A dataset provided by the European Space Agency

Name OT2_bbertinc_1
Title Accurate SFRs and dust masses across the star-forming main sequence of galaxies: PACS observations of a local unbiased sample.
URL

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DOI 10.5270/esa-hs5uel3
Author bertincourt, b.
Description Recent studies in galaxy evolution have uncovered a tight "main sequence" (MS) of star-forming galaxies that evolves with redshift. We propose to obtain Herschel FIR photometry for 100 galaxies from the S5 galaxy sample (Spitzer SDSS Statistical Spectroscopic Survey)---the largest optically selected sample of galaxies with Spitzer mid-IR spectroscopy---in order to test and improve our understanding of this MS. We will derive accurate IR luminosities, dust temperatures, dust masses and derived star formation rates for a representative sample of normal star-forming galaxies extending up to 2 sigma above and below the MS at z~0.07. In combination with the extensive multi-wavelength data that exists for the S5 sample, PACS-Herschel photometry will provide the critical, final piece of the puzzle that we need to track the evolution of physical parameters across the main sequence. Furthermore, we anticipate that this survey will produce a unique data set that will connect Herschel studies of local and distant galaxies to the vast archival resource of SDSS and corollary observations.
Publication
Instrument PACS_PacsPhoto_largeScan
Temporal Coverage 2013-02-20T02:53:46Z/2013-04-27T15:17:06Z
Version SPG v14.2.0
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 2013-10-27T15:13:34Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013-10-27T15:13:34Z, OT2_bbertinc_1, SPG v14.2.0. https://doi.org/10.5270/esa-hs5uel3