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

Abstract

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~{\sc 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~{\sc 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.

arXiv comment12 pages, 7 figures. Accepted for publication in PASJ(2000)

Cited by in corpus (11)

• The Luminosity Function and Star Formation Rate between Redshifts of 0.07 and 1.47 for Narrow-band Emitters in the Subaru Deep Field
• A search for clusters at high redshift - IV. Spectroscopy of H-alpha emitters in a proto-cluster at z=2.16
• The Halpha Luminosity Function and Star Formation Rate at z~0.24 Based on Subaru Deep Imaging Data
• Measurement of [OIII] Emission in Lyman Break Galaxies
• H alpha emitting galaxies and the star formation rate density at z~0.24
• Stellar populations in local star-forming galaxies. I.-Data and modelling procedure
• A contribution to the selection of emission-line galaxies using narrow-band filters in the optical airglow windows
• On the Optimization of Broad-Band Photometry for Galaxy Evolution Studies
• Star-Forming Galaxies at z=0.24 in the Subaru Deep Field and the Sloan Digital Sky Survey
• Clustering Properties of Low-Luminosity Star-Forming galaxies at z = 0.24 and 0.40 in the Subaru Deep Field
• Near-Infrared search for C IV absorption counterparts along the line-of-sights to pair quasars