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Quantifying the suppression of the (un)-obscured star formation in galaxy cluster cores at 0.2 </~ z </~ 0.9
- Publication Year :
- 2019
-
Abstract
- © 2019 The Author(s). The authors thank Françoise Combes, Carlos López-Sanjuan, Dieter Lutz, Bianca Poggianti, and Alvio Renzini for their suggestions to improve this work. We acknowledge funding from the INAF PRINSKA 2017 program 1.05.01.88.04. LR-M acknowledges funding support from the Università degli studi di Padova – Dipartimento di Fisica e Astronomia ‘G. Galilei’. GR and CM acknowledge support from an INAF PRIN-SKA 2017 grant. PGP-G acknowledges funding support from the Spanish Government MINECO under grants AYA2015-70815-ERC and AYA2015-63650-P. ACE acknowledges support from STFC grant ST/P00541/1. AM acknowledges funding from the INAF PRIN-SKA 2017 program 1.05.01.88.04. Analyses were performed in R 3.4.0 (R Core Team 2018).<br />Ministerio de Economía y Competitividad (MINECO)<br />INAF PRINSKA 2017 program<br />Università degli studi di Padova – Dipartimento di Fisica e Astronomia ‘G. Galilei’<br />INAF<br />STFC<br />Depto. de Física de la Tierra y Astrofísica<br />Fac. de Ciencias Físicas<br />TRUE<br />pub
Details
- Database :
- OAIster
- Notes :
- application/pdf, 0035-8711, English
- Publication Type :
- Electronic Resource
- Accession number :
- edsoai.on1468753180
- Document Type :
- Electronic Resource