey with itsHgCdTe detectors derives its name.[1]

2MASS produced anastronomical catalog with over 300 million observedobjects, includingminor planets of the Solar System,brown dwarfs,low-mass stars,nebulae,star clusters andgalaxies. In addition, 1 million objects were cataloged in the2MASS Extended Source Catalog (2MASX). The cataloged objects are designated with a "2MASS" and "2MASX"-prefix respectively.

Catalog

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The final data release for 2MASS occurred in 2003,[3] and is served by theInfrared Science Archive. The goals of this survey included:

  • Detection of galaxies in the "Zone of Avoidance", a strip of sky obscured in visible light by our own galaxy, theMilky Way.
  • Detection of brown dwarfs. 2MASS discovered a total of 173, including2MASS 0939-2448,2MASS 0415-0935,2M1207, and2MASS J04414489+2301513.[4]
  • An extensive survey of low mass stars, the most common type of star both in our own galaxy and others.
  • Cataloging of all detected stars and galaxies.
  • Infrared measurements from the 2MASS survey have been particularly effective at unveiling previously undiscovered star clusters.[5][6]

Numerical descriptions of point sources (stars,planets,asteroids) and extended sources (galaxies, nebulae) were cataloged by automated computer programs to an average limitingmagnitude of about 14. More than 300 millionpoint sources and 1 million extended sources were cataloged. In November 2003, a team of scientists announced the discovery of theCanis Major Dwarf Galaxy, at that time the closest known satellite galaxy to the Milky Way, based on analysis of 2MASS stellar data.

The resulting data and images from the survey are currently in thepublic domain, and may be accessed online for free by anyone.[7] There is also a list of 2MASS science publications with links to free pre-publication copies of the papers.[8]

2MASS is sponsored by theUniversity of Massachusetts Amherst, theInfrared Processing and Analysis Center (IPAC, run byJet Propulsion Laboratory (JPL) andCaltech),NASA, and theNational Science Foundation (NSF).

References

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  1. ^ab"About 2MASS (A Brief Explanation of 2MASS)". University of Massachusetts, Infrared Processing and Analysis Center (JPL/ Caltech), NASA, NSF. 2006-02-01. Retrieved2008-09-21.
  2. ^"Two Micron All Sky Survey (2MASS)". NASA/IPAC Infrared Science Archive. Retrieved2011-10-22.
  3. ^"2MASS All-Sky Data Release FAQ Page".old.ipac.caltech.edu. Caltech. Retrieved14 December 2018.
  4. ^Kirkpatrick, J. Davy (2003). "2MASS Data Mining and the M, L, and T Dwarf Archives".IAU Symposium Vol. 211 ("Brown Dwarfs")(PDF). Brown Dwarfs. Vol. 211. p. 189.arXiv:astro-ph/0207672v1.Bibcode:2003IAUS..211..189K. Archived fromthe original(PDF) on 2020-08-20. Retrieved2011-10-20.
  5. ^Froebrich, D.; Scholz, A.; Raftery, C. L. (2007).A systematic survey for infrared star clusters with |b| <20° using 2MASS, MNRAS, 347, 2
  6. ^Majaess, D. (2013).Discovering protostars and their host clusters via WISE, ApSS, 344, 1
  7. ^"2MASS Data Access". The Two Micron All Sky Survey at IPAC. December 20, 2006. RetrievedSeptember 2, 2012.
  8. ^"2MASS Science Publications". The Two Micron All Sky Survey at IPAC. February 1, 2006. RetrievedSeptember 2, 2012.

External links

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