THE CATALOG OF EDGE-ON DISK GALAXIES FROM SDSS. I. THE CATALOG AND THE STRUCTURAL PARAMETERS OF STELLAR DISKS

被引:66
作者
Bizyaev, D. V. [1 ,2 ,3 ]
Kautsch, S. J. [4 ]
Mosenkov, A. V. [5 ,6 ]
Reshetnikov, V. P. [6 ,7 ]
Sotnikova, N. Ya. [6 ,7 ]
Yablokova, N. V. [6 ]
Hillyer, R. W. [8 ]
机构
[1] Apache Point Observ, Sunspot, NM 88349 USA
[2] New Mexico State Univ, Sunspot, NM 88349 USA
[3] Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow, Russia
[4] Nova SE Univ, Ft Lauderdale, FL 33314 USA
[5] RAS, Cent Astron Observ, Moscow, Russia
[6] St Petersburg State Univ, St Petersburg 199034, Russia
[7] Isaac Newton Inst Chile, St Petersburg Branch, St Petersburg, Russia
[8] Christopher Newport Univ, Newport News, VA 23606 USA
基金
美国安德鲁·梅隆基金会; 美国国家科学基金会;
关键词
galaxies: fundamental parameters; galaxies: general; galaxies: photometry; galaxies: spiral; galaxies: structure; DIGITAL SKY SURVEY; SPIRAL GALAXIES; SURFACE PHOTOMETRY; DATA RELEASE; RADIATIVE-TRANSFER; DUST DISTRIBUTION; THICK DISKS; COLOR; HALOES; LIGHT;
D O I
10.1088/0004-637X/787/1/24
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a catalog of true edge-on disk galaxies automatically selected from the Seventh Data Release of the Sloan Digital Sky Survey (SDSS). A visual inspection of the g, r, and i images of about 15,000 galaxies allowed us to split the initial sample of edge-on galaxy candidates into 4768 (31.8% of the initial sample) genuine edge-on galaxies, 8350 (55.7%) non-edge-on galaxies, and 1865 (12.5%) edge-on galaxies not suitable for simple automatic analysis because these objects either show signs of interaction and warps, or nearby bright stars project on it. We added more candidate galaxies from RFGC, EFIGI, RC3, and Galaxy Zoo catalogs found in the SDSS footprints. Our final sample consists of 5747 genuine edge-on galaxies. We estimate the structural parameters of the stellar disks (the stellar disk thickness, radial scale length, and central surface brightness) in the galaxies by analyzing photometric profiles in each of the g, r, and i images. We also perform simplified three-dimensional modeling of the light distribution in the stellar disks of edge-on galaxies from our sample. Our large sample is intended to be used for studying scaling relations in the stellar disks and bulges and for estimating parameters of the thick disks in different types of galaxies via the image stacking. In this paper, we present the sample selection procedure and general description of the sample.
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