HI-SELECTED GALAXIES IN THE SLOAN DIGITAL SKY SURVEY. I. OPTICAL DATA

被引：35

作者：

West, Andrew A. ^{[1
,2
,3
,4
]}

Garcia-Appadoo, Diego A. ^{[5
,6
]}

Dalcanton, Julianne J. ^{[2
]}

Disney, Mike J. ^{[6
]}

Rockosi, Constance M. ^{[7
]}

Ivezic, Zeljko ^{[2
]}

Bentz, Misty C. ^{[2
,8
]}

Brinkmann, J. ^{[9
]}

机构：

[1] Univ Washington, Dept Astron, Seattle, WA 98195 USA

[2] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA

[3] MIT, Kavli Inst Astrophys & Space Res, Cambridge, MA 02139 USA

[4] Boston Univ, Dept Astron, Boston, MA 02215 USA

[5] European So Observ, Santiago 19, Chile

[6] Cardiff Univ, Cardiff Sch Phys & Astron, Cardiff CF24 3AA, S Glam, Wales

[7] Univ Calif Santa Cruz, Dept Astron & Astrophys, UCO, Lick Observ, Santa Cruz, CA 95064 USA

[8] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA

[9] Apache Point Observ, Sunspot, NM 88349 USA

来源：

ASTRONOMICAL JOURNAL | 2010年 / 139卷 / 02期

关键词：

galaxies: evolution; galaxies: fundamental parameters; galaxies: general; galaxies: photometry; radio lines: galaxies; surveys; CENTIMETER-SELECTED SAMPLE; TULLY-FISHER RELATION; DUAL-BEAM SURVEY; STAR-FORMATION; DATA RELEASE; LOCAL UNIVERSE; HIPASS CATALOG; SPIRAL GALAXIES; DWARF GALAXIES; INFRARED PROPERTIES;

D O I：

10.1088/0004-6256/139/2/315

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the optical data for 195 HI-selected galaxies that fall within both the Sloan Digital Sky Survey (SDSS) and the Parkes Equatorial Survey (ES). The photometric quantities have been independently recomputed for our sample using a new photometric pipeline optimized for large galaxies, thus correcting for SDSS's limited reliability for automatic photometry of angularly large or low surface brightness (LSB) galaxies. We outline the magnitude of the uncertainty in the SDSS catalog-level photometry and derive a quantitative method for correcting the over-sky subtraction in the SDSS photometric pipeline. The main thrust of this paper is to present the ES/SDSS sample and discuss the methods behind the improved photometry, which will be used in future scientific analysis. We present the overall optical properties of the sample and briefly compare to a volume-limited, optically selected sample. Compared to the optically selected SDSS sample (in the similar volume), HI-selected galaxies are bluer and more luminous (fewer dwarf ellipticals and more star formation). However, compared to typical SDSS galaxy studies, which have their own selection effect, our sample is bluer, fainter, and less massive.

引用

页码：315 / 328

页数：14

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