4.7 Article

Metal Lines Associated with the Lyα Forest from eBOSS Data

Journal

ASTROPHYSICAL JOURNAL
Volume 935, Issue 2, Pages -

Publisher

IOP Publishing Ltd
DOI: 10.3847/1538-4357/ac7b2e

Keywords

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Funding

  1. National Key R&D Program of China [2018YFA0404503]
  2. China Scholarship Council [201804910563]
  3. NSF [AST-2007499]
  4. Center for High Performance Computing at the University of Utah
  5. National Research Foundation of Korea (NRF) - Korean Ministry of Education, Science and Technology (MoEST) [2020R1A2C1005655]
  6. Alfred P. Sloan Foundation
  7. U.S. Department of Energy Office of Science
  8. Brazilian Participation Group
  9. Carnegie Institution for Science
  10. Carnegie Mellon University
  11. Center for Astrophysics | Harvard Smithsonian
  12. Chilean Participation Group
  13. French Participation Group
  14. Instituto de Astrofisica de Canarias
  15. Johns Hopkins University
  16. Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo
  17. Korean Participation Group
  18. Lawrence Berkeley National Laboratory
  19. Leibniz Institut fur Astrophysik Potsdam (AIP)
  20. Max-Planck-Institut fur Astronomie (MPIA Heidelberg)
  21. Max-Planck-Institut fur Astrophysik (MPA Garching)
  22. Max-Planck-Institut fur Extraterrestrische Physik (MPE)
  23. National Astronomical Observatories of China
  24. New Mexico State University
  25. New York University
  26. University of Notre Dame
  27. Observatario Nacional/MCTI
  28. Ohio State University
  29. Pennsylvania State University
  30. Shanghai Astronomical Observatory
  31. United Kingdom Participation Group
  32. Universidad Nacional Autonoma de Mexico
  33. University of Arizona
  34. University of Colorado Boulder
  35. University of Oxford
  36. University of Portsmouth
  37. University of Utah
  38. University of Virginia
  39. University of Washington
  40. University of Wisconsin
  41. Vanderbilt University
  42. Yale University

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We investigate the metal species associated with the Ly alpha forest in eBOSS quasar spectra. Up to 13 metal species are identified as being associated with relatively strong Ly alpha absorbers over a specific redshift range. The measurements provide inputs for modeling the metal contamination in the Ly alpha forest and can further elucidate the physical conditions of these absorbers.
We investigate the metal species associated with the Ly alpha forest in eBOSS quasar spectra. Metal absorption lines are revealed in stacked spectra from cross-correlating the selected Ly alpha absorbers in the forest and the flux fluctuation field. Up to 13 metal species are identified as being associated with relatively strong Ly alpha absorbers (those with flux fluctuations - 1.0 < delta (Ly alpha ) < - 0.6 and with a neutral hydrogen column density of similar to 10(15-16) cm(-2)) over the absorber redshift range of 2 < z (abs) < 4. The column densities of these species decrease toward higher redshift and for weaker Ly alpha absorbers. From modeling the column densities of various species, we find that the column density pattern suggests contributions from multiple gas components, both in the circumgalactic medium (CGM) and the intergalactic medium (IGM). While the low-ionization species (e.g., C ii, Si ii, and Mg ii) can be explained by high-density, cool gas (T similar to 10(4) K) from the CGM, the high-ionization species may reside in low-density or high-temperature gas in the IGM. The measurements provide inputs for modeling the metal contamination in the Ly alpha forest baryon acoustic oscillation measurements. Comparisons with metal absorptions in high-resolution quasar spectra and hydrodynamic galaxy formation simulations can further elucidate the physical conditions of these Ly alpha absorbers.

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