Panoramic Views of Cluster-Scale Assemblies Explored by Subaru Wide-Field Imaging
Author(s) -
Tadayuki Kodama,
Masayuki Tanaka,
Takayuki Tamura,
Hideki Yahagi,
Masahiro Nagashima,
Ichi Tanaka,
N. Arimoto,
Toshifumi Futamase,
Masanori Iye,
Yoshikazu Karasawa,
Nobunari Kashikawa,
Wataru Kawasaki,
Tetsu Kitayama,
Hideo Matsuhara,
Fumiaki Nakata,
Takaya Ohashi,
Kouji Ohta,
Takashi Okamoto,
Sadanori Okamura,
Kazuhiro Shimasaku,
Yasushi Suto,
Naoyuki Tamura,
Keiichi Umetsu,
Tōru Yamada
Publication year - 2005
Publication title -
publications of the astronomical society of japan
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.99
H-Index - 110
eISSN - 2053-051X
pISSN - 0004-6264
DOI - 10.1093/pasj/57.2.309
Subject(s) - physics , cluster (spacecraft) , astrophysics , redshift , galaxy cluster , galaxy , scale (ratio) , galaxy groups and clusters , field (mathematics) , computer science , mathematics , quantum mechanics , pure mathematics , programming language
We have started PISCES project; a panoramic imaging and spectroscopic surveyof distant clusters on Subaru. It exploits the unique wide-field imagingcapability of Suprime-Cam, which provides a 34'x27' field of view correspondingto a physical area of 16x13Mpc^2 at z~1. We plan to target 15 clusters in totalat 0.45Mpc from the cores, as well as complex innerstructures. The galaxy distributions in the inner regions of the clusters looksimilar to the X-ray intensity maps, suggesting that most of the opticalstructures trace physically bound systems. We also compared the structures ofthe three clusters with those of model clusters in a numerical simulation(N-body + semi-analytic model) by parameterising the shapes of the iso-densitycontours of galaxies, and found a broad agreement. Our results provide goodevidence that cluster-scale assembly takes place along filaments duringhierarchical clustering, while the structures found here need to be confirmedspectroscopically in the near future.Comment: 14 pages, 12 figures (of which 5 are provided in jpg format), uses pasj00.cls. PASJ in press. Proof corrected. Error in Fig.3 fixe
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