CLASH: The CONCENTRATION-MASS RELATION of GALAXY CLUSTERS

J. Merten; M. Meneghetti; M. Postman; K. Umetsu; A. Zitrin; E. Medezinski; M. Nonino; A. Koekemoer; P. Melchior; D. Gruen; L. A. Moustakas; M. Bartelmann; O. Host; M. Donahue; D. Coe; A. Molino; S. Jouvel; A. Monna; S. Seitz; N. Czakon; D. Lemze; J. Sayers; I. Balestra; P. Rosati; N. Benítez; A. Biviano; R. Bouwens; L. Bradley; T. Broadhurst; M. Carrasco; H. Ford; C. Grillo; L. Infante; D. Kelson; O. Lahav; R. Massey; J. Moustakas; E. Rasia; J. Rhodes; J. Vega; W. Zheng

doi:10.1088/0004-637X/806/1/4

CLASH: The CONCENTRATION-MASS RELATION of GALAXY CLUSTERS

J. Merten
, M. Meneghetti
, M. Postman
, K. Umetsu
, A. Zitrin
, E. Medezinski
, M. Nonino
, A. Koekemoer
, P. Melchior
, D. Gruen
, L. A. Moustakas
, M. Bartelmann
, O. Host
, M. Donahue
, D. Coe
, A. Molino
, S. Jouvel
, A. Monna
, S. Seitz
, N. Czakon

D. Lemze, J. Sayers, I. Balestra, P. Rosati, N. Benítez, A. Biviano, R. Bouwens, L. Bradley, T. Broadhurst, M. Carrasco, H. Ford, C. Grillo, L. Infante, D. Kelson, O. Lahav, R. Massey, J. Moustakas, E. Rasia, J. Rhodes, J. Vega, W. Zheng

Research output: Contribution to journal › Article › peer-review

186 Scopus citations

Abstract

We present a new determination of the concentration-mass (c-M) relation for galaxy clusters based on our comprehensive lensing analysis of 19 X-ray selected galaxy clusters from the Cluster Lensing and Supernova Survey with Hubble (CLASH). Our sample spans a redshift range between 0.19 and 0.89. We combine weak-lensing constraints from the Hubble Space Telescope (HST) and from ground-based wide-field data with strong lensing constraints from HST. The results are reconstructions of the surface-mass density for all CLASH clusters on multi-scale grids. Our derivation of Navarro-Frenk-White parameters yields virial masses between and and the halo concentrations are distributed around with a significant negative slope with cluster mass. We find an excellent 4% agreement in the median ratio of our measured concentrations for each cluster and the respective expectation from numerical simulations after accounting for the CLASH selection function based on X-ray morphology. The simulations are analyzed in two dimensions to account for possible biases in the lensing reconstructions due to projection effects. The theoretical c-M relation from our X-ray selected set of simulated clusters and the c-M relation derived directly from the CLASH data agree at the 90% confidence level.

Original language	English (US)
Article number	4
Journal	Astrophysical Journal
Volume	806
Issue number	1
DOIs	https://doi.org/10.1088/0004-637X/806/1/4
State	Published - Jun 10 2015
Externally published	Yes

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

Keywords

dark matter
galaxies: clusters: general
gravitational lensing: strong
gravitational lensing: weak

Access to Document

10.1088/0004-637X/806/1/4

Cite this

Merten, J., Meneghetti, M., Postman, M., Umetsu, K., Zitrin, A., Medezinski, E., Nonino, M., Koekemoer, A., Melchior, P., Gruen, D., Moustakas, L. A., Bartelmann, M., Host, O., Donahue, M., Coe, D., Molino, A., Jouvel, S., Monna, A., Seitz, S., ... Zheng, W. (2015). CLASH: The CONCENTRATION-MASS RELATION of GALAXY CLUSTERS. Astrophysical Journal, 806(1), Article 4. https://doi.org/10.1088/0004-637X/806/1/4

@article{6c87447fb83b48b7814a54451d61e6f2,

title = "CLASH: The CONCENTRATION-MASS RELATION of GALAXY CLUSTERS",

abstract = "We present a new determination of the concentration-mass (c-M) relation for galaxy clusters based on our comprehensive lensing analysis of 19 X-ray selected galaxy clusters from the Cluster Lensing and Supernova Survey with Hubble (CLASH). Our sample spans a redshift range between 0.19 and 0.89. We combine weak-lensing constraints from the Hubble Space Telescope (HST) and from ground-based wide-field data with strong lensing constraints from HST. The results are reconstructions of the surface-mass density for all CLASH clusters on multi-scale grids. Our derivation of Navarro-Frenk-White parameters yields virial masses between and and the halo concentrations are distributed around with a significant negative slope with cluster mass. We find an excellent 4\% agreement in the median ratio of our measured concentrations for each cluster and the respective expectation from numerical simulations after accounting for the CLASH selection function based on X-ray morphology. The simulations are analyzed in two dimensions to account for possible biases in the lensing reconstructions due to projection effects. The theoretical c-M relation from our X-ray selected set of simulated clusters and the c-M relation derived directly from the CLASH data agree at the 90\% confidence level.",

keywords = "dark matter, galaxies: clusters: general, gravitational lensing: strong, gravitational lensing: weak",

author = "J. Merten and M. Meneghetti and M. Postman and K. Umetsu and A. Zitrin and E. Medezinski and M. Nonino and A. Koekemoer and P. Melchior and D. Gruen and Moustakas, \{L. A.\} and M. Bartelmann and O. Host and M. Donahue and D. Coe and A. Molino and S. Jouvel and A. Monna and S. Seitz and N. Czakon and D. Lemze and J. Sayers and I. Balestra and P. Rosati and N. Ben{\'i}tez and A. Biviano and R. Bouwens and L. Bradley and T. Broadhurst and M. Carrasco and H. Ford and C. Grillo and L. Infante and D. Kelson and O. Lahav and R. Massey and J. Moustakas and E. Rasia and J. Rhodes and J. Vega and W. Zheng",

