Galaxy Zoo: the fraction of merging galaxies in the SDSS and their morphologies

被引:165
作者
Darg, D. W. [1 ]
Kaviraj, S. [1 ,2 ]
Lintott, C. J. [1 ]
Schawinski, K. [3 ,4 ]
Sarzi, M. [5 ]
Bamford, S. [6 ]
Silk, J. [1 ]
Proctor, R. [7 ]
Andreescu, D. [8 ]
Murray, P. [9 ]
Nichol, R. C. [10 ]
Raddick, M. J. [11 ]
Slosar, A. [12 ,13 ]
Szalay, A. S. [11 ]
Thomas, D. [10 ]
Vandenberg, J. [11 ]
机构
[1] Univ Oxford, Dept Phys, Oxford OX1 3RH, England
[2] Univ Coll London, Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England
[3] Yale Univ, Dept Phys, New Haven, CT 06511 USA
[4] Yale Univ, Yale Ctr Astron & Astrophys, New Haven, CT 06520 USA
[5] Univ Hertfordshire, Ctr Astrophys Res, Hatfield AL10 9AB, Herts, England
[6] Univ Nottingham, Ctr Astron & Particle Theory, Nottingham NG7 2RD, England
[7] Waveney Consulting, Waveney Web Serv, Wimborne BH21 3QY, Dorset, England
[8] LinkLab, Bronx, NY 10471 USA
[9] Fingerprint Digital Media, Newtownards BT23 7GY, Co Down, North Ireland
[10] Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 2EG, Hants, England
[11] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA
[12] Univ Calif Berkeley, Lawrence Berkeley Lab, Berkeley Ctr Cosmol Phys, Berkeley, CA 94720 USA
[13] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA
关键词
catalogues; galaxies: elliptical and lenticular; cD; galaxies: evolution; galaxies: general; galaxies: interactions; galaxies: spiral; DIGITAL-SKY-SURVEY; STAR-FORMATION RATES; EARLY DATA RELEASE; MERGER RATE; LUMINOSITY FUNCTION; SPIRAL GALAXIES; CLASSIFIED GALAXIES; MASSIVE GALAXIES; REDSHIFT SURVEY; FIELD GALAXIES;
D O I
10.1111/j.1365-2966.2009.15686.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the largest, most homogeneous catalogue of merging galaxies in the nearby Universe obtained through the Galaxy Zoo project - an interface on the World Wide Web enabling large-scale morphological classification of galaxies through visual inspection of images from the Sloan Digital Sky Survey (SDSS). The method converts a set of visually inspected classifications for each galaxy into a single parameter (the 'weighted-merger-vote fraction,' f(m)) which describes our confidence that the system is part of an ongoing merger. We describe how f(m) is used to create a catalogue of 3003 visually selected pairs of merging galaxies from the SDSS in the redshift range 0.005 < z < 0.1. We use our merger sample and values of f(m) applied to the SDSS Main Galaxy Spectral sample to estimate that the fraction of volume-limited (M(r) < -20.55) major mergers (1/3 < M*(1)/M*(2) < 3) in the nearby Universe is 1-3 x C per cent, where C similar to 1.5 is a correction factor for spectroscopic incompleteness. Having visually classified the morphologies of the constituent galaxies in our mergers, we find that the spiral-to-elliptical ratio of galaxies in mergers is higher by a factor of similar to 2 relative to the global population. In a companion paper, we examine the internal properties of these merging galaxies and conclude that this high spiral-to-elliptical ratio in mergers is due to a longer time-scale over which mergers with spirals are detectable compared to mergers with ellipticals.
引用
收藏
页码:1043 / 1056
页数:14
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