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Galaxy Zoo: morphological classifications for 120 000 galaxies in HST legacy imaging

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Galaxy Zoo: morphological classifications for 120 000 galaxies in HST legacy imaging. / Willett, Kyle W.; Galloway, Melanie A.; Bamford, Steven P. et al.
In: Monthly Notices of the Royal Astronomical Society, Vol. 464, No. 4, 01.02.2017, p. 4176-4203.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Willett, KW, Galloway, MA, Bamford, SP, Lintott, CJ, Masters, KL, Scarlata, C, Simmons, BD, Beck, M, Cardamone, CN, Cheung, E, Edmondson, EM, Fortson, LF, Griffith, RL, Häußler, B, Han, A, Hart, R, Melvin, T, Parrish, M, Schawinski, K, Smethurst, RJ & Smith, AM 2017, 'Galaxy Zoo: morphological classifications for 120 000 galaxies in HST legacy imaging', Monthly Notices of the Royal Astronomical Society, vol. 464, no. 4, pp. 4176-4203. https://doi.org/10.1093/mnras/stw2568

APA

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., ... 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

Vancouver

Willett KW, Galloway MA, Bamford SP, Lintott CJ, Masters KL, Scarlata C et al. Galaxy Zoo: morphological classifications for 120 000 galaxies in HST legacy imaging. Monthly Notices of the Royal Astronomical Society. 2017 Feb 1;464(4):4176-4203. doi: 10.1093/mnras/stw2568

Author

Willett, Kyle W. ; Galloway, Melanie A. ; Bamford, Steven P. et al. / Galaxy Zoo : morphological classifications for 120 000 galaxies in HST legacy imaging. In: Monthly Notices of the Royal Astronomical Society. 2017 ; Vol. 464, No. 4. pp. 4176-4203.

Bibtex

@article{844f018ba60349d58569b8a7c452787b,
title = "Galaxy Zoo: morphological classifications for 120 000 galaxies in HST legacy imaging",
abstract = "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.",
author = "Willett, {Kyle W.} and Galloway, {Melanie A.} and Bamford, {Steven P.} and Lintott, {Chris J.} and Masters, {Karen L.} and Claudia Scarlata and Simmons, {B. D.} and Melanie Beck and Cardamone, {Carolin N.} and Edmond Cheung and Edmondson, {Edward M.} and Fortson, {Lucy F.} and Griffith, {Roger L.} and Boris H{\"a}u{\ss}ler and Anna Han and Ross Hart and Thomas Melvin and Michael Parrish and Kevin Schawinski and Smethurst, {R. J.} and Smith, {Arfon M.}",
year = "2017",
month = feb,
day = "1",
doi = "10.1093/mnras/stw2568",
language = "English",
volume = "464",
pages = "4176--4203",
journal = "Monthly Notices of the Royal Astronomical Society",
issn = "0035-8711",
publisher = "OXFORD UNIV PRESS",
number = "4",

}

RIS

TY - JOUR

T1 - Galaxy Zoo

T2 - morphological classifications for 120 000 galaxies in HST legacy imaging

AU - Willett, Kyle W.

AU - Galloway, Melanie A.

AU - Bamford, Steven P.

AU - Lintott, Chris J.

AU - Masters, Karen L.

AU - Scarlata, Claudia

AU - Simmons, B. D.

AU - Beck, Melanie

AU - Cardamone, Carolin N.

AU - Cheung, Edmond

AU - Edmondson, Edward M.

AU - Fortson, Lucy F.

AU - Griffith, Roger L.

AU - Häußler, Boris

AU - Han, Anna

AU - Hart, Ross

AU - Melvin, Thomas

AU - Parrish, Michael

AU - Schawinski, Kevin

AU - Smethurst, R. J.

AU - Smith, Arfon M.

PY - 2017/2/1

Y1 - 2017/2/1

N2 - 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.

AB - 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.

U2 - 10.1093/mnras/stw2568

DO - 10.1093/mnras/stw2568

M3 - Journal article

VL - 464

SP - 4176

EP - 4203

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 4

ER -