The Infrared Astronomical Satellite (IRAS) mission
G. Neugebauer,H. J. Habing,R. J. van Duinen,H. H. Aumann,B. Baud,Charles Beichman,D. A. Beintema,N. Boggess,P. E. Clegg,T. de Jong,J. P. Emerson,T. N. Gautier,F. C. Gillett,S. Harris,M. G. Hauser,J. R. Houck,R. E. Jennings,F. J. Low,P. L. Marsden,George K. Miley,F. M. Olnon,Stuart Pottasch,E. Raimond,M. Rowan-Robinson,B. T. Soifer,Russell G. Walker,P. R. Wesselius,Erick T. Young +27 more
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The Infrared Astronomical Satellite (IRAS) as discussed by the authors consists of a spacecraft and a liquid helium cryostat that contains a cooled IR telescope, whose focal plane assembly is cooled to less than 3 K, and contains 62 IR detectors in the survey array.Abstract:
The Infrared Astronomical Satellite (IRAS) consists of a spacecraft and a liquid helium cryostat that contains a cooled IR telescope. The telescope's focal plane assembly is cooled to less than 3 K, and contains 62 IR detectors in the survey array which are arranged so that every source crossing the field of view can be seen by at least two detectors in each of four wavelength bands. The satellite was launched into a 900 km-altitude near-polar orbit, and its cryogenic helium supply was exhausted on November 22, 1983. By mission's end, 72 percent of the sky had been observed with three or more hours-confirming scans, and 95 percent with two or more hours-confirming scans. About 2000 stars detected at 12 and 25 microns early in the mission, and identified in the SAO (1966) catalog, have a positional uncertainty ellipse whose axes are 45 x 9 arcsec for an hours-confirmed source.read more
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Journal ArticleDOI
Maps of Dust Infrared Emission for Use in Estimation of Reddening and Cosmic Microwave Background Radiation Foregrounds
TL;DR: In this article, a reprocessed composite of the COBE/DIRBE and IRAS/ISSA maps, with the zodiacal foreground and confirmed point sources removed, is presented.
Journal ArticleDOI
The wide-field infrared survey explorer (wise): mission description and initial on-orbit performance
Edward L. Wright,Peter Eisenhardt,Amy Mainzer,Michael E. Ressler,Roc M. Cutri,Thomas H. Jarrett,J. Davy Kirkpatrick,Deborah L. Padgett,Robert S. McMillan,Michael F. Skrutskie,Spencer A. Stanford,Spencer A. Stanford,Martin Cohen,Russell G. Walker,John C. Mather,David Leisawitz,Thomas N. Gautier,Ian S. McLean,Dominic J. Benford,Carol J. Lonsdale,Andrew Blain,B. Mendez,William R. Irace,Valerie G. Duval,Fengchuan Liu,Don Royer,I. Heinrichsen,Joan Howard,Mark A. Shannon,Martha Kendall,Amy L. Walsh,Mark F. Larsen,Joel Cardon,Scott Schick,Mark Schwalm,Mohamed Abid,Beth Fabinsky,Larry Naes,Chao-Wei Tsai +38 more
TL;DR: The Wide-field Infrared Survey Explorer (WISE) is mapping the whole sky following its launch on 14 December 2009 and completed its first full coverage of the sky on July 17 as discussed by the authors.
Journal ArticleDOI
Herschel Space Observatory - An ESA facility for far-infrared and submillimetre astronomy
Göran Pilbratt,J. R. Riedinger,T. Passvogel,G. Crone,D. Doyle,U. Gageur,Ana M. Heras,C. Jewell,L. Metcalfe,S. Ott,Michael Schmidt +10 more
TL;DR: Herschel was launched on 14 May 2009, and is now an operational ESA space observatory o ering unprecedented observational capabilities in the far-infrared and sub-millimetre spectral range 55 671 m.
Journal ArticleDOI
Luminous infrared galaxies
David B. Sanders,I. F. Mirabel +1 more
TL;DR: At the highest luminosities (Lir > 1012 ), nearly all objects appear to be advanced mergers powered by a mixture of circumnuclear starburst and active galactic nucleus energy sources, both of which are fueled by an enormous concentration of molecular gas that has been funneled into the merger nucleus as discussed by the authors.
Journal ArticleDOI
A Highly Consistent Framework for the Evolution of the Star-Forming "Main Sequence" from z~0-6
Joshua S. Speagle,Joshua S. Speagle,Charles L. Steinhardt,Charles L. Steinhardt,Peter Capak,John D. Silverman +5 more
TL;DR: In this article, the authors investigate the evolution of the star-forming galaxy (SFG) main sequence (MS) in stellar mass and star formation rate (SFR) out to z ~ 6.4 Gyr.
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