The Observed Evolution of the Stellar Mass–Halo Mass Relation for Brightest Central Galaxies

Golden-Marx, Jesse B.; Miller, C. J.; Zhang, Y.; Ogando, R. C.; Palmese, A.; Abbott, T. C.; Aguena, M.; Allam, S.; Andrade-Oliveira, F.; Annis, J.; Bacon, D.; Bertin, E.; Brooks, D.; Buckley-Geer, E.; Carnero Rosell, A.; Carrasco Kind, M.; Castander, F. J.; Costanzi, M.; Crocce, M.; da Costa, L. N.; Pereira, M. S.; De Vicente, J.; Desai, S.; Diehl, H. T.; Doel, P.; Drlica-Wagner, A.; Everett, S.; Evrard, A. E.; Ferrero, I.; Flaugher, B.; Fosalba, P.; Frieman, J.; García-Bellido, J.; Gaztanaga, E.; Gerdes, D. W.; Gruen, D.; Gruendl, R. A.; Gschwend, J.; Gutierrez, G.; Hartley, W. G.; Hinton, S. R.; Hollowood, D. L.; Honscheid, K.; Hoyle, B.; James, D. J.; Jeltema, T.; Kim, A. G.; Krause, E.; Kuehn, K.; Kuropatkin, N.; Lahav, O.; Lima, M.; Maia, M. G.; Marshall, J. L.; Melchior, P.; Menanteau, F.; Miquel, R.; Mohr, J. J.; Morgan, R.; Paz-Chinchón, F.; Petravick, D.; Pieres, A.; Plazas Malagón, A. A.; Prat, J.; Romer, A. K.; Sanchez, E.; Santiago, B.; Scarpine, V.; Schubnell, M.; Serrano, S.; Sevilla-Noarbe, I.; Smith, M.; Soares-Santos, M.; Suchyta, Eric; Tarle, G.; Varga, T. N.

doi:10.3847/1538-4357/ac4cb4

Title: The Observed Evolution of the Stellar Mass–Halo Mass Relation for Brightest Central Galaxies

Abstract

We quantify evolution in the cluster-scale stellar mass–halo mass (SMHM) relation's parameters using 2323 clusters and brightest central galaxies (BCGs) over the redshift range 0.03 ≤ z ≤ 0.60. The precision on the inferred SMHM parameters is improved by including the magnitude gap (m_gap) between the BCG and fourth-brightest cluster member (M14) as a third parameter in the SMHM relation. At fixed halo mass, accounting for m_gap, through a stretch parameter, reduces the SMHM relation's intrinsic scatter. To explore this redshift range, we use clusters, BCGs, and cluster members identified using the Sloan Digital Sky Survey C4 and redMaPPer cluster catalogs and the Dark Energy Survey redMaPPer catalog. Through this joint analysis, we detect no systematic differences in BCG stellar mass, m_gap, and cluster mass (inferred from richness) between the data sets. We utilize the Pareto function to quantify each parameter's evolution. We confirm prior findings of negative evolution in the SMHM relation's slope (3.5σ), and detect negative evolution in the stretch parameter (4.0σ) and positive evolution in the offset parameter (5.8σ). This observed evolution, combined with the absence of BCG growth, when stellar mass is measured within 50 kpc, suggests that this evolution results from changes in the cluster'smore »« less

Authors:

; Miller, C. J.;

;

; Allam, S.; Andrade-Oliveira, F.;

;

; Buckley-Geer, E.;

;

Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States)

Publication Date:: Thu Mar 24 00:00:00 EDT 2022

Research Org.:: Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States); SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States); Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States); Univ. of Michigan, Ann Arbor, MI (United States)

Sponsoring Org.:: USDOE Office of Science (SC), High Energy Physics (HEP); European Research Council (ERC); Brazilian Instituto Nacional de Ciênciae Tecnologia (INCT); National Science Foundation (NSF); MICINN; USDOE Office of Science (SC), Basic Energy Sciences (BES)

Contributing Org.:: DES Collaboration

OSTI Identifier:: 1824314

Alternate Identifier(s):: OSTI ID: 1867383; OSTI ID: 1883723; OSTI ID: 1923763; OSTI ID: 1983575

