The Astrophysical Journal (Jan 2024)
Measuring the Conditional Luminosity and Stellar Mass Functions of Galaxies by Combining the Dark Energy Spectroscopic Instrument Legacy Imaging Surveys Data Release 9, Survey Validation 3, and Year 1 Data
- Yirong Wang,
- Xiaohu Yang,
- Yizhou Gu,
- Xiaoju Xu,
- Haojie Xu,
- Yuyu Wang,
- Antonios Katsianis,
- Jiaxin Han,
- Min He,
- Yunliang Zheng,
- Qingyang Li,
- Yaru Wang,
- Wensheng Hong,
- Jiaqi Wang,
- Zhenlin Tan,
- Hu Zou,
- Johannes Ulf Lange,
- ChangHoon Hahn,
- Peter Behroozi,
- Jessica Nicole Aguilar,
- Steven Ahlen,
- David Brooks,
- Todd Claybaugh,
- Shaun Cole,
- Axel de la Macorra,
- Biprateep Dey,
- Peter Doel,
- Jaime E. Forero-Romero,
- Klaus Honscheid,
- Robert Kehoe,
- Theodore Kisner,
- Andrew Lambert,
- Marc Manera,
- Aaron Meisner,
- Ramon Miquel,
- John Moustakas,
- Jundan Nie,
- Claire Poppett,
- Mehdi Rezaie,
- Graziano Rossi,
- Eusebio Sanchez,
- Michael Schubnell,
- Gregory Tarlé,
- Benjamin Alan Weaver,
- Zhimin Zhou
Affiliations
- Yirong Wang
- ORCiD
- Department of Astronomy, School of Physics and Astronomy, and Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai Jiao Tong University , Shanghai 200240, People's Republic of China ; [email protected], [email protected]
- Xiaohu Yang
- ORCiD
- Department of Astronomy, School of Physics and Astronomy, and Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai Jiao Tong University , Shanghai 200240, People's Republic of China ; [email protected], [email protected]; Tsung-Dao Lee Institute, and Key Laboratory for Particle Physics, Astrophysics and Cosmology, Ministry of Education, Shanghai Jiao Tong University , Shanghai 200240, People's Republic of China
- Yizhou Gu
- ORCiD
- Department of Astronomy, School of Physics and Astronomy, and Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai Jiao Tong University , Shanghai 200240, People's Republic of China ; [email protected], [email protected]
- Xiaoju Xu
- Department of Astronomy, School of Physics and Astronomy, and Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai Jiao Tong University , Shanghai 200240, People's Republic of China ; [email protected], [email protected]
- Haojie Xu
- ORCiD
- Department of Astronomy, School of Physics and Astronomy, and Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai Jiao Tong University , Shanghai 200240, People's Republic of China ; [email protected], [email protected]; Shanghai Astronomical Observatory, Chinese Academy of Sciences , Nandan Road 80, Shanghai 200240, People's Republic of China
- Yuyu Wang
- ORCiD
- Department of Astronomy, School of Physics and Astronomy, and Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai Jiao Tong University , Shanghai 200240, People's Republic of China ; [email protected], [email protected]
- Antonios Katsianis
- Department of Astronomy, School of Physics and Astronomy, and Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai Jiao Tong University , Shanghai 200240, People's Republic of China ; [email protected], [email protected]; School of Physics and Astronomy, Sun Yat-sen University , Zhuhai Campus, 2 Daxue Road, Xiangzhou District, Zhuhai, People’s Republic of China
- Jiaxin Han
- ORCiD
- Department of Astronomy, School of Physics and Astronomy, and Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai Jiao Tong University , Shanghai 200240, People's Republic of China ; [email protected], [email protected]
- Min He
- ORCiD
- Department of Astronomy, School of Physics and Astronomy, and Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai Jiao Tong University , Shanghai 200240, People's Republic of China ; [email protected], [email protected]
- Yunliang Zheng
