Galaxy Zoo DESI: Detailed morphology measurements for 8.7M galaxies in the DESI Legacy Imaging Surveys

Author:

Walmsley Mike1ORCID,Géron Tobias2ORCID,Kruk Sandor3ORCID,Scaife Anna M M14ORCID,Lintott Chris2ORCID,Masters Karen L5ORCID,Dawson James M6,Dickinson Hugh7ORCID,Fortson Lucy89,Garland Izzy L10ORCID,Mantha Kameswara89,O’Ryan David10,Popp Jürgen7,Simmons Brooke10ORCID,Baeten Elisabeth M11,Macmillan Christine11

Affiliation:

1. Department of Physics & Astronomy, Jodrell Bank Centre for Astrophysics, University of Manchester , Oxford Road, Manchester M13 9PL , UK

2. Oxford Astrophysics, Department of Physics, University of Oxford , Denys Wilkinson Building, Keble Road, Oxford, OX1 3RH , UK

3. European Space Agency (ESA), European Space Astronomy Centre (ESAC) , Camino Bajo del Castillo s/n E-28692 Villanueva de la Cañada, Madrid , Spain

4. The Alan Turing Institute , 96 Euston Road, London NW1 2DB , UK

5. Department of Physics and Astronomy, Haverford College , 370 Lancaster Avenue, Haverford, Pennsylvania 19041 , USA

6. South African Radio Astronomy Observatory (SARAO) , Black River Park North, 2 Fir St, Cape Town 7925 , South Africa

7. School of Physical Sciences, The Open University , Milton Keynes, MK7 6AA , UK

8. School of Physics and Astronomy, University of Minnesota , Minneapolis, Minnesota 55455 , USA

9. Minnesota Institute for Astrophysics, University of Minnesota , Minneapolis, Minnesota 55455 , USA

10. Department of Physics, Lancaster University , Lancaster LA1 4YB , UK

11. Citizen Scientist, Zooniverse c/o University of Oxford , Keble Road, Oxford OX1 3RH , UK

Abstract

ABSTRACT We present detailed morphology measurements for 8.67 million galaxies in the DESI Legacy Imaging Surveys (DECaLS, MzLS, and BASS, plus DES). These are automated measurements made by deep learning models trained on Galaxy Zoo volunteer votes. Our models typically predict the fraction of volunteers selecting each answer to within 5–10 per cent for every answer to every GZ question. The models are trained on newly collected votes for DESI-LS DR8 images as well as historical votes from GZ DECaLS. We also release the newly collected votes. Extending our morphology measurements outside of the previously released DECaLS/SDSS intersection increases our sky coverage by a factor of 4 (5000–19 000 deg2) and allows for full overlap with complementary surveys including ALFALFA and MaNGA.

Funder

Science and Technology Facilities Council

National Science Foundation

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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