A dataset provided by the European Space Agency

Name OT2_dweedman_2
Title Luminosities and Temperatures of Dust with SPIRE for Most Luminous Quasars to z = 5
URL

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DOI 10.5270/esa-sctp10l
Author weedman, d.
Description SPIRE photometry is proposed for the 156 most infrared-luminous quasars with 1.5 < z < 5 to determine accurate total infrared luminosities and evolution of luminosity and dust temperature. Sources are chosen using new mid infrared measures with the Wide Field Infrared Survey Explorer of quasars from the Sloan Digital Sky Survey. SPIRE will measure all quasars in this redshift range at rest frame 80 micron, near the luminosity peak, and will give full SEDs from rest frame ultraviolet to far infrared when combined with WISE and SDSS data. Results can be compared to existing archival results for the most luminous, heavily obscured, type 2 quasars discovered with Spitzer and contained in Herschel key project survey fields.
Publication Dusty Quasars at High Redshifts . Weedman Daniel et al. . The Astrophysical Journal, Volume 828, Issue 1, article id. 43, 17 pp. (2016). . 828 . 10.3847\/0004-637X\/828\/1\/43 . 2016ApJ...828...43W ,
The WISSH quasars project. II. Giant star nurseries in hyper-luminous quasars . Duras F. et al. . Astronomy & Astrophysics, Volume 604, id.A67, 19 pp. . 604 . 10.1051\/0004-6361\/201731052 . 2017A&A...604A..67D ,
Instrument SPIRE_SpirePhoto_small
Temporal Coverage 2013-03-25T04:35:15Z/2013-04-17T11:20:52Z
Version SPG v14.1.0
Mission Description Herschel was launched on 14 May 2009! It is the fourth 'cornerstone' mission in the ESA science programme. With a 3.5 m Cassegrain telescope it is the largest space telescope ever launched. It is performing photometry and spectroscopy in approximately the 55-671 ┬Ám range, bridging the gap between earlier infrared space missions and groundbased facilities.
Creator Contact https://support.cosmos.esa.int/herschel/
Date Published 2013-10-17T11:18:03Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013-10-17T11:18:03Z, OT2_dweedman_2, SPG v14.1.0. https://doi.org/10.5270/esa-sctp10l