Journal
ASTROPHYSICAL JOURNAL LETTERS
Volume 685, Issue 1, Pages L13-L17Publisher
IOP PUBLISHING LTD
DOI: 10.1086/592328
Keywords
cosmology: observations; galaxies: evolution; galaxies: spiral; radio lines: galaxies
Categories
Funding
- NASA/IPAC Extragalactic Database (NED)
- Jet Propulsion Laboratory, California Institute of Technology
- NSF [AST 03-07396, AST 03-07661]
- NAIC
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We present the first results of a targeted survey carried out with the 305 m Arecibo telescope to detect H I line emission from galaxies at redshift z > 0.16. The targets, selected from the Sloan Digital Sky Survey database, are noninteracting disk galaxies in relatively isolated fields. We present here the H I spectra and derived H I parameters for 10 objects detected in this pilot program. All are massive disk galaxies in the redshift interval 0.17-0.25 (i.e., 2-3 Gyr look-back time), with H I masses M-HI = (3-8) x 10(10) M-circle dot and high gas mass fractions (H I-to-stellar mass ratios similar to 10%-30%). Our results demonstrate the efficacy of exploiting Arecibo's large collecting area to measure the H I mass and rotational velocity of galaxies above redshift. In particular, z = 0.2 this sample includes the highest redshift detections of H I emission from individual galaxies made to date. Extension of this pilot program will allow us to study the H I properties of field galaxies at cosmological distances, thus complementing ongoing radio synthesis observations of cluster samples at z similar to 0.2.
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