The role of AGN activity in the building up of the BCG at z ∼ 1.6
Abstract
XDCPJ0044.0-2033 is one of the most massive galaxy cluster at z ∼1.6, for which a wealth of multi-wavelength photometric and spectroscopic data have been collected during the last years. I have reported on the properties of the galaxy members in the very central region (∼ 70kpc × 70kpc) of the cluster, derived through deep HST photometry, SINFONI and KMOS IFU spectroscopy, together with Chandra X-ray, ALMA and JVLA radio data.
- Publication:
-
Nuclear Activity in Galaxies Across Cosmic Time
- Pub Date:
- January 2021
- DOI:
- 10.1017/S1743921320003105
- arXiv:
- arXiv:2008.12129
- Bibcode:
- 2021IAUS..356..280B
- Keywords:
-
- galaxy cluster;
- BCG formation;
- active galaxies;
- galaxy formation;
- Astrophysics - Astrophysics of Galaxies
- E-Print:
- Proceeding for the IAUS 356: Nuclear Activity in Galaxies Across Cosmic Time. arXiv admin note: text overlap with arXiv:2008.11132