A dataset provided by the European Space Agency

Name OT1_jrigby_1
Title Resolved Herschel photometry and line spectroscopy for the brightest lensed galaxy at z~2
URL

http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342237740&instrument_name=HIFI&product_level=LEVEL0&compress=true
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http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342237740&instrument_name=SPIRE&product_level=LEVEL0&compress=true
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http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342237742&instrument_name=PACS&product_level=LEVEL0&compress=true
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http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342237743&instrument_name=SPIRE&product_level=LEVEL0&compress=true
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DOI 10.5270/esa-rzadruu
Author rigby, j.
Description We propose to obtain deep, spatially--resolved Herschel PACS and SPIRE photometry and PACs and HIFI spectroscopy of the brightest (in the rest-UV) lensed galaxy yet discovered, RCS0327 at z=1.7038. The goal is to characterize the dust--reprocessed spectral energy distribution (SED) of a typical star--forming galaxy at the epoch when half the Universe.s stars formed. Because RCS0327 extends across 38 arcsec, Herschel will spatially resolve it, and thus will measure spectral energy distributions in multiple spatially--distinct regions. The resulting SED will serve as one of very few templates of low--extinction star forming galaxies beyond the local universe. We will measure the far-infrared luminosity and thus infer a star formation rate, which we will compare to rates measured from the optical-nIR. Finally, we will measure the luminosities of the [O I] 63 and [C II] 158 micron lines, which with the far-IR luminosity constrain the densities, pressures, and radiation fields of the photo-dissociation regions. Such observations are impossible for Herschel in the distant universe without lensing amplification.
Publication
Instrument HIFI_HifiPoint_dbs, PACS_PacsPhoto_largeScan, SPIRE_SpirePhoto_small, PACS_PacsLineSpec_point
Temporal Coverage 2012-01-20T21:55:12Z/2012-07-05T14:55:54Z
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 2013-01-05T09:49:11Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2013-01-05T09:49:11Z, OT1_jrigby_1, SPG v14.2.0. https://doi.org/10.5270/esa-rzadruu