A dataset provided by the European Space Agency

Name OT2_gwilson_3
Title Constraining the star-formation activity in 10 SpARCS clusters: star-formation in the densest regions at z =1
URL

http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342245740&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=1342247406&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=1342248662&instrument_name=PACS&product_level=LEVEL0&compress=true

DOI https://doi.org/10.5270/esa-s9lmh8r
Author wilson, g.
Description We propose deep PACS imaging at 110/160 microns of a unique sample of ten high-redshift galaxy clusters spanning 0.87<z<1.34. These rich clusters are drawn from the homogeneously selected Spitzer Adaptation of the Red-sequence Cluster Survey (SpARCS), and have impressive spectroscopic coverage (a total of 457 confirmed members) and extensive multi-wavelength follow-up data (UV-MIR). These clusters bridge a pivotal epoch when star formation shifts toward higher densities and when substantial cluster mass is assembled. Moreover, MIPS imaging has already identified 55 cluster members, confirming that dust enshrouded star formation is occurring in these dense fields. We will use the PACS/MIPS data, in combination with the extensive optical spectroscopy and photometry, to characterize the nature of IR-luminous galaxies in clusters at zvirgul1. We will also measure the total star formation rate in these clusters, which will be used to study the effect of environment on galaxy formation.
Publication
Instrument PACS_PacsPhoto_largeScan
Temporal Coverage 2012-05-14T08:08:48Z/2012-07-29T00:46:21Z
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 µm range, bridging the gap between earlier infrared space missions and groundbased facilities.
Creator Contact https://support.cosmos.esa.int/h®erschel/
Date Published 2013-01-28T21:11:04Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, wilson, g., 2013, OT2_gwilson_3, SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-s9lmh8r