CLASH: Joint analysis of strong-lensing, weak-lensing shear, and magnification data for 20 galaxy clusters*
Abstract
Here, we present a comprehensive analysis of strong-lensing, weak-lensing shear and magnification data for a sample of 16 X-ray-regular and 4 high-magnification galaxy clusters at $$0.19\lesssim z\lesssim 0.69$$ selected from Cluster Lensing And Supernova survey with Hubble (CLASH). Our analysis combines constraints from 16-band Hubble Space Telescope observations and wide-field multi-color imaging taken primarily with Suprime-Cam on the Subaru Telescope, spanning a wide range of cluster radii (10''–16'). We reconstruct surface mass density profiles of individual clusters from a joint analysis of the full lensing constraints, and determine masses and concentrations for all of the clusters. We find the internal consistency of the ensemble mass calibration to be ≤5% ± 6% in the one-halo regime (200–2000 kpc h–1) compared to the CLASH weak-lensing-only measurements of Umetsu et al. For the X-ray-selected subsample of 16 clusters, we examine the concentration–mass (c–M) relation and its intrinsic scatter using a Bayesian regression approach. Our model yields a mean concentration of $$c{| }_{z=0.34}=3.95\pm 0.35$$ at M200c sime 14 × 1014 M⊙ and an intrinsic scatter of $$\sigma (\mathrm{ln}{c}_{200{\rm{c}}})=0.13\pm 0.06$$, which is in excellent agreement with Λ cold dark matter predictions when the CLASH selection function based on X-ray morphological regularity and the projection effects are taken into account. We also derive an ensemble-averaged surface mass density profile for the X-ray-selected subsample by stacking their individual profiles. The stacked lensing signal is detected at 33σ significance over the entire radial range ≤4000 kpc h–1, accounting for the effects of intrinsic profile variations and uncorrelated large-scale structure along the line of sight. The stacked mass profile is well described by a family of density profiles predicted for cuspy dark-matter-dominated halos in gravitational equilibrium, namely, the Navarro–Frenk–White (NFW), Einasto, and DARKexp models, whereas the single power-law, cored isothermal and Burkert density profiles are disfavored by the data. We show that cuspy halo models that include the large-scale two-halo term provide improved agreement with the data. For the NFW halo model, we measure a mean concentration of $${c}_{200{\rm{c}}}={3.79}_{-0.28}^{+0.30}$$ at $${M}_{200{\rm{c}}}={14.1}_{-1.0}^{+1.0}\times {10}^{14}\;{M}_{\odot }$$, demonstrating consistency between the complementary analysis methods.
- Authors:
-
[1];
[2];
[5];
- Academia Sinica, Taipei (Taiwan)
- California Inst. of Technology (CalTech), Pasadena, CA (United States)
- Univ.-Sternwarte, Munchen (Germany); Max-Planck-Institut fur extraterrestrische Physik, Garching (Germany); SLAC National Accelerator Lab., Menlo Park, CA (United States); Stanford Univ., Palo Alto, CA (United States)
- Univ. of Oxford, Oxford (United Kingdom)
- Michigan State Univ., East Lansing, MI (United States)
- Space Telescope Science Institute, Baltimore, MD (United States)
- Publication Date:
- Research Org.:
- SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
- Sponsoring Org.:
- USDOE
- OSTI Identifier:
- 1333874
- Report Number(s):
- 1333874
Journal ID: ISSN 1538-4357
- Grant/Contract Number:
- AC02-76SF00515
- Resource Type:
- Accepted Manuscript
- Journal Name:
- The Astrophysical Journal (Online)
- Additional Journal Information:
- Journal Name: The Astrophysical Journal (Online); Journal Volume: 821; Journal Issue: 2; Journal ID: ISSN 1538-4357
- Publisher:
- Institute of Physics (IOP)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; cosmology: observations; dark matter; galaxies: clusters: general; gravitational lensing: strong; gravitational lensing: weak
Citation Formats
Umetsu, Keiichi, Zitrin, Adi, Gruen, Daniel, Merten, Julian, Donahue, Megan, and Postman, Marc. CLASH: Joint analysis of strong-lensing, weak-lensing shear, and magnification data for 20 galaxy clusters*. United States: N. p., 2016.
