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Subaru Deep Survey I. Near-Infrared Observations

2001; Oxford University Press; Volume: 53; Issue: 1 Linguagem: Inglês

10.1093/pasj/53.1.25

2053-051X

Toshinori Maihara, Fumihide Iwamuro, Hirohisa Tanabe, Tomoyuki Taguchi, Ryuji Hata, Shin Oya, Nobunari Kashikawa, Masanori Iye, Satoshi Miyazaki, Hiroshi Karoji, M. Yoshida, Tomonori Totani, Yuzuru Yoshii, Sadanori Okamura, Kazuhiro Shimasaku, Yoshihiko Saito, Hiroyasu Ando, Miwa Goto, Masahiko Hayashi, Norio Kaifu, Naoto Kobayashi, George Kosugi, Kentaro Motohara, Tetsuo Nishimura, Junichi Noumaru, Ryusuke Ogasawara, Toshiyuki Sasaki, K. Sekiguchi, Tadafumi Takata, Hiroshi Terada, Takuya Yamashita, Tomonori Usuda, A. T. Tokunaga,

Astronomy and Astrophysical Research

Deep near-infrared images of a blank 2'x2' section of sky near the Galactic north pole taken by Subaru Telescope are presented. The total integration times of the J and K' bands are 12.1 hours and 9.7 hours, resulting in 5-sigma limiting magnitudes of 25.1 and 23.5 mag, respectively. The numbers of sources within these limiting magnitudes found with an automated detection procedure are 385 in the J band and 350 in K'. Based on photometric measurements of these sources, we present number count vs. magnitude relations, color vs. magnitude diagrams, size vs. color relationships, etc. The slope of the galaxy number count plotted against the AB magnitude scale is about 0.23 in the 22 to 26 AB magnitude range of both bands. The spatial number density of galaxies as well as the slopes in the faint-end region given by the Subaru Deep Field (SDF) survey is consistent with those given by HST-NICMOS surveys as expressed on the AB magnitude diagram. Several sources having very large J-K' color are found including a few K' objects without detection at J. In addition, a number of faint Galactic stars are also detected, most of which are assigned to M-subdwarfs, together with a few brown dwarf candidates.