- ORCiD
- Department of Astronomy, School of Physics and Astronomy, and Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai Jiao Tong University , Shanghai 200240, People's Republic of China ; [email protected], [email protected]
- Qingyang Li
- Department of Astronomy, School of Physics and Astronomy, and Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai Jiao Tong University , Shanghai 200240, People's Republic of China ; [email protected], [email protected]
- Yaru Wang
- Department of Astronomy, School of Physics and Astronomy, and Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai Jiao Tong University , Shanghai 200240, People's Republic of China ; [email protected], [email protected]
- Wensheng Hong
- Department of Astronomy, School of Physics and Astronomy, and Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai Jiao Tong University , Shanghai 200240, People's Republic of China ; [email protected], [email protected]
- Jiaqi Wang
- Department of Astronomy, School of Physics and Astronomy, and Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai Jiao Tong University , Shanghai 200240, People's Republic of China ; [email protected], [email protected]
- Zhenlin Tan
- Department of Astronomy, School of Physics and Astronomy, and Shanghai Key Laboratory for Particle Physics and Cosmology, Shanghai Jiao Tong University , Shanghai 200240, People's Republic of China ; [email protected], [email protected]
- Hu Zou
- ORCiD
- National Astronomical Observatories, Chinese Academy of Sciences , A20 Datun Road, Chaoyang District, Beijing, 100012, People's Republic of China
- Johannes Ulf Lange
- Kavli Institute for Particle Astrophysics and Cosmology and Department of Physics, Stanford University , CA 94305, USA; Department of Astronomy and Astrophysics, University of California , Santa Cruz, CA 95064, USA; Department of Physics, University of Michigan , Ann Arbor, MI 48109, USA; Leinweber Center for Theoretical Physics, University of Michigan , Ann Arbor, MI 48109, USA
- ChangHoon Hahn
- ORCiD
- Department of Astrophysical Sciences, Princeton University , Peyton Hall, Princeton, NJ 08544, USA; Lawrence Berkeley National Laboratory , One Cyclotron Road, Berkeley, CA 94720, USA
- Peter Behroozi
- Department of Astronomy and Steward Observatory, University of Arizona , Tucson, AZ 85721, USA
- Jessica Nicole Aguilar
- Lawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USA
- Steven Ahlen
- ORCiD
- Physics Department, Boston University , 590 Commonwealth Avenue, Boston, MA 02215, USA
- David Brooks
- ORCiD
- Department of Physics & Astronomy, University College London , Gower Street, London, WC1E 6BT, UK
- Todd Claybaugh
- Lawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USA
- Shaun Cole
- ORCiD
- Institute for Computational Cosmology, Department of Physics, Durham University , South Road, Durham DH1 3LE, UK
- Axel de la Macorra
- ORCiD
- Instituto de Física, Universidad Nacional Autónoma de México , Cd. de México C.P. 04510, Mexico
- Biprateep Dey
- ORCiD
- 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
- Peter Doel
- Department of Physics & Astronomy, University College London , Gower Street, London, WC1E 6BT, UK
- Jaime E. Forero-Romero
- ORCiD
- Departamento de Física, Universidad de los Andes , Cra. 1 No. 18A-10, Edificio Ip, CP 111711, Bogotá, Colombia; Observatorio Astronómico, Universidad de los Andes , Cra. 1 No. 18A-10, Edificio H, CP 111711 Bogotá, Colombia
- Klaus Honscheid
- Department of Physics, The Ohio State University , 191 West Woodruff Avenue, Columbus, OH 43210, USA; Center for Cosmology and AstroParticle Physics, The Ohio State University , 191 West Woodruff Avenue, Columbus, OH 43210, USA
