---
res:
  bibo_abstract:
  - Binary black hole mergers encode information about their environment and the astrophysical
    processes that led to their formation. Measuring the redshift dependence of their
    merger rate will help probe the formation and evolution of galaxies and the evolution
    of the star formation rate. Here we compute the cosmic evolution of the merger
    rate for stellar-mass binaries in the disks of active galactic nuclei (AGNs).
    We focus on recent evolution out to redshift z = 2, covering the accessible range
    of current Earth-based gravitational-wave observatories. On this scale, the AGN
    population density is the main contributor to redshift dependence. We find that
    the AGN-assisted merger rate varies by less than a factor of two in the range
    0 < z ≤ 2, comparable to the expected level of evolution for globular clusters,
    but much smaller than the order-of-magnitude evolution for field binaries.@eng
  bibo_authorlist:
  - foaf_Person:
      foaf_givenName: Y.
      foaf_name: Yang, Y.
      foaf_surname: Yang
  - foaf_Person:
      foaf_givenName: I.
      foaf_name: Bartos, I.
      foaf_surname: Bartos
  - foaf_Person:
      foaf_givenName: Zoltán
      foaf_name: Haiman, Zoltán
      foaf_surname: Haiman
      foaf_workInfoHomepage: http://www.librecat.org/personId=7c006e8c-cc0d-11ee-8322-cb904ef76f36
  - foaf_Person:
      foaf_givenName: B.
      foaf_name: Kocsis, B.
      foaf_surname: Kocsis
  - foaf_Person:
      foaf_givenName: S.
      foaf_name: Márka, S.
      foaf_surname: Márka
  - foaf_Person:
      foaf_givenName: H.
      foaf_name: Tagawa, H.
      foaf_surname: Tagawa
  bibo_doi: 10.3847/1538-4357/ab91b4
  bibo_issue: '2'
  bibo_volume: 896
  dct_date: 2020^xs_gYear
  dct_isPartOf:
  - http://id.crossref.org/issn/0004-637X
  - http://id.crossref.org/issn/1538-4357
  dct_language: eng
  dct_publisher: American Astronomical Society@
  dct_title: Cosmic evolution of stellar-mass black hole merger rate in active galactic
    nuclei@
...