Web. doi:10.3847/0004-637X/821/2/116.
Umetsu, Keiichi, Zitrin, Adi, Gruen, Daniel, Merten, Julian, Donahue, Megan, & Postman, Marc. CLASH: Joint analysis of strong-lensing, weak-lensing shear, and magnification data for 20 galaxy clusters*. United States. https://doi.org/10.3847/0004-637X/821/2/116
Umetsu, Keiichi, Zitrin, Adi, Gruen, Daniel, Merten, Julian, Donahue, Megan, and Postman, Marc. Wed .
"CLASH: Joint analysis of strong-lensing, weak-lensing shear, and magnification data for 20 galaxy clusters*". United States. https://doi.org/10.3847/0004-637X/821/2/116. https://www.osti.gov/servlets/purl/1333874.
@article{osti_1333874,
title = {CLASH: Joint analysis of strong-lensing, weak-lensing shear, and magnification data for 20 galaxy clusters*},
author = {Umetsu, Keiichi and Zitrin, Adi and Gruen, Daniel and Merten, Julian and Donahue, Megan and Postman, Marc},
abstractNote = {Here, we present a comprehensive analysis of strong-lensing, weak-lensing shear and magnification data for a sample of 16 X-ray-regular and 4 high-magnification galaxy clusters at $0.19\lesssim z\lesssim 0.69$ selected from Cluster Lensing And Supernova survey with Hubble (CLASH). Our analysis combines constraints from 16-band Hubble Space Telescope observations and wide-field multi-color imaging taken primarily with Suprime-Cam on the Subaru Telescope, spanning a wide range of cluster radii (10''–16'). We reconstruct surface mass density profiles of individual clusters from a joint analysis of the full lensing constraints, and determine masses and concentrations for all of the clusters. We find the internal consistency of the ensemble mass calibration to be ≤5% ± 6% in the one-halo regime (200–2000 kpc h–1) compared to the CLASH weak-lensing-only measurements of Umetsu et al. For the X-ray-selected subsample of 16 clusters, we examine the concentration–mass (c–M) relation and its intrinsic scatter using a Bayesian regression approach. Our model yields a mean concentration of $c{| }_{z=0.34}=3.95\pm 0.35$ at M200c sime 14 × 1014 M⊙ and an intrinsic scatter of $\sigma (\mathrm{ln}{c}_{200{\rm{c}}})=0.13\pm 0.06$, which is in excellent agreement with Λ cold dark matter predictions when the CLASH selection function based on X-ray morphological regularity and the projection effects are taken into account. We also derive an ensemble-averaged surface mass density profile for the X-ray-selected subsample by stacking their individual profiles. The stacked lensing signal is detected at 33σ significance over the entire radial range ≤4000 kpc h–1, accounting for the effects of intrinsic profile variations and uncorrelated large-scale structure along the line of sight. The stacked mass profile is well described by a family of density profiles predicted for cuspy dark-matter-dominated halos in gravitational equilibrium, namely, the Navarro–Frenk–White (NFW), Einasto, and DARKexp models, whereas the single power-law, cored isothermal and Burkert density profiles are disfavored by the data. We show that cuspy halo models that include the large-scale two-halo term provide improved agreement with the data. For the NFW halo model, we measure a mean concentration of ${c}_{200{\rm{c}}}={3.79}_{-0.28}^{+0.30}$ at ${M}_{200{\rm{c}}}={14.1}_{-1.0}^{+1.0}\times {10}^{14}\;{M}_{\odot }$, demonstrating consistency between the complementary analysis methods.},
doi = {10.3847/0004-637X/821/2/116},
journal = {The Astrophysical Journal (Online)},
number = 2,
volume = 821,
place = {United States},
year = {Wed Apr 20 00:00:00 EDT 2016},
month = {Wed Apr 20 00:00:00 EDT 2016}
}
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