year = "2015",

month = jun,

day = "10",

doi = "10.1088/0004-637X/806/1/4",

language = "English (US)",

volume = "806",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "American Astronomical Society",

number = "1",

}

Merten, J, Meneghetti, M, Postman, M, Umetsu, K, Zitrin, A, Medezinski, E, Nonino, M, Koekemoer, A, Melchior, P, Gruen, D, Moustakas, LA, Bartelmann, M, Host, O, Donahue, M, Coe, D, Molino, A, Jouvel, S, Monna, A, Seitz, S, Czakon, N, Lemze, D, Sayers, J, Balestra, I, Rosati, P, Benítez, N, Biviano, A, Bouwens, R, Bradley, L, Broadhurst, T, Carrasco, M, Ford, H, Grillo, C, Infante, L, Kelson, D, Lahav, O, Massey, R, Moustakas, J, Rasia, E, Rhodes, J, Vega, J & Zheng, W 2015, 'CLASH: The CONCENTRATION-MASS RELATION of GALAXY CLUSTERS', Astrophysical Journal, vol. 806, no. 1, 4. https://doi.org/10.1088/0004-637X/806/1/4

TY - JOUR

T1 - CLASH

T2 - The CONCENTRATION-MASS RELATION of GALAXY CLUSTERS

AU - Merten, J.

AU - Meneghetti, M.

AU - Postman, M.

AU - Umetsu, K.

AU - Zitrin, A.

AU - Medezinski, E.

AU - Nonino, M.

AU - Koekemoer, A.

AU - Melchior, P.

AU - Gruen, D.

AU - Moustakas, L. A.

AU - Bartelmann, M.

AU - Host, O.

AU - Donahue, M.

AU - Coe, D.

AU - Molino, A.

AU - Jouvel, S.

AU - Monna, A.

AU - Seitz, S.

AU - Czakon, N.

AU - Lemze, D.

AU - Sayers, J.

AU - Balestra, I.

AU - Rosati, P.

AU - Benítez, N.

AU - Biviano, A.

AU - Bouwens, R.

AU - Bradley, L.

AU - Broadhurst, T.

AU - Carrasco, M.

AU - Ford, H.

AU - Grillo, C.

AU - Infante, L.

AU - Kelson, D.

AU - Lahav, O.

AU - Massey, R.

AU - Moustakas, J.

AU - Rasia, E.

AU - Rhodes, J.

AU - Vega, J.

AU - Zheng, W.

PY - 2015/6/10

Y1 - 2015/6/10

N2 - We present a new determination of the concentration-mass (c-M) relation for galaxy clusters based on our comprehensive lensing analysis of 19 X-ray selected galaxy clusters from the Cluster Lensing and Supernova Survey with Hubble (CLASH). Our sample spans a redshift range between 0.19 and 0.89. We combine weak-lensing constraints from the Hubble Space Telescope (HST) and from ground-based wide-field data with strong lensing constraints from HST. The results are reconstructions of the surface-mass density for all CLASH clusters on multi-scale grids. Our derivation of Navarro-Frenk-White parameters yields virial masses between and and the halo concentrations are distributed around with a significant negative slope with cluster mass. We find an excellent 4% agreement in the median ratio of our measured concentrations for each cluster and the respective expectation from numerical simulations after accounting for the CLASH selection function based on X-ray morphology. The simulations are analyzed in two dimensions to account for possible biases in the lensing reconstructions due to projection effects. The theoretical c-M relation from our X-ray selected set of simulated clusters and the c-M relation derived directly from the CLASH data agree at the 90% confidence level.

AB - We present a new determination of the concentration-mass (c-M) relation for galaxy clusters based on our comprehensive lensing analysis of 19 X-ray selected galaxy clusters from the Cluster Lensing and Supernova Survey with Hubble (CLASH). Our sample spans a redshift range between 0.19 and 0.89. We combine weak-lensing constraints from the Hubble Space Telescope (HST) and from ground-based wide-field data with strong lensing constraints from HST. The results are reconstructions of the surface-mass density for all CLASH clusters on multi-scale grids. Our derivation of Navarro-Frenk-White parameters yields virial masses between and and the halo concentrations are distributed around with a significant negative slope with cluster mass. We find an excellent 4% agreement in the median ratio of our measured concentrations for each cluster and the respective expectation from numerical simulations after accounting for the CLASH selection function based on X-ray morphology. The simulations are analyzed in two dimensions to account for possible biases in the lensing reconstructions due to projection effects. The theoretical c-M relation from our X-ray selected set of simulated clusters and the c-M relation derived directly from the CLASH data agree at the 90% confidence level.

KW - dark matter

KW - galaxies: clusters: general

KW - gravitational lensing: strong

KW - gravitational lensing: weak

UR - https://www.scopus.com/pages/publications/84934933322

UR - https://www.scopus.com/pages/publications/84934933322#tab=citedBy

U2 - 10.1088/0004-637X/806/1/4

DO - 10.1088/0004-637X/806/1/4

M3 - Article

AN - SCOPUS:84934933322

SN - 0004-637X

VL - 806

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 1

M1 - 4

ER -

CLASH: The CONCENTRATION-MASS RELATION of GALAXY CLUSTERS

Abstract

All Science Journal Classification (ASJC) codes

Keywords

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