First detection of the BAO signal from early DESI data

Author:

Moon Jeongin1,Valcin David2,Rashkovetskyi Michael3ORCID,Saulder Christoph4,Aguilar Jessica Nicole5,Ahlen Steven6,Alam Shadab7,Bailey Stephen5,Baltay Charles8,Blum Robert9,Brooks David10,Burtin Etienne11,Chaussidon Edmond11,Dawson Kyle12,de la Macorra Axel13,de M attia Arnaud11,Dhungana Govinda14,Eisenstein Daniel3,Flaugher Brenna15,Font-Ribera Andreu16,Forero-Romero Jaime E17,Garcia-Quintero Cristhian18,Gontcho A Gontcho Satya5,Guy Julien5,Hanif Malik Muhammad Sikandar19,Honscheid Klaus2021,Ishak Mustapha18,Kehoe Robert14,Kim Sumi22,Kisner Theodore5,Kremin Anthony5,Landriau Martin5,Le Guillou Laurent23,Levi Michael5,Manera Marc24,Martini Paul2521,McDonald Patrick5,Meisner Aaron9,Miquel Ramon1626,Moustakas John27,Myers Adam28,Nadathur Seshadri29,Neveux Richard30,Newman Jeffrey A31,Nie Jundan32,Padmanabhan Nikhil8ORCID,Palanque-Delabrouille Nathalie511,Percival Will3334,Pérez Fernández Alejandro13,Poppett Claire355,Prada Francisco36,Raichoor Anand5,Ross Ashley J2521,Rossi Graziano1,Samushia Lado37,Schlegel David5,Seo Hee-Jong2ORCID,Tarlé Gregory19,Vargas Magana Mariana13,Variu Andrei38,Weaver Benjamin Alan9,White Martin J39,Yèche Christophe11,Yuan Sihan40,Zhao Cheng38,Zhou Rongpu5,Zhou Zhimin32,Zou Hu32

Affiliation:

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

2. Department of Physics and Astronomy, Ohio University , Athens, OH 45701 , USA

3. Center for Astrophysics | Harvard and Smithsonian , 60 Garden Street, Cambridge, MA 02138 , USA

4. Korea Astronomy and Space Science Institute , 776 Daedeok-daero, Yuseong-gu, Daejeon 34055 , Republic of Korea

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

6. Physics Department, Boston University , 590 Commonwealth Avenue, Boston, MA 02215 , USA

7. Tata Institute of Fundamental Research , Homi Bhabha Road, Mumbai 400005 , India

8. Physics Department, Yale University , PO Box 208120, New Haven, CT 06511 , USA

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

10. Department of Physics and Astronomy, University College London , Gower Street, London WC1E 6BT , UK

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

12. Department of Physics and Astronomy, The University of Utah , 115 South 1400 East, Salt Lake City, UT 84112 , USA

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

14. Department of Physics, Southern Methodist University , 3215 Daniel Avenue, Dallas, TX 75275 , USA

15. Fermi National Accelerator Laboratory , PO Box 500, Batavia, IL 60510 , USA

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

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

18. Department of Physics, The University of Texas at Dallas , Richardson, TX 75080 , USA

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

20. Department of Physics, The Ohio State University , 191 West Woodruff Avenue, Columbus, OH 43210 , USA

21. Center for Cosmology and AstroParticle Physics, The Ohio State University , 191 West Woodruff Avenue, Columbus, OH 43210 , USA

22. Natural Science Research Institute, University of Seoul , 163 Seoulsiripdae-ro, Dongdaemun-gu, Seoul 02504 , South Korea

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

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

25. Department of Astronomy, The Ohio State University , 4055 McPherson Laboratory, 140 W 18th Avenue, Columbus, OH 43210 , USA

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

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

28. Department of Physics and Astronomy, University of Wyoming , 1000 E. University, Dept. 3905, Laramie, WY 82071 , USA

29. Institute of Cosmology and Gravitation, University of Portsmouth , Dennis Sciama Building, Portsmouth PO1 3FX , UK

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

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

32. National Astronomical Observatories, Chinese Academy of Sciences , A20 Datun Rd, Chaoyang District, Beijing 100012 , P.R. China

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

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

35. Space Sciences Laboratory, University of California , Berkeley, 7 Gauss Way, Berkeley, CA 94720 , USA

36. Instituto de Astrofísica de Andalucía (CSIC) , Glorieta de la Astronomía, s/n, E-18008 Granada , Spain

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

38. Ecole Polytechnique Fédérale de Lausanne , CH-1015 Lausanne , Switzerland

39. Department of Physics, University of California , Berkeley, 366 LeConte Hall MC 7300, Berkeley, CA 94720-7300 , USA

40. SLAC National Accelerator Laboratory , Menlo Park, CA 94305 , USA

Abstract

ABSTRACT We present the first detection of the baryon acoustic oscillations (BAOs) signal obtained using unblinded data collected during the initial 2 months of operations of the Stage-IV ground-based Dark Energy Spectroscopic Instrument (DESI). From a selected sample of 261 291 luminous red galaxies spanning the redshift interval 0.4 < z < 1.1 and covering 1651 square degrees with a 57.9  per cent completeness level, we report a ∼5σ level BAO detection and the measurement of the BAO location at a precision of 1.7  per cent. Using a bright galaxy sample of 109 523 galaxies in the redshift range 0.1 < z < 0.5, over 3677 square degrees with a 50.0  per cent completeness, we also detect the BAO feature at ∼3σ significance with a 2.6  per cent precision. These first BAO measurements represent an important milestone, acting as a quality control on the optimal performance of the complex robotically actuated, fibre-fed DESI spectrograph, as well as an early validation of the DESI spectroscopic pipeline and data management system. Based on these first promising results, we forecast that DESI is on target to achieve a high-significance BAO detection at sub-per cent precision with the completed 5-yr survey data, meeting the top-level science requirements on BAO measurements. This exquisite level of precision will set new standards in cosmology and confirm DESI as the most competitive BAO experiment for the remainder of this decade.

Funder

Korean Ministry of Education, Science and Technology

U.S. Department of Energy

Simons Foundation

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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