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Title: Environmental Quenching of Low-surface-brightness Galaxies Near Hosts from Large Magellanic Cloud to Milky Way Mass Scales

Journal Article · · Astrophys.J.
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  1. Ohio State U., Dept. Astron.; Ohio State U., CCAPP
  2. Ohio State U., Dept. Astron.; Ohio State U.; Ohio State U., CCAPP; Princeton, Inst. Advanced Study
  3. Ohio State U., Dept. Astron.; Ohio State U.; Ohio State U., CCAPP
  4. Dartmouth Coll.; Chicago U., Astron. Astrophys. Ctr.; Chicago U., KICP
  5. Chicago U., Astron. Astrophys. Ctr.; Chicago U., KICP; Fermilab
  6. Carnegie Mellon U.
  7. Texas A-M
  8. Durham U.
  9. Ohio State U., CCAPP
  10. Chicago U., KICP
  11. LIneA, Rio de Janeiro
  12. U. Michigan, Ann Arbor
  13. Portsmouth U., ICG
  14. University Coll. London
  15. IAC, La Laguna; LIneA, Rio de Janeiro; Laguna U., Tenerife
  16. Barcelona, IFAE
  17. Hamburg Observ.
  18. Queensland U.
  19. Indian Inst. Tech., Hyderabad
  20. Inst. Theor. Astrophys., Oslo
  21. Fermilab; Chicago U., KICP
  22. Madrid, IFT
  23. Barcelona, IFAE; Chicago U., KICP
  24. Munich U.
  25. NCSA, Urbana; Illinois U., Urbana, Astron. Dept.
  26. UC, Santa Cruz
  27. Ohio State U., CCAPP; Ohio State U.
  28. Harvard-Smithsonian Ctr. Astrophys.
  29. Australian Astron. Observ.; Lowell Observ.
  30. LPSC, Grenoble
  31. ICREA, Barcelona; Barcelona, Autonoma U.; Barcelona, IFAE
  32. LIneA, Rio de Janeiro; Rio de Janeiro Observ.
  33. KIPAC, Menlo Park; SLAC
  34. Madrid, CIEMAT
  35. Rio Grande do Sul U.; LIneA, Rio de Janeiro
  36. Southampton U.
  37. ORNL, Oak Ridge (main)
  38. NCSA, Urbana
  39. Portsmouth U., ICG; Southampton U.
  40. Cerro-Tololo InterAmerican Obs.
  41. U. Michigan, Ann Arbor; LBL, Berkeley

Low-surface-brightness galaxies (LSBGs) are excellent probes of quenching and other environmental processes near massive galaxies. We study an extensive sample of LSBGs near massive hosts in the local universe that are distributed across a diverse range of environments. The LSBGs with surface-brightness μeff,g>24.2magarcsec−2are drawn from the Dark Energy Survey Year 3 catalog while the hosts with masses 9.0

Research Organization:
Australian Astron. Observ.; Barcelona, Autonoma U.; Barcelona, IFAE; Carnegie Mellon U.; Cerro-Tololo InterAmerican Obs.; Chicago U., Astron. Astrophys. Ctr.; Chicago U., KICP; Dartmouth Coll.; Durham U.; Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); Hamburg Observ.; Harvard-Smithsonian Ctr. Astrophys.; IAC, La Laguna; ICREA, Barcelona; Illinois U., Urbana, Astron. Dept.; Indian Inst. Tech., Hyderabad; Inst. Theor. Astrophys., Oslo; LIneA, Rio de Janeiro; LPSC, Grenoble; Laguna U., Tenerife; Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States); Lowell Observ.; Madrid, CIEMAT; Madrid, IFT; Munich U.; NCSA, Urbana; Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States); Ohio State U.; Ohio State U., CCAPP; Ohio State U., Dept. Astron.; Portsmouth U., ICG; Princeton, Inst. Advanced Study; Queensland U.; Rio Grande do Sul U.; Rio de Janeiro Observ.; SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States); Southampton U.; Texas A-M; U. Michigan, Ann Arbor; UC, Santa Cruz; University Coll. London
Sponsoring Organization:
US Department of Energy; USDOE Office of Science (SC), High Energy Physics (HEP)
Contributing Organization:
Dark Energy Survey Collaboration; Fermi National Accelerator Laboratory (FNAL); Lawrence Berkeley National Laboratory (LBNL); Oak Ridge National Laboratory (ORNL)
Grant/Contract Number:
89243024CSC000002; AC02-07CH11359; AC02-76SF00515; AC05-00OR22725
OSTI ID:
2283687
Report Number(s):
DES-2023-0789; FERMILAB-PUB--23-743; FERMILAB-PUB-23-743; arXiv:2312.00773; oai:inspirehep.net:2729400; oai:inspirehep.net:2729400; arXiv:2312.00773
Journal Information:
Astrophys.J., Journal Name: Astrophys.J. Journal Issue: 2 Vol. 975
Country of Publication:
United States
Language:
English