Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/31128
Campo DC | Valore | Lingua |
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dc.contributor.author | Umetsu, Keiichi | en_US |
dc.contributor.author | Sereno, Mauro | en_US |
dc.contributor.author | Lieu, Maggie | en_US |
dc.contributor.author | Miyatake, Hironao | en_US |
dc.contributor.author | Medezinski, Elinor | en_US |
dc.contributor.author | Nishizawa, Atsushi J. | en_US |
dc.contributor.author | Giles, Paul | en_US |
dc.contributor.author | GASTALDELLO, FABIO | en_US |
dc.contributor.author | McCarthy, Ian G. | en_US |
dc.contributor.author | Kilbinger, Martin | en_US |
dc.contributor.author | Birkinshaw, Mark | en_US |
dc.contributor.author | ETTORI, STEFANO | en_US |
dc.contributor.author | Okabe, Nobuhiro | en_US |
dc.contributor.author | Chiu, I. -Non | en_US |
dc.contributor.author | Coupon, Jean | en_US |
dc.contributor.author | Eckert, Dominique | en_US |
dc.contributor.author | Fujita, Yutaka | en_US |
dc.contributor.author | Higuchi, Yuichi | en_US |
dc.contributor.author | Koulouridis, Elias | en_US |
dc.contributor.author | Maughan, Ben | en_US |
dc.contributor.author | Miyazaki, Satoshi | en_US |
dc.contributor.author | Oguri, Masamune | en_US |
dc.contributor.author | Pacaud, Florian | en_US |
dc.contributor.author | Pierre, Marguerite | en_US |
dc.contributor.author | Rapetti, David | en_US |
dc.contributor.author | Smith, Graham P. | en_US |
dc.date.accessioned | 2021-11-23T14:27:01Z | - |
dc.date.available | 2021-11-23T14:27:01Z | - |
dc.date.issued | 2020 | en_US |
dc.identifier.issn | 0004-637X | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/31128 | - |
dc.description.abstract | We present a weak-lensing analysis of X-ray galaxy groups and clusters selected from the XMM-XXL survey using the first-year data from the Hyper Suprime-Cam (HSC) Subaru Strategic Program. Our joint weak-lensing and X-ray analysis focuses on 136 spectroscopically confirmed X-ray-selected systems at 0.031 ≤ z ≤ 1.033 detected in the 25 deg<SUP>2</SUP> XXL-N region, which largely overlaps with the HSC-XMM field. With high-quality HSC weak-lensing data, we characterize the mass distributions of individual clusters and establish the concentration-mass (c-M) relation for the XXL sample, by accounting for selection bias and statistical effects and marginalizing over the remaining mass calibration uncertainty. We find the mass-trend parameter of the c-M relation to be $\beta =-0.07\pm 0.28$ and the normalization to be ${c}_{200}=4.8\pm 1.0\,(\mathrm{stat})\pm 0.8\,(\mathrm{syst})$ at ${M}_{200}={10}^{14}\,{h}^{-1}\,{M}_{\odot }$ and z = 0.3. We find no statistical evidence for redshift evolution. Our weak-lensing results are in excellent agreement with dark-matter-only c-M relations calibrated for recent ΛCDM cosmologies. The level of intrinsic scatter in c<SUB>200</SUB> is constrained as $\sigma (\mathrm{ln}{c}_{200})\lt 24 \% $ ( $99.7 \% $ CL), which is smaller than predicted for the full population of ΛCDM halos. This is likely caused in part by the X-ray selection bias in terms of the cool-core or relaxation state. We determine the temperature-mass (T<SUB>X</SUB>-M<SUB>500</SUB>) relation for a subset of 105 XXL clusters that have both measured HSC lensing masses and X-ray temperatures. The resulting T<SUB>X</SUB>-M<SUB>500</SUB> relation is consistent with the self-similar prediction. Our T<SUB>X</SUB>-M<SUB>500</SUB> relation agrees with the XXL DR1 results at group scales but has a slightly steeper mass trend, implying a smaller mass scale in the cluster regime. The overall offset in the T<SUB>X</SUB>-M<SUB>500</SUB> relation is at the ∼1.5σ level, corresponding to a mean mass offset of $34 \% \pm 20 \% $ . We also provide bias-corrected, weak-lensing-calibrated M<SUB>200</SUB> and M<SUB>500</SUB> mass estimates of individual XXL clusters based on their measured X-ray temperatures. | en_US |
dc.language.iso | eng | en_US |
dc.title | Weak-lensing Analysis of X-Ray-selected XXL Galaxy Groups and Clusters with Subaru HSC Data | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.3847/1538-4357/ab6bca | en_US |
dc.identifier.url | https://iopscience.iop.org/article/10.3847/1538-4357/ab6bca | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 890 | en_US |
dc.relation.issue | 2 | en_US |
dc.relation.firstpage | 148 | en_US |
dc.type.referee | REF_1 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | THE ASTROPHYSICAL JOURNAL | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2020ApJ...890..148U | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation::PE9_9 Clusters of galaxies and large scale structures | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Article | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.orcid | 0000-0003-0302-0325 | - |
crisitem.author.orcid | 0000-0002-9112-0184 | - |
crisitem.journal.journalissn | 0004-637X | - |
crisitem.journal.ance | E016252 | - |
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1909.10524.pdf | preprint | 3.09 MB | Adobe PDF | Visualizza/apri |
Umetsu_2020_ApJ_890_148.pdf | [Administrators only] | 3.86 MB | Adobe PDF |
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