Shapley supercluster survey: galaxy evolution from filaments to cluster cores
| dc.contributor.author | Merluzzi, P. | |
| dc.contributor.author | Busarello, G. | |
| dc.contributor.author | Haines, C. P. | |
| dc.contributor.author | Mercurio, A. | |
| dc.contributor.author | Okabe, N. | |
| dc.contributor.author | Pimbblet, K. J. | |
| dc.contributor.author | Dopita, M. A. | |
| dc.contributor.author | Grado, A. | |
| dc.contributor.author | Limatola, L. | |
| dc.contributor.author | Bourdin, H. | |
| dc.contributor.author | Mazzotta, P. | |
| dc.contributor.author | Capaccioli, M. | |
| dc.contributor.author | Napolitano, N. R. | |
| dc.contributor.author | Schipani, P. | |
| dc.date.accessioned | 2015-05-12T01:29:50Z | |
| dc.date.available | 2015-05-12T01:29:50Z | |
| dc.date.issued | 2015-01 | |
| dc.date.updated | 2015-12-10T10:39:22Z | |
| dc.description.abstract | We present an overview of a multiwavelength survey of the Shapley Supercluster (SSC; z ~ 0.05) covering a contiguous area of 260 h70 -2 Mpc2 including the supercluster core. The project main aim is to quantify the influence of cluster-scale mass assembly | |
| dc.description.sponsorship | The research leading to these results has received funding from the European Community’s Seventh Framework Programme (FP7/2007–13) under grant agreement number 312430 (OPTICON; PI: P. Merluzzi) and PRIN-INAF 2011 ‘Galaxy evolution with the VLT Surveys Telescope (VST)’ (PI A. Grado). CPH was funded by CONICYT Anillo project ACT-1122. N.Okabe is supported by a Grant-in-Aid from the Ministry of Education, Culture, Sports, Science and Technology of Japan (26800097) and by World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan. | en_AU |
| dc.identifier.issn | 0035-8711 | en_AU |
| dc.identifier.uri | http://hdl.handle.net/1885/13443 | |
| dc.publisher | Oxford University Press | |
| dc.rights | http://www.sherpa.ac.uk/romeo/issn/0035-8711/..."Author's Post-print and Publisher's version/PDF on Institutional repositories or Central repositories, Set phrase to accompany archived copy (see policy)" from SHERPA/RoMEO site (as at 11/05/15) This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2014 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. | |
| dc.source | Monthly Notices of the Royal Astronomical Society | |
| dc.subject | gravitational lensing: weak | |
| dc.subject | galaxies: clusters: general | |
| dc.subject | galaxies: evolution | |
| dc.subject | galaxies: photometry | |
| dc.subject | galaxies: stellar contents | |
| dc.subject | galaxies: clusters: individual: A3552, A3554, A3556, A3558, A3559, A3560, A3562, AS0724 | |
| dc.title | Shapley supercluster survey: galaxy evolution from filaments to cluster cores | |
| dc.type | Journal article | |
| dcterms.dateAccepted | 2014-10-06 | |
| local.bibliographicCitation.issue | 1 | en_AU |
| local.bibliographicCitation.lastpage | 822 | en_AU |
| local.bibliographicCitation.startpage | 803 | en_AU |
| local.contributor.affiliation | Dopita, M. A., Research School of Astronomy and Astrophysics, The Australian National University | en_AU |
| local.contributor.authoruid | u7501303 | en_AU |
| local.identifier.absfor | 020100 - ASTRONOMICAL AND SPACE SCIENCES | |
| local.identifier.absseo | 970102 - Expanding Knowledge in the Physical Sciences | |
| local.identifier.ariespublication | a383154xPUB1370 | |
| local.identifier.citationvolume | 446 | en_AU |
| local.identifier.doi | 10.1093/mnras/stu2085 | en_AU |
| local.identifier.scopusID | 2-s2.0-84924463061 | |
| local.publisher.url | http://www.oxfordjournals.org/en/ | en_AU |
| local.type.status | Published Version | en_AU |