The cluster sample presented in this work has been observed by the CLASH survey, using the ACS and WFC3 cameras onboard HST, in 16 filters from the UV through the NIR. <P />Up to now, a total of 11 CLASH clusters have been observed by MUSE in different programmes. In previous works, we have used deep observations on three targets, MACS J1206, Abell 1063 and MACS J0416 (Caminha et al. 2016A&A...587A..80C, 2017, Cat. J/A+A/600/A90, 2017A&A...607A..93C), where the last two clusters are also part of the HFF initiative. In this work, we make use of archival MUSE data from the ESO programme IDs 095.A-0525, 096.A-0105, 097.A-0909 and 098.A-0590 (P.I. J.-P. Kneib) on the remaining eight clusters. <P />The observations were carried out during the period between 2015-June and 2017-January, with observation blocks (OBs) consisting of two exposures of ~1465 seconds. <P />(19 data files).
VizieR Online Data Catalog: Strong lensing models of 8 CLASH clusters (Caminha+, 2019)
MERCURIO, AMATA;
2019
Abstract
The cluster sample presented in this work has been observed by the CLASH survey, using the ACS and WFC3 cameras onboard HST, in 16 filters from the UV through the NIR. Up to now, a total of 11 CLASH clusters have been observed by MUSE in different programmes. In previous works, we have used deep observations on three targets, MACS J1206, Abell 1063 and MACS J0416 (Caminha et al. 2016A&A...587A..80C, 2017, Cat. J/A+A/600/A90, 2017A&A...607A..93C), where the last two clusters are also part of the HFF initiative. In this work, we make use of archival MUSE data from the ESO programme IDs 095.A-0525, 096.A-0105, 097.A-0909 and 098.A-0590 (P.I. J.-P. Kneib) on the remaining eight clusters. The observations were carried out during the period between 2015-June and 2017-January, with observation blocks (OBs) consisting of two exposures of ~1465 seconds. (19 data files).I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
