DESI Early Data Release Milky Way Survey value-added catalogue

Author:

Koposov Sergey E123ORCID,Allende Prieto C4,Cooper A P5ORCID,Li T S6ORCID,Beraldo e Silva L78ORCID,Kim B1ORCID,Carrillo A9ORCID,Dey A10ORCID,Manser C J1112ORCID,Nikakhtar F13,Riley A H9,Rockosi C141516,Valluri M717,Aguilar J18,Ahlen S19,Bailey S18,Blum R10,Brooks D20,Claybaugh T18,Cole S9,de la Macorra A21,Dey B22,Forero-Romero J E2324ORCID,Gaztañaga E252627,Guy J18,Kremin A18,Le Guillou L28,Levi M E18,Manera M2930,Meisner A10ORCID,Miquel R3130,Moustakas J32,Nie J33,Palanque-Delabrouille N1834,Percival W J353637ORCID,Rezaie M38ORCID,Rossi G39,Sanchez E40,Schlafly E F41,Schubnell M1742,Tarlé G17,Weaver B A10,Zhou Z33

Affiliation:

1. Institute for Astronomy, University of Edinburgh, Royal Observatory , Blackford Hill, Edinburgh EH9 3HJ , UK

2. Institute of Astronomy, University of Cambridge , Madingley Road, Cambridge CB3 0HA , UK

3. Kavli Institute for Cosmology, University of Cambridge , Madingley Road, Cambridge CB3 0HA , UK

4. Instituto de Astrofísica de Canarias , C/ Vía Láctea, s/n, E-38205 La Laguna, Tenerife, Spain, Universidad de La Laguna, Dept. de Astrofísica, E-38206 La Laguna, Tenerife , Spain

5. Institute of Astronomy and Department of Physics, National Tsing Hua University , 101 Kuang-Fu Rd. Sec. 2, 30013 Hsinchu , Taiwan

6. Department of Astronomy & Astrophysics, University of Toronto , Toronto, ON M5S 3H4 , Canada

7. Department of Astronomy, University of Michigan , Ann Arbor, MI 48109 , USA

8. Steward Observatory, University of Arizona , 933 N, Cherry Ave, Tucson, AZ 85721 , USA

9. Institute for Computational Cosmology, Department of Physics, Durham University , South Road, Durham DH1 3LE , UK

10. NSF’s NOIRLab , 950 N. Cherry Ave., Tucson, AZ 85719 , USA

11. Astrophysics Group, Department of Physics, Imperial College London , Prince Consort Rd, London, SW7 2AZ , UK

12. Department of Physics, University of Warwick , Gibbet Hill Road, Coventry, CV4 7AL , UK

13. Physics Department, Yale University , P.O. Box 208120, New Haven, CT 06511 , USA

14. Department of Astronomy and Astrophysics, UCO/Lick Observatory, University of California , 1156 High Street, Santa Cruz, CA 95064 , USA

15. Department of Astronomy and Astrophysics, University of California , Santa Cruz, 1156 High Street, Santa Cruz, CA 95065 , USA

16. University of California Observatories , 1156 High Street, Sana Cruz, CA 95065 , USA

17. University of Michigan , Ann Arbor, MI 48109 , USA

18. Lawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720 , USA

19. Physics Dept., Boston University , 590 Commonwealth Avenue, Boston, MA 02215 , USA

20. Department of Physics & Astronomy, University College London , Gower Street, London, WC1E 6BT , UK

21. Instituto de Física, Universidad Nacional Autónoma de México , Cd. de México C.P. 04510 , México

22. Department of Physics & Astronomy and Pittsburgh Particle Physics, Astrophysics, and Cosmology Center (PITT PACC), University of Pittsburgh , 3941 O’Hara Street, Pittsburgh, PA 15260 , USA

23. Departamento de Física, Universidad de los Andes , Cra. 1 No. 18A-10, Edificio Ip, CP 111711, Bogotá , Colombia

24. Observatorio Astronómico, Universidad de los Andes , Cra. 1 No. 18A-10, Edificio H, CP 111711 Bogotá , Colombia

25. Institut d’Estudis Espacials de Catalunya (IEEC) , E-08034 Barcelona , Spain

26. Institute of Cosmology & Gravitation, University of Portsmouth, Dennis Sciama Building , Portsmouth, PO1 3FX , UK

27. Institute of Space Sciences , ICE-CSIC, Campus UAB, Carrer de Can Magrans s/n, E-08913 Bellaterra, Barcelona , Spain

28. Sorbonne Université, CNRS/IN2P3, Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE) , F-75005 Paris , France

29. Departament de Física, Serra Húnter, Universitat Autònoma de Barcelona , E-08193 Bellaterra (Barcelona) , Spain

30. Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology , Campus UAB, E-08193 Bellaterra Barcelona , Spain

31. Institució Catalana de Recerca i Estudis Avançats, Passeig de Lluís Companys , 23, E-08010 Barcelona , Spain

32. Department of Physics and Astronomy, Siena College , 515 Loudon Road, Loudonville, NY 12211 , USA

33. National Astronomical Observatories, Chinese Academy of Sciences , A20 Datun Rd., Chaoyang District, 100012 Beijing , PR China

34. IRFU, CEA, Université Paris-Saclay , F-91191 Gif-sur-Yvette , France

35. Department of Physics and Astronomy, University of Waterloo , 200 University Ave W, Waterloo, ON N2L 3G1 , Canada

36. Perimeter Institute for Theoretical Physics , 31 Caroline St. North, Waterloo, ON N2L 2Y5 , Canada

37. Waterloo Centre for Astrophysics, University of Waterloo , 200 University Ave W, Waterloo, ON N2L 3G1 , Canada

38. Department of Physics, Kansas State University , 116 Cardwell Hall, Manhattan, KS 66506 , USA

39. Department of Physics and Astronomy, Sejong University , 143-747 Seoul , Korea

40. CIEMAT , Avenida Complutense 40, E-28040 Madrid , Spain

41. Space Telescope Science Institute , 3700 San Martin Drive, Baltimore, MD 21218 , USA

42. Department of Physics, University of Michigan , Ann Arbor, MI 48109 , USA

Abstract

ABSTRACT We present the stellar value-added catalogue based on the Dark Energy Spectroscopic Instrument (DESI) Early Data Release. The catalogue contains radial velocity and stellar parameter measurements for $\simeq$ 400 000 unique stars observed during commissioning and survey validation by DESI. These observations were made under conditions similar to the Milky Way Survey (MWS) currently carried out by DESI but also include multiple specially targeted fields, such as those containing well-studied dwarf galaxies and stellar streams. The majority of observed stars have $16\lt r\lt 20$ with a median signal-to-noise ratio in the spectra of $\sim$ 20. In the paper, we describe the structure of the catalogue, give an overview of different target classes observed, as well as provide recipes for selecting clean stellar samples. We validate the catalogue using external high-resolution measurements and show that radial velocities, surface gravities, and iron abundances determined by DESI are accurate to 1 km s−1, 0.3 dex, and $\sim$ 0.15 dex respectively. We also demonstrate possible uses of the catalogue for chemo-dynamical studies of the Milky Way stellar halo and Draco dwarf spheroidal. The value-added catalogue described in this paper is the very first DESI MWS catalogue. The next DESI data release, expected in less than a year, will add the data from the first year of DESI survey operations and will contain approximately 4 million stars, along with significant processing improvements.

Funder

STFC

MICINN

National Science and Technology Council

Natural Sciences and Engineering Research Council of Canada

NASA

Publisher

Oxford University Press (OUP)

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