Report Number(s):: FERMILAB-PUB-21-303-AE; arXiv:2107.02197
Journal ID: ISSN 0004-637X; oai:inspirehep.net:1899577; TRN: US2215686

Grant/Contract Number:: AC02-05CH11231; AC02-07CH11359; AST-1138766; AST-1536171; ESP2017-89838; PGC2018-094773; PGC2018-102021; SEV-2016-0588; SEV-2016-0597; MDM-2015-0509; 240672; 291329; 306478; 465376/2014-2; AC02-76SF00515; AC05-00OR22725; SC0019193

Resource Type:: Accepted Manuscript

Journal Name:: The Astrophysical Journal

Additional Journal Information:: Journal Volume: 928; Journal Issue: 1; Journal ID: ISSN 0004-637X

Publisher:: IOP Publishing

Country of Publication:: United States

Language:: English

Subject:: 79 ASTRONOMY AND ASTROPHYSICS; galaxy clusters; galaxy evolution; brightest cluster galaxies

Citation Formats


                    Golden-Marx, Jesse B., Miller, C. J., Zhang, Y., Ogando, R. C., Palmese, A., Abbott, T. C., Aguena, M., Allam, S., Andrade-Oliveira, F., Annis, J., Bacon, D., Bertin, E., Brooks, D., Buckley-Geer, E., Carnero Rosell, A., Carrasco Kind, M., Castander, F. J., Costanzi, M., Crocce, M., da Costa, L. N., Pereira, M. S., De Vicente, J., Desai, S., Diehl, H. T., Doel, P., Drlica-Wagner, A., Everett, S., Evrard, A. E., Ferrero, I., Flaugher, B., Fosalba, P., Frieman, J., García-Bellido, J., Gaztanaga, E., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hartley, W. G., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hoyle, B., James, D. J., Jeltema, T., Kim, A. G., Krause, E., Kuehn, K., Kuropatkin, N., Lahav, O., Lima, M., Maia, M. G., Marshall, J. L., Melchior, P., Menanteau, F., Miquel, R., Mohr, J. J., Morgan, R., Paz-Chinchón, F., Petravick, D., Pieres, A., Plazas Malagón, A. A., Prat, J., Romer, A. K., Sanchez, E., Santiago, B., Scarpine, V., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Smith, M., Soares-Santos, M., Suchyta, Eric, Tarle, G., and Varga, T. N. The Observed Evolution of the Stellar Mass–Halo Mass Relation for Brightest Central Galaxies.  United States: N. p., 2022. 
Web.  doi:10.3847/1538-4357/ac4cb4.

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                    Golden-Marx, Jesse B., Miller, C. J., Zhang, Y., Ogando, R. C., Palmese, A., Abbott, T. C., Aguena, M., Allam, S., Andrade-Oliveira, F., Annis, J., Bacon, D., Bertin, E., Brooks, D., Buckley-Geer, E., Carnero Rosell, A., Carrasco Kind, M., Castander, F. J., Costanzi, M., Crocce, M., da Costa, L. N., Pereira, M. S., De Vicente, J., Desai, S., Diehl, H. T., Doel, P., Drlica-Wagner, A., Everett, S., Evrard, A. E., Ferrero, I., Flaugher, B., Fosalba, P., Frieman, J., García-Bellido, J., Gaztanaga, E., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hartley, W. G., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hoyle, B., James, D. J., Jeltema, T., Kim, A. G., Krause, E., Kuehn, K., Kuropatkin, N., Lahav, O., Lima, M., Maia, M. G., Marshall, J. L., Melchior, P., Menanteau, F., Miquel, R., Mohr, J. J., Morgan, R., Paz-Chinchón, F., Petravick, D., Pieres, A., Plazas Malagón, A. A., Prat, J., Romer, A. K., Sanchez, E., Santiago, B., Scarpine, V., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Smith, M., Soares-Santos, M., Suchyta, Eric, Tarle, G., & Varga, T. N. The Observed Evolution of the Stellar Mass–Halo Mass Relation for Brightest Central Galaxies.  United States.  https://doi.org/10.3847/1538-4357/ac4cb4

