A dataset provided by the European Space Agency

Name SDP_gsmith01_3
Title LoCuSS: A Legacy Survey of Galaxy Clusters at z=0.2
URL

http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342186762&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342186763&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342187012&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342187013&instrument_name=PACS&product_level=LEVEL0&compress=true
DOI https://doi.org/10.5270/esa-17s9u19
Author smith, g.
Description We propose a definitive census of obscured star formation in intermediate redshift clusters and its relationship with the recent mass assembly and thermodynamic histories of the clusters. Specifically, we propose to use Herschel/PACS observations at 100 and 160um in conjunction with our Spitzer 24um data to characterize the dust-obscured galaxy populations (star formation rate, AGN contamination, bolometric IR luminosity, dust temperature) in a large unbiased sample of galaxy clusters at 0.15<z<0.3. The sample of 32 clusters is drawn from the Local Cluster Substructure Survey (LoCuSS) for which outstanding supporting data are available, including gravitational lensing, X-ray spectro-imaging, and Spitzer 24um maps. This unprecedented dataset on a large and unbiased cluster sample will enable us to answer definitively the question: what physical process(es) are responsible for triggering obscured star-formation in cluster galaxies?. The enduring legacy will be a baseline study of the demographics of low-intermediate redshift clusters against which to compare and thus interpret the rapidly growing menagerie of high redshift cluster observations. This will be achieved through a series of public data releases, that will include quantities derived from the Herschel data (e.g. L_IR, T_dust) and from our huge investment in supporting data (e.g. dark matter density, galaxy redshifts, galaxy morphologies). All of this can be achieved with a modest Key Programme of 145 hours duration.
Publication
  • A Catalog of Host Galaxies for WISE-selected AGN: Connecting Host Properties with Nuclear Activity and Identifying Contaminants | Barrows R. Scott et al. | The Astrophysical Journal | null | null | 2021ApJ...922..179B |
  • LoCuSS: Probing galaxy transformation physics with Herschel | Smith G. P. et al. | Astronomy and Astrophysics Volume 518 id.L18 5 pp. | 518 | 10.1051\\/0004-6361\\/201014691 | 2010A&A...518L..18S | http://adsabs.harvard.edu/abs/2010A%26A...518L..18S
  • A Herschel Study of 24 mmm-Selected AGNs and Their Host Galaxies | Xu Lei et al. | The Astrophysical Journal Supplement Series Volume 219 Issue 2 article id. 18 36 pp. (2015). | 219 | 10.1088\\/0067-0049\\/219\\/2\\/18 | 2015ApJS..219...18X | http://adsabs.harvard.edu/abs/2015ApJS..219...18X
  • Extensive Lensing Survey of Optical and Near-infrared Dark Objects (El Sonido): HST H-faint Galaxies behind 101 Lensing Clusters | Sun Fengwu et al. | The Astrophysical Journal | null | null | 2021ApJ...922..114S |
  • LoCuSS: The Steady Decline and Slow Quenching of Star Formation in Cluster Galaxies over the Last Four Billion Years | Haines C. P. et al. | The Astrophysical Journal Volume 775 Issue 2 article id. 126 23 pp. (2013). | 775 | 10.1088\\/0004-637X\\/775\\/2\\/126 | 2013ApJ...775..126H | http://adsabs.harvard.edu/abs/2013ApJ...775..126H
  • LoCuSS: exploring the connection between local environment, star formation, and dust mass in Abell 1758 | Bianconi M. et al. | Monthly Notices of the Royal Astronomical Society | null | null | 2020MNRAS.492.4599B |
  • The role of massive halos in the star formation history of the Universe | Popesso P. et al. | Astronomy & Astrophysics Volume 579 id.A132 17 pp. | 579 | 10.1051\\/0004-6361\\/201424715 | 2015A&A...579A.132P | http://adsabs.harvard.edu/abs/2015A%26A...579A.132P
  • The Relation between Luminous AGNs and Star Formation in Their Host Galaxies | Xu Lei et al. | The Astrophysical Journal Volume 808 Issue 2 article id. 159 10 pp. (2015). | 808 | 10.1088\\/0004-637X\\/808\\/2\\/159 | 2015ApJ...808..159X | http://adsabs.harvard.edu/abs/2015ApJ...808..159X
Instrument PACS_PacsPhoto_largeScan
Temporal Coverage 2009-11-07T00:15:52Z/2009-11-15T04:54:10Z
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 2009-12-25T02:25:30Z
Keywords Herschel, HSC, submillimetre, far-infrared, HIFI, PACS, SPIRE
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, smith et al., 2009, 'LoCuSS: A Legacy Survey of Galaxy Clusters at z=0.2', SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-17s9u19