Shin OYA

Deep near-infrared images of a blank 2 ′ × 2 ′ section of sky near the galactic north pole taken by Subaru Telescope are presented. The total integration times of the J and K ′ bands were 12.1 hr and 9.7 hr, resulting in 5 σ limiting magnitudes of 25.1 and 23.5 mag, respectively. The numbers of sour...

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Bibliographic Details
Main Authors: Toshinori Maihara, Fumihide Iwamuro, Hirohisa Tanabe, Tomoyuki Taguchi, Ryuji Hata, Nobunari Kashikawa, Masanori Iye, Satoshi Miyazaki, Hiroshi Karoji, Michitoshi Yoshida, Tomonori Totani, Yuzuru Yoshii, Sadanori Okamura, Kazuhiro Shimasaku, Yoshihiko Saito, Kentaro Motohara, Tetsuo Nishimura, Ryusuke Ogasawara, Toshiyuki Sasaki, Kazuhiro Sekiguchi, Tadafumi Takata, Hiroshi Terada, Alan T. Tokunaga
Other Authors: The Pennsylvania State University CiteSeerX Archives
Format: Text
Language:English
Published: 2000
Subjects:
North Pole
Online Access:http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.1032.5083
http://pasj.oxfordjournals.org/content/53/1/25.full.pdf
Description
Summary:Deep near-infrared images of a blank 2 ′ × 2 ′ section of sky near the galactic north pole taken by Subaru Telescope are presented. The total integration times of the J and K ′ bands were 12.1 hr and 9.7 hr, resulting in 5 σ 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 are consistent with those given by HST–NICMOS

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