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                    Golden-Marx, Jesse B., Miller, C. J., Zhang, Y., Ogando, R. C., Palmese, A., Abbott, T. C., Aguena, M., Allam, S., Andrade-Oliveira, F., Annis, J., Bacon, D., Bertin, E., Brooks, D., Buckley-Geer, E., Carnero Rosell, A., Carrasco Kind, M., Castander, F. J., Costanzi, M., Crocce, M., da Costa, L. N., Pereira, M. S., De Vicente, J., Desai, S., Diehl, H. T., Doel, P., Drlica-Wagner, A., Everett, S., Evrard, A. E., Ferrero, I., Flaugher, B., Fosalba, P., Frieman, J., García-Bellido, J., Gaztanaga, E., Gerdes, D. W., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Hartley, W. G., Hinton, S. R., Hollowood, D. L., Honscheid, K., Hoyle, B., James, D. J., Jeltema, T., Kim, A. G., Krause, E., Kuehn, K., Kuropatkin, N., Lahav, O., Lima, M., Maia, M. G., Marshall, J. L., Melchior, P., Menanteau, F., Miquel, R., Mohr, J. J., Morgan, R., Paz-Chinchón, F., Petravick, D., Pieres, A., Plazas Malagón, A. A., Prat, J., Romer, A. K., Sanchez, E., Santiago, B., Scarpine, V., Schubnell, M., Serrano, S., Sevilla-Noarbe, I., Smith, M., Soares-Santos, M., Suchyta, Eric, Tarle, G., and Varga, T. N. Thu .  
"The Observed Evolution of the Stellar Mass–Halo Mass Relation for Brightest Central Galaxies".  United States.  https://doi.org/10.3847/1538-4357/ac4cb4.  https://www.osti.gov/servlets/purl/1824314.

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@article{osti_1824314,

  title        = {The Observed Evolution of the Stellar Mass–Halo Mass Relation for Brightest Central Galaxies},

  author       = {Golden-Marx, Jesse B. and Miller, C. J. and Zhang, Y. and Ogando, R. C. and Palmese, A. and Abbott, T. C. and Aguena, M. and Allam, S. and Andrade-Oliveira, F. and Annis, J. and Bacon, D. and Bertin, E. and Brooks, D. and Buckley-Geer, E. and Carnero Rosell, A. and Carrasco Kind, M. and Castander, F. J. and Costanzi, M. and Crocce, M. and da Costa, L. N. and Pereira, M. S. and De Vicente, J. and Desai, S. and Diehl, H. T. and Doel, P. and Drlica-Wagner, A. and Everett, S. and Evrard, A. E. and Ferrero, I. and Flaugher, B. and Fosalba, P. and Frieman, J. and García-Bellido, J. and Gaztanaga, E. and Gerdes, D. W. and Gruen, D. and Gruendl, R. A. and Gschwend, J. and Gutierrez, G. and Hartley, W. G. and Hinton, S. R. and Hollowood, D. L. and Honscheid, K. and Hoyle, B. and James, D. J. and Jeltema, T. and Kim, A. G. and Krause, E. and Kuehn, K. and Kuropatkin, N. and Lahav, O. and Lima, M. and Maia, M. G. and Marshall, J. L. and Melchior, P. and Menanteau, F. and Miquel, R. and Mohr, J. J. and Morgan, R. and Paz-Chinchón, F. and Petravick, D. and Pieres, A. and Plazas Malagón, A. A. and Prat, J. and Romer, A. K. and Sanchez, E. and Santiago, B. and Scarpine, V. and Schubnell, M. and Serrano, S. and Sevilla-Noarbe, I. and Smith, M. and Soares-Santos, M. and Suchyta, Eric and Tarle, G. and Varga, T. N.},

