Subaru deep survey I. Near-infrared observations

Citation
T. Maihara et al., Subaru deep survey I. Near-infrared observations, PUB AST S J, 53(1), 2001, pp. 25-36
Citations number
30
Categorie Soggetti
Space Sciences
Journal title
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN
ISSN journal
00046264 → ACNP
Volume
53
Issue
1
Year of publication
2001
Pages
25 - 36
Database
ISI
SICI code
0004-6264(2001)53:1<25:SDSINO>2.0.ZU;2-9
Abstract
Deep near-infrared images of a blank 2' x 2' section of sky near the galact ic north pole taken by Subaru Telescope are presented. The total integratio n times of the J and K' bands were 12.1 hr and 9.7 hr, resulting in 5 sigma limiting magnitudes of 25.1 and 23.5 mag, respectively. The numbers of sou rces within these limiting magnitudes found with an automated detection pro cedure are 385 in the J band and 350 in K'. Based on photometric measuremen ts of these sources, we present number count vs, magnitude relations, color vs. magnitude diagrams, size vs. color relationships, etc. The slope of th e 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 densit y of galaxies as well as the slopes in the faint-end region given by the Su baru Deep Field (SDF) survey are consistent with those given by HST-NICMOS surveys, as expressed on the AB magnitude diagram. Several sources having v ery large J - K' color have been found, including a few K' objects without detection at J. In addition, a number of faint galactic stars were also det ected, most of which are assigned to M-subdwarfs, together with a few brown dwarf candidates.