The Astrophysical Journal (Jan 2024)
Large-scale Structures in COSMOS2020: Evolution of Star Formation Activity in Different Environments at 0.4 < z < 4
- Sina Taamoli,
- Bahram Mobasher,
- Nima Chartab,
- Behnam Darvish,
- John R. Weaver,
- Shoubaneh Hemmati,
- Caitlin M. Casey,
- Zahra Sattari,
- Gabriel Brammer,
- Peter L. Capak,
- Olivier Ilbert,
- Jeyhan S. Kartaltepe,
- Henry J. McCracken,
- Andrea Moneti,
- David B. Sanders,
- Nicholas Scoville,
- Charles L. Steinhardt,
- Sune Toft
Affiliations
- Sina Taamoli
- ORCiD
- Department of Physics and Astronomy, University of California , Riverside, 900 University Avenue, Riverside, CA 92521, USA
- Bahram Mobasher
- ORCiD
- Department of Physics and Astronomy, University of California , Riverside, 900 University Avenue, Riverside, CA 92521, USA
- Nima Chartab
- ORCiD
- Observatories of the Carnegie Institution of Washington, Pasadena , CA, USA
- Behnam Darvish
- ORCiD
- Department of Physics and Astronomy, University of California , Riverside, 900 University Avenue, Riverside, CA 92521, USA
- John R. Weaver
- ORCiD
- Department of Astronomy, University of Massachusetts , Amherst, MA 01003, USA
- Shoubaneh Hemmati
- ORCiD
- Infrared Processing and Analysis Center , California Institute of Technology, Pasadena, CA 91125, USA
- Caitlin M. Casey
- ORCiD
- Department of Astronomy, The University of Texas at Austin , 2515 Speedway Boulevard Stop C1400, Austin, TX 78712, USA
- Zahra Sattari
- ORCiD
- Department of Physics and Astronomy, University of California , Riverside, 900 University Avenue, Riverside, CA 92521, USA; Observatories of the Carnegie Institution of Washington, Pasadena , CA, USA
- Gabriel Brammer
- ORCiD
- Cosmic Dawn Center (DAWN) , Denmark; Niels Bohr Institute, University of Copenhagen , Jagtvej 128, DK-2200 Copenhagen, Denmark
- Peter L. Capak
- ORCiD
- Infrared Processing and Analysis Center , California Institute of Technology, Pasadena, CA 91125, USA
- Olivier Ilbert
- ORCiD
- Aix Marseille University , CNRS, LAM, Laboratoire d’Astrophysique de Marseille, Marseille, France
- Jeyhan S. Kartaltepe
- ORCiD
- Laboratory for Multiwavelength Astrophysics, School of Physics and Astronomy , Rochester Institute of Technology, 84 Lomb Memorial Drive, Rochester, NY 14623, USA
- Henry J. McCracken
- ORCiD
- Institut d’Astrophysique de Paris , UMR 7095, CNRS, and Sorbonne Université, 98 bis boulevard Arago, F-75014 Paris, France
- Andrea Moneti
- Institut d’Astrophysique de Paris , UMR 7095, CNRS, and Sorbonne Université, 98 bis boulevard Arago, F-75014 Paris, France
- David B. Sanders
- ORCiD
- Institute for Astronomy (IfA), University of Hawaii , 2680 Woodlawn Drive, Honolulu, HI 96822, USA
- Nicholas Scoville
- ORCiD
- California Institute of Technology , 1200 East California Boulevard, Pasadena, CA 91125, USA
- Charles L. Steinhardt
- ORCiD
- Cosmic Dawn Center (DAWN) , Denmark; Niels Bohr Institute, University of Copenhagen , Lyngbyvej 2, DK-2100 Copenhagen Ø, Denmark
- Sune Toft
- ORCiD
- Cosmic Dawn Center (DAWN) , Denmark; Niels Bohr Institute, University of Copenhagen , Jagtvej 128, DK-2200 Copenhagen, Denmark
- DOI
- https://doi.org/10.3847/1538-4357/ad32c5
- Journal volume & issue
-
Vol. 966,
no. 1
p. 18
Abstract
To study the role of environment in galaxy evolution, we reconstruct the underlying density field of galaxies based on COSMOS2020 (The Farmer catalog) and provide the density catalog for a magnitude-limited ( K _s 2.
Keywords
