X-ray properties of high-richness CAMIRA clusters in the Hyper Suprime-Cam Subaru Strategic Program field
Abstract
Abstract We present the first results of a pilot X-ray study of 37 rich galaxy clusters at 0.1 < z < 1.1 in the Hyper Suprime-Cam Subaru Strategic Program field. Diffuse X-ray emissions from these clusters were serendipitously detected in the XMM-Newton fields of view. We systematically analyze X-ray images of 37 clusters and emission spectra of a subsample of 17 clusters with high photon statistics by using the XMM-Newton archive data. The frequency distribution of the offset between the X-ray centroid or peak and the position of the brightest cluster galaxy was derived for the optical cluster sample. The fraction of relaxed clusters estimated from the X-ray peak offsets in 17 clusters is 29 ± 11(±13)%, which is smaller than that of the X-ray cluster samples such as HIFLUGCS. Since the optical cluster search is immune to the physical state of X-ray-emitting gas, it is likely to cover a larger range of the cluster morphology. We also derive the luminosity–temperature relation and found that the slope is marginally shallower than those of X-ray-selected samples and consistent with the self-similar model prediction of 2. Accordingly, our results show that the X-ray properties of the optical clusters are marginally different from thosemore »
- Publication Date:
- Sponsoring Org.:
- USDOE
- OSTI Identifier:
- 1573429
- Resource Type:
- Published Article
- Journal Name:
- Publications of the Astronomical Society of Japan
- Additional Journal Information:
- Journal Name: Publications of the Astronomical Society of Japan Journal Volume: 72 Journal Issue: 1; Journal ID: ISSN 0004-6264
- Publisher:
- Oxford University Press
- Country of Publication:
- Japan
- Language:
- English
Citation Formats
Ota, Naomi, Mitsuishi, Ikuyuki, Babazaki, Yasunori, Akamatsu, Hiroki, Ichinohe, Yuto, Ueda, Shutaro, Okabe, Nobuhiro, Oguri, Masamune, Fujimoto, Ryuichi, Hamana, Takashi, Miyaoka, Keita, Miyazaki, Satoshi, Otani, Hanae, Tanaka, Keigo, Tsuji, Ayumi, and Yoshida, Atsushi. X-ray properties of high-richness CAMIRA clusters in the Hyper Suprime-Cam Subaru Strategic Program field. Japan: N. p., 2019.
Web. doi:10.1093/pasj/psz118.
Ota, Naomi, Mitsuishi, Ikuyuki, Babazaki, Yasunori, Akamatsu, Hiroki, Ichinohe, Yuto, Ueda, Shutaro, Okabe, Nobuhiro, Oguri, Masamune, Fujimoto, Ryuichi, Hamana, Takashi, Miyaoka, Keita, Miyazaki, Satoshi, Otani, Hanae, Tanaka, Keigo, Tsuji, Ayumi, & Yoshida, Atsushi. X-ray properties of high-richness CAMIRA clusters in the Hyper Suprime-Cam Subaru Strategic Program field. Japan. https://doi.org/10.1093/pasj/psz118
Ota, Naomi, Mitsuishi, Ikuyuki, Babazaki, Yasunori, Akamatsu, Hiroki, Ichinohe, Yuto, Ueda, Shutaro, Okabe, Nobuhiro, Oguri, Masamune, Fujimoto, Ryuichi, Hamana, Takashi, Miyaoka, Keita, Miyazaki, Satoshi, Otani, Hanae, Tanaka, Keigo, Tsuji, Ayumi, and Yoshida, Atsushi. Thu .
"X-ray properties of high-richness CAMIRA clusters in the Hyper Suprime-Cam Subaru Strategic Program field". Japan. https://doi.org/10.1093/pasj/psz118.
@article{osti_1573429,
title = {X-ray properties of high-richness CAMIRA clusters in the Hyper Suprime-Cam Subaru Strategic Program field},
author = {Ota, Naomi and Mitsuishi, Ikuyuki and Babazaki, Yasunori and Akamatsu, Hiroki and Ichinohe, Yuto and Ueda, Shutaro and Okabe, Nobuhiro and Oguri, Masamune and Fujimoto, Ryuichi and Hamana, Takashi and Miyaoka, Keita and Miyazaki, Satoshi and Otani, Hanae and Tanaka, Keigo and Tsuji, Ayumi and Yoshida, Atsushi},
abstractNote = {Abstract We present the first results of a pilot X-ray study of 37 rich galaxy clusters at 0.1 < z < 1.1 in the Hyper Suprime-Cam Subaru Strategic Program field. Diffuse X-ray emissions from these clusters were serendipitously detected in the XMM-Newton fields of view. We systematically analyze X-ray images of 37 clusters and emission spectra of a subsample of 17 clusters with high photon statistics by using the XMM-Newton archive data. The frequency distribution of the offset between the X-ray centroid or peak and the position of the brightest cluster galaxy was derived for the optical cluster sample. The fraction of relaxed clusters estimated from the X-ray peak offsets in 17 clusters is 29 ± 11(±13)%, which is smaller than that of the X-ray cluster samples such as HIFLUGCS. Since the optical cluster search is immune to the physical state of X-ray-emitting gas, it is likely to cover a larger range of the cluster morphology. We also derive the luminosity–temperature relation and found that the slope is marginally shallower than those of X-ray-selected samples and consistent with the self-similar model prediction of 2. Accordingly, our results show that the X-ray properties of the optical clusters are marginally different from those observed in the X-ray samples. The implication of the results and future prospects are briefly discussed.},
doi = {10.1093/pasj/psz118},
journal = {Publications of the Astronomical Society of Japan},
number = 1,
volume = 72,
place = {Japan},
year = {Thu Nov 07 00:00:00 EST 2019},
month = {Thu Nov 07 00:00:00 EST 2019}
}
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