- Robert Kehoe
- Department of Physics, Southern Methodist University , 3215 Daniel Avenue, Dallas, TX 75275, USA
- Theodore Kisner
- ORCiD
- Lawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USA
- Andrew Lambert
- Lawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USA
- Marc Manera
- ORCiD
- Institut de Física d’Altes Energies (IFAE) , The Barcelona Institute of Science and Technology, Campus UAB, 08193 Bellaterra Barcelona, Spain; Departament de Física, Serra Húnter, Universitat Autònoma de Barcelona , 08193 Bellaterra (Barcelona), Spain
- Aaron Meisner
- ORCiD
- NSF’s NOIRLab , 950 North Cherry Avenue, Tucson, AZ 85719, USA
- Ramon Miquel
- ORCiD
- Institut de Física d’Altes Energies (IFAE) , The Barcelona Institute of Science and Technology, Campus UAB, 08193 Bellaterra Barcelona, Spain; Institució Catalana de Recerca i Estudis Avançats , Passeig de Lluís Companys, 23, 08010 Barcelona, Spain
- John Moustakas
- ORCiD
- Department of Physics and Astronomy, Siena College , 515 Loudon Road, Loudonville, NY 12211, USA
- Jundan Nie
- ORCiD
- National Astronomical Observatories, Chinese Academy of Sciences , A20 Datun Road, Chaoyang District, Beijing, 100012, People's Republic of China
- Claire Poppett
- ORCiD
- Lawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USA; Space Sciences Laboratory, University of California , Berkeley, 7 Gauss Way, Berkeley, CA 94720, USA
- Mehdi Rezaie
- ORCiD
- Department of Physics, Kansas State University , 116 Cardwell Hall, Manhattan, KS 66506, USA
- Graziano Rossi
- Department of Physics and Astronomy, Sejong University , Seoul, 143-747, Republic of Korea
- Eusebio Sanchez
- ORCiD
- CIEMAT , Avenida Complutense 40, E-28040 Madrid, Spain
- Michael Schubnell
- Department of Physics, University of Michigan , Ann Arbor, MI 48109, USA
- Gregory Tarlé
- ORCiD
- University of Michigan , Ann Arbor, MI 48109, USA
- Benjamin Alan Weaver
- NSF’s NOIRLab , 950 North Cherry Avenue, Tucson, AZ 85719, USA
- Zhimin Zhou
- ORCiD
- National Astronomical Observatories, Chinese Academy of Sciences , A20 Datun Road, Chaoyang District, Beijing, 100012, People's Republic of China
- DOI
- https://doi.org/10.3847/1538-4357/ad5294
- Journal volume & issue
-
Vol. 971,
no. 1
p. 119
Abstract
In this investigation, we leverage the combination of the Dark Energy Spectroscopic Instrument (DESI) Legacy Imaging Surveys Data Release 9, Survey Validation 3, and Year 1 data sets to estimate the conditional luminosity functions and conditional stellar mass functions (CLFs and CSMFs) of galaxies across various halo mass bins and redshift ranges. To support our analysis, we utilize a realistic DESI mock galaxy redshift survey (MGRS) generated from a high-resolution Jiutian simulation. An extended halo-based group finder is applied to both MGRS catalogs and DESI observation. By comparing the r - and z -band luminosity functions (LFs) and stellar mass functions (SMFs) derived using both photometric and spectroscopic data, we quantified the impact of photometric redshift (photo- z ) errors on the galaxy LFs and SMFs, especially in the low-redshift bin at the low-luminosity/mass end. By conducting prior evaluations of the group finder using MGRS, we successfully obtain a set of CLF and CSMF measurements from observational data. We find that at low redshift, the faint-end slopes of CLFs and CSMFs below ∼10 ^9 h ^−2 L _⊙ (or h ^−2 M _⊙ ) evince a compelling concordance with the subhalo mass functions. After correcting the cosmic variance effect of our local Universe following Chen et al., the faint-end slopes of the LFs/SMFs turn out to also be in good agreement with the slope of the halo mass function.
Keywords
