Near-infrared emission-line galaxies in the Hubble Deep Field North

被引：17

作者：

Iwamuro, F ^{[1
]}

Motohara, K

Maihara, T

Iwai, J

Tanabe, H

Taguchi, T

Hata, R

Terada, H

Goto, M

Oya, S

Iye, M

Yoshida, M

Karoji, H

Ogasawara, R

Sekiguchi, K

机构：

[1] Kyoto Univ, Dept Phys, Kyoto 6068502, Japan

[2] Commun Res Labs, Tokyo 1848975, Japan

[3] Natl Astron Observ, Opt & Infrared Astron Div, Tokyo 1818588, Japan

[4] Natl Astron Observ, Hilo, HI 96720 USA

来源：

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN | 2000年 / 52卷 / 01期

关键词：

cosmology : observations; galaxies : formation; infrared : galaxies;

D O I：

10.1093/pasj/52.1.73

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the 2.12 mu m narrow-band image of the Hubble Deep Field North taken with the near-infrared camera (CISCO) on the Subaru telescope. Among five targets whose H alpha or [O III] emission lines are redshifted into our narrow-band range expected from their spectroscopic redshift, four of them have strong emission lines, especially for the two [O III] emission-line objects. The remaining one target shows no H alpha emission in spite of its bright rest-UV luminosity, indicating that this object is already under the post-starburst phase. The volume-averaged SFR derived from the detected two H alpha emission is roughly consistent with that evaluated from the rest-UV continuum.

引用

页码：73 / 79

页数：7

共 26 条

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