PROPERTIES of WEAK LENSING CLUSTERS DETECTED on HYPER SUPRIME-CAM's 2.3 deg2 FIELD

Satoshi Miyazaki, Masamune Oguri, Takashi Hamana, Masayuki Tanaka, Lance Miller, Yousuke Utsumi, Yutaka Komiyama, Hisanori Furusawa, Junya Sakurai, Satoshi Kawanomoto, Fumiaki Nakata, Fumihiro Uraguchi, Michitaro Koike, Daigo Tomono, Robert Lupton, James E. Gunn, Hiroshi Karoji, Hiroaki Aihara, Hitoshi Murayama, Masahiro Takada

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36 Scopus citations

Abstract

We present properties of moderately massive clusters of galaxies detected by the newly developed Hyper Suprime-Cam on the Subaru telescope using weak gravitational lensing. Eight peaks exceeding a signal-to-noise ratio (S/N) of 4.5 are identified on the convergence S/N map of a 2.3 deg2 field observed during the early commissioning phase of the camera. Multi-color photometric data are used to generate optically selected clusters using the Cluster finding algorithm based on the Multiband Identification of Red-sequence galaxies algorithm. The optical cluster positions were correlated with the peak positions from the convergence map. All eight significant peaks have optical counterparts. The velocity dispersion of clusters is evaluated by adopting the Singular Isothemal Sphere fit to the tangential shear profiles, yielding virial mass estimates, M500c, of the clusters which range from 2.7 × 1013 to 4.4 × 10 M. The number of peaks is considerably larger than the average number expected from ΛCDM cosmology but this is not extremely unlikely if one takes the large sample variance in the small field into account. We could, however, safely argue that the peak count strongly favors the recent Planck result suggesting a high value of 0.83. The ratio of stellar mass to the dark matter halo mass shows a clear decline as the halo mass increases. If the gas mass fraction, fg, in halos is universal, as has been suggested in the literature, the observed baryon mass in stars and gas shows a possible deficit compared with the total baryon density estimated from the baryon oscillation peaks in anisotropy of the cosmic microwave background.

Original languageEnglish (US)
Article number22
JournalAstrophysical Journal
Volume807
Issue number1
DOIs
StatePublished - Jul 1 2015

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • galaxies: clusters: general
  • gravitational lensing: weak
  • large-scale structure of universe

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