  abstractNote = {We quantify evolution in the cluster-scale stellar mass–halo mass (SMHM) relation's parameters using 2323 clusters and brightest central galaxies (BCGs) over the redshift range 0.03 ≤ z ≤ 0.60. The precision on the inferred SMHM parameters is improved by including the magnitude gap (mgap) between the BCG and fourth-brightest cluster member (M14) as a third parameter in the SMHM relation. At fixed halo mass, accounting for mgap, through a stretch parameter, reduces the SMHM relation's intrinsic scatter. To explore this redshift range, we use clusters, BCGs, and cluster members identified using the Sloan Digital Sky Survey C4 and redMaPPer cluster catalogs and the Dark Energy Survey redMaPPer catalog. Through this joint analysis, we detect no systematic differences in BCG stellar mass, mgap, and cluster mass (inferred from richness) between the data sets. We utilize the Pareto function to quantify each parameter's evolution. We confirm prior findings of negative evolution in the SMHM relation's slope (3.5σ), and detect negative evolution in the stretch parameter (4.0σ) and positive evolution in the offset parameter (5.8σ). This observed evolution, combined with the absence of BCG growth, when stellar mass is measured within 50 kpc, suggests that this evolution results from changes in the cluster's mgap. For this to occur, late-term growth must be in the intracluster light surrounding the BCG. We also compare the observed results to IllustrisTNG 300-1 cosmological hydrodynamic simulations and find modest qualitative agreement. However, the simulations lack the evolutionary features detected in the real data.},

  doi          = {10.3847/1538-4357/ac4cb4},

  journal      = {The Astrophysical Journal},

  number       = 1,

  volume       = 928,

  place        = {United States},

  year         = {Thu Mar 24 00:00:00 EDT 2022},

  month        = {Thu Mar 24 00:00:00 EDT 2022}

}

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Mind the gap: tightening the mass–richness relation with magnitude gaps
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Zu, Ying; Mandelbaum, Rachel
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Jones, L. R.; Ponman, T. J.; Forbes, D. A.
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Engler, Christoph; Pillepich, Annalisa; Joshi, Gandhali D.
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EzGal: A Flexible Interface for Stellar Population Synthesis Models
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Mancone, Conor L.; Gonzalez, Anthony H.
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Intracluster light at the Frontier – II. The Frontier Fields Clusters
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Murante, G.; Giovalli, M.; Gerhard, O.
Monthly Notices of the Royal Astronomical Society, Vol. 377, Issue 1
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Surface Brightness and Evolution of Galaxies
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Petrosian, Vahe
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Title: The Observed Evolution of the Stellar Mass–Halo Mass Relation for Brightest Central Galaxies

Abstract

Citation Formats

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The Eleventh and Twelfth data Releases of the Sloan Digital sky Survey: Final data from Sdss-Iii journal, July 2015

The dark Energy Camera journal, October 2015

The Masses of Nuclear Black Holes in Luminous Elliptical Galaxies and Implications for the Space Density of the Most Massive Black Holes journal, June 2007

emerge – an empirical model for the formation of galaxies since z ∼ 10 journal, March 2018

emcee : The MCMC Hammer journal, March 2013

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The ATLAS3D Project – XXX. Star formation histories and stellar population scaling relations of early-type galaxies journal, March 2015

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SPIDER - I. Sample and galaxy parameters in the grizYJHK wavebands: SPIDER - I. Sample and data analysis journal, September 2010

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The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colours of galaxies journal, January 2006

First results from the IllustrisTNG simulations: matter and galaxy clustering journal, December 2017

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journal, February 2011

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journal, December 2012

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journal, September 2005

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journal, March 2015

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journal, May 2019

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journal, May 2019

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journal, February 2021

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journal, January 2016

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journal, February 2007

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journal, June 1980

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journal, December 2014

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journal, April 2017

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journal, February 2020

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journal, June 2016

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journal, January 1984

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journal, April 2014

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journal, April 1989

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journal, June 2018

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journal, December 2016

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journal, June 2019

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journal, July 2015

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journal, June 2007

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journal, March 2013

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journal, January 2020

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journal, March 2015

The growth of intracluster light in XCS-HSC galaxy clusters from 0.1 < z < 0.5
journal, January 2021

Probing the galaxy–halo connection with total satellite luminosity
journal, June 2021

Luminous red galaxies in clusters: central occupation, spatial distributions and miscentring
journal, July 2015

Individual stellar haloes of massive galaxies measured to 100 kpc at 0.3 < z < 0.5 using Hyper Suprime-Cam
journal, December 2017

Closing the loop: a self-consistent model of optical, X-ray and Sunyaev–Zel'dovich scaling relations for clusters of Galaxies
journal, December 2013

