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Title: Mass calibration of the CODEX cluster sample using SPIDERS spectroscopy – II. The X-ray luminosity–mass relation

Abstract

ABSTRACT We perform the calibration of the X-ray luminosity–mass scaling relation on a sample of 344 CODEX clusters with z < 0.66 using the dynamics of their member galaxies. Spectroscopic follow-up measurements have been obtained from the SPIDERS survey, leading to a sample of 6658 red member galaxies. We use the Jeans equation to calculate halo masses, assuming an NFW mass profile and analysing a broad range of anisotropy profiles. With a scaling relation of the form $$L_{\rm {X}} \propto \text{A}_{\rm {X}}M_{\text{200c}}^{\text{B}_{\rm {X}}} E(z)^2 (1+z)^{\gamma _{\rm {X}}}$$, we find best-fitting parameters $$\text{A}_{\rm {X}}=0.62^{+0.05}_{-0.06} (\pm 0.06)\times 10^{44}\, \mathrm{erg\, s^{-1}}$$, $$\text{B}_{\rm {X}}=2.35^{+0.21}_{-0.18}(\pm 0.09)$$, $$\gamma _{\rm {X}}=-2.77^{+1.06}_{-1.05}(\pm 0.79)$$, where we include systematic uncertainties in parentheses and for a pivot mass and redshift of $$3\times 10^{14}\, \mathrm{M}_\odot$$ and 0.16, respectively. We compare our constraints with previous results, and we combine our sample with the SPT SZE-selected cluster subsample observed with XMM–Newton  extending the validity of our results to a wider range of redshifts and cluster masses.

Authors:
ORCiD logo [1];  [2];  [3];  [4];  [5];  [6];  [7];  [8];  [9];  [10];  [10];  [10]
  1. Faculty of Physics, Ludwig-Maximilians-Universität, Scheinerstr. 1, D-81679 Munich, Germany, Excellence Cluster Universe, Boltzmannstr. 2, D-85748 Garching, Germany, INAF-Osservatorio Astronomico di Trieste, via G. B. Tiepolo 11, I-34143 Trieste, Italy, IFPU - Institute for Fundamental Physics of the Universe, Via Beirut 2, I-34014 Trieste, Italy, The Oskar Klein Centre, Department of Physics, Stockholm University, Albanova University Center, SE-10691 Stockholm, Sweden
  2. Faculty of Physics, Ludwig-Maximilians-Universität, Scheinerstr. 1, D-81679 Munich, Germany, Excellence Cluster Universe, Boltzmannstr. 2, D-85748 Garching, Germany, Max Planck Institute for Extraterrestrial Physics, Giessenbachstr. D-85748 Garching, Germany
  3. INAF-Osservatorio Astronomico di Trieste, via G. B. Tiepolo 11, I-34143 Trieste, Italy, IFPU - Institute for Fundamental Physics of the Universe, Via Beirut 2, I-34014 Trieste, Italy, Astronomy Unit, Department of Physics, University of Trieste, via Tiepolo 11, I-34131 Trieste, Italy
  4. INAF-Osservatorio Astronomico di Trieste, via G. B. Tiepolo 11, I-34143 Trieste, Italy
  5. Max Planck Institute for Extraterrestrial Physics, Giessenbachstr. D-85748 Garching, Germany, IRAP, Université de Toulouse, CNRS, UPS, CNES, 31400 Toulouse, France
  6. Max Planck Institute for Extraterrestrial Physics, Giessenbachstr. D-85748 Garching, Germany, Department of Physics, University of Helsinki, Gustaf Hällströmin katu 2a, FI-00014 Helsinki, Finland
  7. Faculty of Physics, Ludwig-Maximilians-Universität, Scheinerstr. 1, D-81679 Munich, Germany, Max Planck Institute for Extraterrestrial Physics, Giessenbachstr. D-85748 Garching, Germany
  8. Faculty of Physics, Ludwig-Maximilians-Universität, Scheinerstr. 1, D-81679 Munich, Germany, Excellence Cluster Universe, Boltzmannstr. 2, D-85748 Garching, Germany
  9. Astrophysics Research Institute, Liverpool John Moores University, IC2, Liverpool Science Park, 146 Brownlow Hill, Liverpool, L3 5RF, UK
  10. Department of Physics, University of Helsinki, Gustaf Hällströmin katu 2a, FI-00014 Helsinki, Finland
Publication Date:
Sponsoring Org.:
USDOE
OSTI Identifier:
1615868
Resource Type:
Published Article
Journal Name:
Monthly Notices of the Royal Astronomical Society
Additional Journal Information:
Journal Name: Monthly Notices of the Royal Astronomical Society Journal Volume: 494 Journal Issue: 2; Journal ID: ISSN 0035-8711
Publisher:
Oxford University Press
Country of Publication:
United Kingdom
Language:
English

