Kyle W. Willett
Galaxy Zoo: Morphological classifications for 120 000 galaxies in HST legacy imaging
Willett, Kyle W.; Galloway, Melanie A.; Bamford, Steven P.; Lintott, Chris J.; Masters, Karen L.; Scarlata, Claudia; Simmons, B. D.; Beck, Melanie; Cardamone, Carolin N.; Cheung, Edmond; Edmondson, Edward M.; Fortson, Lucy F.; Griffith, Roger L.; H�u�ler, Boris; Han, Anna; Hart, Ross; Melvin, Thomas; Parrish, Michael; Schawinski, Kevin; Smethurst, Rebecca J.; Smith, Arfon M.
Authors
Melanie A. Galloway
Dr STEVEN BAMFORD STEVEN.BAMFORD@NOTTINGHAM.AC.UK
ASSOCIATE PROFESSOR
Chris J. Lintott
Karen L. Masters
Claudia Scarlata
B. D. Simmons
Melanie Beck
Carolin N. Cardamone
Edmond Cheung
Edward M. Edmondson
Lucy F. Fortson
Roger L. Griffith
Boris H�u�ler
Anna Han
Ross Hart
Thomas Melvin
Michael Parrish
Kevin Schawinski
Rebecca J. Smethurst
Arfon M. Smith
Abstract
© 2016 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. We present the data release paper for the Galaxy Zoo: Hubble (GZH) project. This is the third phase in a large effort to measure reliable, detailed morphologies of galaxies by using crowdsourced visual classifications of colour-composite images. Images in GZH were selected from various publicly released Hubble Space Telescope legacy programmes conducted with the Advanced Camera for Surveys, with filters that probe the rest-frame optical emission from galaxies out to z ~ 1. The bulk of the sample is selected to have mI814W < 23.5, but goes as faint as mI814W < 26.8 for deep images combined over five epochs. The median redshift of the combined samples is 〈 z 〉 = 0.9 ± 0.6, with a tail extending out to z ≃ 4. The GZH morphological data include measurements of both bulge- and disc-dominated galaxies, details on spiral disc structure that relate to the Hubble type, bar identification, and numerous measurements of clump identification and geometry. This paper also describes a new method for calibrating morphologies for galaxies of different luminosities and at different redshifts by using artificially redshifted galaxy images as a baseline. The GZH catalogue contains both raw and calibrated morphological vote fractions for 119 849 galaxies, providing the largest data set to date suitable for large-scale studies of galaxy evolution out to z ~ 1.
Citation
Willett, K. W., Galloway, M. A., Bamford, S. P., Lintott, C. J., Masters, K. L., Scarlata, C., Simmons, B. D., Beck, M., Cardamone, C. N., Cheung, E., Edmondson, E. M., Fortson, L. F., Griffith, R. L., Häußler, B., Han, A., Hart, R., Melvin, T., Parrish, M., Schawinski, K., Smethurst, R. J., & Smith, A. M. (2017). Galaxy Zoo: Morphological classifications for 120 000 galaxies in HST legacy imaging. Monthly Notices of the Royal Astronomical Society, 464(4), 4176-4203. https://doi.org/10.1093/mnras/stw2568
Journal Article Type | Article |
---|---|
Acceptance Date | Oct 5, 2016 |
Online Publication Date | Oct 8, 2016 |
Publication Date | Feb 1, 2017 |
Deposit Date | Jan 6, 2017 |
Publicly Available Date | Jan 6, 2017 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Oxford University Press |
Peer Reviewed | Peer Reviewed |
Volume | 464 |
Issue | 4 |
Pages | 4176-4203 |
DOI | https://doi.org/10.1093/mnras/stw2568 |
Keywords | methods: data analysis ; catalogues ; galaxies: evolution ; galaxies: highredshift ; galaxies: structure |
Public URL | https://nottingham-repository.worktribe.com/output/837776 |
Publisher URL | http://mnras.oxfordjournals.org/content/464/4/4176 |
Contract Date | Jan 6, 2017 |
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