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journal, March 2015

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journal, March 2020

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journal, May 2016

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journal, August 2007

The Dark Energy Survey: Data Release 1
journal, November 2018

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journal, April 1951

Fossil groups origins: I. RX J105453.3+552102 a very massive and relaxed system at z ~ 0.5
journal, February 2011

The Dark Energy Survey Image Processing Pipeline
journal, May 2018

The Luminosity Function and Stellar Evolution.
journal, January 1955

The Evolution of Brightest Cluster Galaxies in a Hierarchical Universe
journal, October 2012

THE AVERAGE STAR FORMATION HISTORIES OF GALAXIES IN DARK MATTER HALOS FROM z = 0-8
journal, May 2013

Hierarchical Galaxy Growth and Scatter in the Stellar Mass–Halo mass Relation
journal, December 2016

Formation channels of slowly rotating early-type galaxies
journal, March 2020

SPIDER - I. Sample and galaxy parameters in the grizYJHK wavebands: SPIDER - I. Sample and data analysis
journal, September 2010

The Stellar mass Growth of Brightest Cluster Galaxies in the irac Shallow Cluster Survey
journal, June 2013

Brightest group galaxies: stellar mass and star formation rate (paper I)
journal, March 2016

Constraining the galaxy–halo connection over the last 13.3 Gyr: star formation histories, galaxy mergers and structural properties
journal, May 2017

First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies
journal, December 2017

Populating a cluster of galaxies - I. Results at \fontshape{it}{z}=0
journal, December 2001

The Redmapper Galaxy Cluster Catalog from des Science Verification data
journal, May 2016

Do the stellar populations of the brightest two group galaxies depend on the magnitude gap?
journal, October 2016

The structure of brightest cluster members. I - Surface photometry
journal, January 1986

Galaxy Clusters Discovered via the Sunyaev-Zel'Dovich Effect in the 2500-Square-Degree Spt-Sz Survey
journal, January 2015

Stellar mass–halo mass relation for the brightest central galaxies of X-ray clusters since z ∼ 0.65
journal, November 2019

THE XMM CLUSTER SURVEY: THE STELLAR MASS ASSEMBLY OF FOSSIL GALAXIES
journal, May 2012

Dark Energy Survey Year 1 results: weak lensing mass calibration of redMaPPer galaxy clusters
journal, October 2018

Exploring relations between BCG and cluster properties in the SPectroscopic IDentification of eROSITA Sources survey from 0.05
journal, June 2018

THE GROWTH OF MASSIVE GALAXIES SINCE z = 2
journal, January 2010

Dark Energy Survey Year 1 Results: Detection of Intracluster Light at Redshift ∼ 0.25
journal, April 2019

Forward Global Photometric Calibration of the Dark Energy Survey
journal, December 2017

K ‐band Properties of Galaxy Clusters and Groups: Brightest Cluster Galaxies and Intracluster Light
journal, December 2004

μ⋆ masses: weak-lensing calibration of the Dark Energy Survey Year 1 redMaPPer clusters using stellar masses
journal, September 2020

The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colours of galaxies
journal, January 2006

First results from the IllustrisTNG simulations: matter and galaxy clustering
journal, December 2017

The Luminosities, Sizes, and Velocity Dispersions of Brightest Cluster Galaxies: Implications for Formation History
journal, March 2007

Simulating galaxy formation with the IllustrisTNG model
journal, October 2017

First Results on the Cluster Galaxy Population from the Subaru Hyper Suprime-Cam Survey. III. Brightest Cluster Galaxies, Stellar Mass Distribution, and Active Galaxies
journal, December 2017

Galaxy And Mass Assembly (GAMA): testing galaxy formation models through the most massive galaxies in the Universe
journal, March 2014

How special are brightest group and cluster galaxies?
journal, July 2007

The two Phases of Galaxy Formation
journal, December 2010

Galaxy Clusters Selected via the Sunyaev–Zel’dovich Effect in the SPTpol 100-square-degree Survey
journal, February 2020

Spatial kinematics of Brightest Cluster Galaxies and their close companions from Integral Field Unit spectroscopy★: Spatial kinematics of BCGs
journal, May 2011

Stellar population synthesis at the resolution of 2003
journal, October 2003