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=1342247340&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342247341&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342247406&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342247407&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
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, 2013-01-28T21:11:04Z, OT2_gwilson_3, SPG v14.2.0. https://doi.org/10.5270/esa-s9lmh8r