Stellar mass–halo mass relation for the brightest central galaxies of X-ray clusters since z ~ 0.65

Erfanianfar, G.; Finoguenov, A.; Furnell, K.; Popesso, P.; Biviano, A.; Wuyts, S.; Collins, C. A.; Mirkazemi, M.; Comparat, J.; Khosroshahi, H.; Nandra, K.; Capasso, R.; Rykoff, E.; Wilman, D.; Merloni, A.; Clerc, N.; Salvato, M.; Chitham, J. I.; Kelvin, L. S.; Gozaliasl, G.; Weijmans, A.; Brownstein, J.; Egami, E.; Pereira, M. J.; Schneider, D. P.; Kirkpatrick, C.; Damsted, S.; Kukkola, A.

doi:10.1051/0004-6361/201935375

Title: Stellar mass–halo mass relation for the brightest central galaxies of X-ray clusters since z ~ 0.65

Journal Article · 18 November 2019 · Astronomy and Astrophysics

DOI: https://doi.org/10.1051/0004-6361/201935375 · OSTI ID:1596766

Erfanianfar, G. ^[1]; Finoguenov, A. ^[2]; Furnell, K. ^[3]; Popesso, P. ^[4]; Biviano, A. ^[5]; Wuyts, S. ^[6]; Collins, C. A. ^[3]; Mirkazemi, M. ^[4]; Comparat, J. ^[1]; Khosroshahi, H. ^[7]; Nandra, K. ^[1]; Capasso, R. ^[8]; Rykoff, E. ^[9]; Wilman, D. ^[1]; Merloni, A. ^[1]; Clerc, N. ^[10]; Salvato, M. ^[1]; Chitham, J. I. ^[1]; Kelvin, L. S. ^[3]; Gozaliasl, G. ^[11] more »

Max Planck Inst. for Extraterrestrial Physics, Garching by Munich (Germany)
Max Planck Inst. for Extraterrestrial Physics, Garching by Munich (Germany); Univ. of Helsinki (Finland)
Liverpool John Moores Univ. (United Kingdom). Astrophysics Research Inst.
Excellence Cluster Universe, Garching bei München (Germany)
INAF/Osservatorio Astronomico di Trieste, Trieste (Italy)
Univ. of Bath (United Kingdom)
Inst. for Research in Fundamental Sciences (IPM), Tehran (Iran)
Ludwig-Maximilians-Univ., Munich (Germany); Excellence Cluster Universe, Garching bei München (Germany)
Stanford Univ., CA (United States). Kavli Inst. for Particle Astrophysics & Cosmology; SLAC National Accelerator Lab., Menlo Park, CA (United States)
L'Inst. de Recherche en Astrophysique et Planétologie (IRAP), Toulouse, (France); Univ. de Toulouse (France); Centre National de la Recherche Scientifique (CNRS), Toulouse (France); Centre National d'Études Spatiales (CNES), Toulouse (France)
Univ. of Turku, Quantum (Finland). Finnish centre for Astronomy with ESO (FINCA); Univ. of Helsinki (Finland)
Univ. of St. Andrews, Scotland (United Kingdom)
Univ. of Utah, Salt Lake City, UT (United States)
Univ. of Arizona, Tucson, AZ (United States)
Pennsylvania State Univ., University Park, PA (United States)
Univ. of Helsinki (Finland)

We present the brightest cluster galaxies (BCGs) catalog for SPectroscoic IDentification of eROSITA Sources (SPIDERS) DR14 cluster program value-added catalog. We list the 416 BCGs identified as part of this process, along with their stellar mass, star formation rates (SFRs), and morphological properties. We identified the BCGs based on the available spectroscopic data from SPIDERS and photometric data from SDSS. We computed stellar masses and SFRs of the BCGs on the basis of SDSS, WISE, and GALEX photometry using spectral energy distribution fitting. Morphological properties for all BCGs were derived by Sersic profile fitting using the software package SIGMA in different optical bands ($g,r,i$). We combined this catalog with the BCGs of galaxy groups and clusters extracted from the deeper AEGIS, CDFS, COSMOS, XMM-CFHTLS, and XMM-XXL surveys to study the stellar mass–halo mass relation using the largest sample of X-ray groups and clusters known to date. This result suggests that the mass growth of the central galaxy is controlled by the hierarchical mass growth of the host halo. We find a strong correlation between the stellar mass of BCGs and the mass of their host halos. This relation shows no evolution since $$z$$ ~ 0.65. We measure a mean scatter of 0.21 and 0.25 for the stellar mass of BCGs in a given halo mass at low (0.1 < $$z$$ < 0.3) and high (0.3 < $$z$$ < 0.65) redshifts, respectively. We further demonstrate that the BCG mass is covariant with the richness of the host halos in the very X-ray luminous systems. We also find evidence that part of the scatter between X-ray luminosity and richness can be reduced by considering stellar mass as an additional variable.

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Research Organization:: SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)

Sponsoring Organization:: USDOE Office of Science (SC)

Grant/Contract Number:: AC02-76SF00515

OSTI ID:: 1596766

Journal Information:: Astronomy and Astrophysics, Journal Name: Astronomy and Astrophysics Vol. 631; ISSN 0004-6361

Publisher:: EDP SciencesCopyright Statement

Country of Publication:: United States

Language:: English

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Galaxy sizes and the galaxy–halo connection – I. The remarkable tightness of the size distributions Zanisi, Lorenzo; Shankar, Francesco; Lapi, Andrea Monthly Notices of the Royal Astronomical Society, Vol. 492, Issue 2 https://doi.org/10.1093/mnras/stz3516	journal	December 2019

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79 ASTRONOMY AND ASTROPHYSICS
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