Citation Formats

Capasso, R., Mohr, J. J., Saro, A., Biviano, A., Clerc, N., Finoguenov, A., Klein, M., Grandis, S., Collins, C., Damsted, S., Kirkpatrick, C., and Kukkola, A. Mass calibration of the CODEX cluster sample using SPIDERS spectroscopy – II. The X-ray luminosity–mass relation. United Kingdom: N. p., 2020. Web. doi:10.1093/mnras/staa888.
Capasso, R., Mohr, J. J., Saro, A., Biviano, A., Clerc, N., Finoguenov, A., Klein, M., Grandis, S., Collins, C., Damsted, S., Kirkpatrick, C., & Kukkola, A. Mass calibration of the CODEX cluster sample using SPIDERS spectroscopy – II. The X-ray luminosity–mass relation. United Kingdom. doi:https://doi.org/10.1093/mnras/staa888
Capasso, R., Mohr, J. J., Saro, A., Biviano, A., Clerc, N., Finoguenov, A., Klein, M., Grandis, S., Collins, C., Damsted, S., Kirkpatrick, C., and Kukkola, A. Tue . "Mass calibration of the CODEX cluster sample using SPIDERS spectroscopy – II. The X-ray luminosity–mass relation". United Kingdom. doi:https://doi.org/10.1093/mnras/staa888.
@article{osti_1615868,
title = {Mass calibration of the CODEX cluster sample using SPIDERS spectroscopy – II. The X-ray luminosity–mass relation},
author = {Capasso, R. and Mohr, J. J. and Saro, A. and Biviano, A. and Clerc, N. and Finoguenov, A. and Klein, M. and Grandis, S. and Collins, C. and Damsted, S. and Kirkpatrick, C. and Kukkola, A.},
abstractNote = {ABSTRACT We perform the calibration of the X-ray luminosity–mass scaling relation on a sample of 344 CODEX clusters with z < 0.66 using the dynamics of their member galaxies. Spectroscopic follow-up measurements have been obtained from the SPIDERS survey, leading to a sample of 6658 red member galaxies. We use the Jeans equation to calculate halo masses, assuming an NFW mass profile and analysing a broad range of anisotropy profiles. With a scaling relation of the form $L_{\rm {X}} \propto \text{A}_{\rm {X}}M_{\text{200c}}^{\text{B}_{\rm {X}}} E(z)^2 (1+z)^{\gamma _{\rm {X}}}$, we find best-fitting parameters $\text{A}_{\rm {X}}=0.62^{+0.05}_{-0.06} (\pm 0.06)\times 10^{44}\, \mathrm{erg\, s^{-1}}$, $\text{B}_{\rm {X}}=2.35^{+0.21}_{-0.18}(\pm 0.09)$, $\gamma _{\rm {X}}=-2.77^{+1.06}_{-1.05}(\pm 0.79)$, where we include systematic uncertainties in parentheses and for a pivot mass and redshift of $3\times 10^{14}\, \mathrm{M}_\odot$ and 0.16, respectively. We compare our constraints with previous results, and we combine our sample with the SPT SZE-selected cluster subsample observed with XMM–Newton  extending the validity of our results to a wider range of redshifts and cluster masses.},
doi = {10.1093/mnras/staa888},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 2,
volume = 494,
place = {United Kingdom},
year = {2020},
month = {4}
}

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DOI: https://doi.org/10.1093/mnras/staa888

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