The DESI One-Percent Survey: exploring a generalized SHAM for multiple tracers with the UNIT simulation

Author:

Yu Jiaxi1ORCID,Zhao Cheng12ORCID,Gonzalez-Perez Violeta34ORCID,Chuang Chia-Hsun5ORCID,Brodzeller Allyson5ORCID,de Mattia Arnaud6,Kneib Jean-Paul17,Krolewski Alex8910,Rocher Antoine6ORCID,Ross Ashley11ORCID,Wang Yunchong12ORCID,Yuan Sihan1314ORCID,Zhang Hanyu15ORCID,Zhou Rongpu16ORCID,Aguilar Jessica Nicole16,Ahlen Steven17ORCID,Brooks David18,Dawson Kyle5,de la Macorra Alex19ORCID,Doel Peter18,Fanning Kevin1120ORCID,Font-Ribera Andreu21ORCID,Forero-Romero Jaime22ORCID,Gontcho Satya Gontcho A16ORCID,Honscheid Klaus1120,Kehoe Robert23,Kisner Theodore16ORCID,Kremin Anthony16ORCID,Landriau Martin16ORCID,Manera Marc2124ORCID,Martini Paul1125ORCID,Meisner Aaron26ORCID,Miquel Ramon2127,Moustakas John28ORCID,Nie Jundan29ORCID,Percival Will8910ORCID,Poppett Claire163031,Raichoor Anand16ORCID,Rossi Graziano32,Seo Hee-Jong33ORCID,Tarlé Gregory34ORCID,Zhou Zhimin29ORCID,Zou Hu29ORCID

Affiliation:

1. Laboratory of Astrophysics, École Polytechnique Fédérale de Lausanne (EPFL), Observatoire de Sauverny , CH-1290 Versoix , Switzerland

2. Department of Astronomy, Tsinghua University , Beijing 100084 , China

3. Departamento de Física Teórica, Facultad de Ciencias, Universidad Autónoma de Madrid , E-28049 Madrid , Spain

4. Centro de Investigación Avanzada en Física Fundamental (CIAFF), Facultad de Ciencias, Universidad Autónoma de Madrid , E-28049 Madrid , Spain

5. Department of Physics and Astronomy, University of Utah, Salt Lake City , UT 84112 , USA

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

7. LAM (Laboratoire d’Astrophysique de Marseille), Aix Marseille Université, CNRS , UMR 7326, F13388, Marseille , France

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

9. Waterloo Centre for Astrophysics, University of Waterloo , Waterloo, ON N2L 3G1 , Canada

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

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

12. Physics Department, Stanford University , 382 Via Pueblo Mall, Stanford, CA 94305 , USA

13. Physics Department, Kavli Institute for Particle Astrophysics and Cosmology, Stanford University , Stanford, CA 94305 , USA

14. SLAC National Accelerator Laboratory , Menlo Park, CA 94025 , USA

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

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

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

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

19. Departamento de Física, Universidad de Guanajuato–DCI , C.P. 37150, Leon, Guanajuato , México

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

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

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

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

24. Serra Húnter Fellow, Departament de Física, Universitat Auònoma de Barcelona , 08193 Bellaterra (Barcelona) , Spain

25. Department of Astronomy, The Ohio State University , 140 W. 18th Ave., Columbus, OH 43210 , USA

26. NSF’s National Optical-Infrared Astronomy Research Laboratory , 950 N. Cherry Avenue, Tucson, AZ 85719 , USA

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

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

29. National Astronomical Observatories, Chinese Academy of Sciences , A20 Datun Road, Chaoyang District, Beijing, 100101 , People’s Republic of China

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

31. University of California , Berkeley, 110 Sproul Hall no. 5800 Berkeley, CA 94720 , USA

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

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

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

Abstract

ABSTRACT We perform SubHalo Abundance Matching (SHAM) studies on UNIT simulations with {σ, Vceil, vsmear}-SHAM and {σ, Vceil, fsat}-SHAM. They are designed to reproduce the clustering on 5–30 $\, {\, h^{-1}\, {\rm Mpc}}$ of luminous red galaxies (LRGs), emission-line galaxies (ELGs), and quasi-stellar objects (QSOs) at 0.4 < z < 3.5 from DESI (Dark Energy Spectroscopic Instrument) One Percent Survey. Vceil is the incompleteness of the massive host (sub)haloes and is the key to the generalized SHAM. vsmear models the clustering effect of redshift uncertainties, providing measurements consistent with those from repeat observations. A free satellite fraction fsat is necessary to reproduce the clustering of ELGs. We find ELGs present a more complex galaxy–halo mass relation than LRGs reflected in their weak constraints on σ. LRGs, QSOs, and ELGs show increasing Vceil values, corresponding to the massive galaxy incompleteness of LRGs, the quenched star formation of ELGs and the quenched black hole accretion of QSOs. For LRGs, a Gaussian vsmear presents a better profile for subsamples at redshift bins than a Lorentzian profile used for other tracers. The impact of the statistical redshift uncertainty on ELG clustering is negligible. The best-fitting satellite fraction for DESI ELGs is around 4 per cent, lower than previous estimations for ELGs. The mean halo mass log10(〈Mvir〉) in ${{\, h^{-1}\, \mbox{M}_\odot }}{}$ for LRGs, ELGs, and QSOs are 13.16 ± 0.01, 11.90 ± 0.06, and 12.66 ± 0.45, respectively. Our generalized SHAM algorithms facilitate the production of multitracer galaxy mocks for cosmological tests.

Funder

SNF

Comunidad de Madrid

MICINN

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 7 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

同舟云学术

1.学者识别学者识别

2.学术分析学术分析

3.人才评估人才评估

"同舟云学术"是以全球学者为主线,采集、加工和组织学术论文而形成的新型学术文献查询和分析系统,可以对全球学者进行文献检索和人才价值评估。用户可以通过关注某些学科领域的顶尖人物而持续追踪该领域的学科进展和研究前沿。经过近期的数据扩容,当前同舟云学术共收录了国内外主流学术期刊6万余种,收集的期刊论文及会议论文总量共计约1.5亿篇,并以每天添加12000余篇中外论文的速度递增。我们也可以为用户提供个性化、定制化的学者数据。欢迎来电咨询!咨询电话:010-8811{复制后删除}0370

www.globalauthorid.com

TOP

Copyright © 2019-2024 北京同舟云网络信息技术有限公司
京公网安备11010802033243号  京ICP备18003416号-3