LoCuSS: A COMPARISON OF CLUSTER MASS MEASUREMENTS FROM XMM-NEWTON AND SUBARU—TESTING DEVIATION FROM HYDROSTATIC EQUILIBRIUM AND NON-THERMAL PRESSURE SUPPORT
The Astrophysical Journal 711 巻 2 号
1033-1043 頁
2010-03-10 発行
アクセス数 : 611 件
ダウンロード数 : 154 件
今月のアクセス数 : 5 件
今月のダウンロード数 : 4 件
この文献の参照には次のURLをご利用ください : https://ir.lib.hiroshima-u.ac.jp/00047040
ファイル情報(添付) |
ApJ_711_1033.pdf
375 KB
種類 :
全文
|
タイトル ( eng ) |
LoCuSS: A COMPARISON OF CLUSTER MASS MEASUREMENTS FROM XMM-NEWTON AND SUBARU—TESTING DEVIATION FROM HYDROSTATIC EQUILIBRIUM AND NON-THERMAL PRESSURE SUPPORT
|
作成者 |
Zhang Yu-Ying
Finoguenov Alexis
Smith Graham P.
Piffaretti Rocco
Valdarnini Riccardo
Babul Arif
Evrard August E.
Mazzotta Pasquale
Sanderson Alastair J. R.
Marrone Daniel P.
|
収録物名 |
The Astrophysical Journal
|
巻 | 711 |
号 | 2 |
開始ページ | 1033 |
終了ページ | 1043 |
抄録 |
We compare X-ray hydrostatic and weak-lensing mass estimates for a sample of 12 clusters that have been observed with both XMM-Newton and Subaru. At an over-density of Δ = 500, we obtain 1 − MX/MWL = 0.01 ± 0.07 for the whole sample. We also divided the sample into undisturbed and disturbed sub-samples based on quantitative X-ray morphologies using asymmetry and fluctuation parameters, obtaining 1 − MX/MWL = 0.09 ± 0.06 and −0.06 ± 0.12 for the undisturbed and disturbed clusters, respectively. In addition to non-thermal pressure support, there may be a competing effect associated with adiabatic compression and/or shock heating which leads to overestimate of X-ray hydrostatic masses for disturbed clusters, for example, in the famous merging cluster A1914. Despite the modest statistical significance of the mass discrepancy, on average, in the undisturbed clusters, we detect a clear trend of improving agreement between MX and MWL as a function of increasing overdensity, MX/MWL = (0.908 ± 0.004) + (0.187 ± 0.010) · log10(Δ/500). We also examine the gas mass fractions, fgas = Mgas/MWL, finding that they are an increasing function of cluster radius, with no dependence on dynamical state, in agreement with predictions from numerical simulations.Overall, our results demonstrate that XMM-Newton and Subaru are a powerful combination for calibrating systematic uncertainties in cluster mass measurements.
|
著者キーワード |
cosmology: observations – galaxies: clusters: general – galaxies: clusters: individual (Abell 1914) – gravitational lensing: weak – surveys – X-rays: galaxies: clusters
|
内容記述 |
We acknowledge support from KICP in Chicago for hospitality, and thank our LoCuSS collaborators, especially Masahiro Takada and Keiichi Umetsu, for helpful comments on the
manuscript. Y.Y.Z. thanks Massimo Meneghetti and Gabriel Pratt for useful discussion. Y.Y.Z. acknowledges support by the DFG through Emmy Noether Research Grant RE 1462/ 2, through Schwerpunkt Program 1177, and through project B6 “Gravitational Lensing and X-ray Emission by Non-Linear Structures” of Transregional Collaborative Research Centre TRR 33 The Dark Universe, and support by the German BMBF through the Verbundforschung under grant 50 OR 0601. This work is supported by a Grant-in-Aid for the COE Program “Exploring New Science by Bridging Particle-Matter Hierarchy” and G-COE Program “Weaving Science Web beyond Particle-Matter Hierarchy” in Tohoku University, funded by theMinistry of Education, Science, Sports and Culture of Japan. This work is, in part, supported by a Grant-in-Aid for Science Research in a Priority Area “Probing the Dark Energy through an Extremely Wide and Deep Survey with Subaru Telescope” (18072001) from the Ministry of Education, Culture, Sports, Science, and Technology of Japan. N.O. is, in part, supported by a Grant-in-Aid from the Ministry of Education, Culture, Sports, Science, and Technology of Japan (20740099). A.F. acknowledges support from BMBF/DLR under grant 50 OR 0207 and MPG, and was partially supported by a NASA grant NNX08AX46G to UMBC. G.P.S. acknowledges support from the Royal Society and STFC. D.P.M. acknowledges support provided by NASA through Hubble Fellowship grant HF-51259.01 awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS 5-26555. |
NDC分類 |
天文学・宇宙科学 [ 440 ]
|
言語 |
英語
|
資源タイプ | 学術雑誌論文 |
出版者 |
IOP Publishing
|
発行日 | 2010-03-10 |
権利情報 |
© 2010. The American Astronomical Society. All rights reserved.
|
出版タイプ | Version of Record(出版社版。早期公開を含む) |
アクセス権 | オープンアクセス |
収録物識別子 |
[ISSN] 0004-637X
[ISSN] 1538-4357
[NCID] AA00553253
[DOI] 10.1088/0004-637X/711/2/1033
[DOI] https://doi.org/10.1088/0004-637X/711/2/1033
|