@article{17629,
  abstract     = {We propose an observational test for gravitationally recoiling supermassive black holes in active galactic nuclei, based on a positive correlation between the velocities of black holes relative to their host galaxies, |Δv|, and their obscuring dust column densities, Σdust, both measured along the line of sight. Our findings using a set of toy models implemented to a Monte Carlo simulation imply that models of the galactic centre and of recoil dynamics can be tested by future observations of the potential Σdust–|Δv| correlation. We have also found that the fraction of obscured quasars decreases with |Δv|, for which the predicted trend can be compared to the observed fraction of type II quasars, and can further test combinations of models we may implement.},
  author       = {Raffai, P. and Bécsy, B. and Haiman, Zoltán and Frei, Z.},
  issn         = {1743-9213},
  journal      = {Proceedings of the International Astronomical Union},
  number       = {S324},
  pages        = {227--230},
  publisher    = {Cambridge University Press},
  title        = {{A statistical method for detecting gravitational recoils of supermassive black holes in active galactic nuclei}},
  doi          = {10.1017/s1743921317000734},
  volume       = {12},
  year         = {2017},
}

@article{17749,
  abstract     = {We discuss the UV radiative feedback on high-redshift proto-galaxies.},
  author       = {Mesinger, Andrei and Haiman, Greg L. and Haiman, Zoltán},
  issn         = {1743-9213},
  journal      = {Proceedings of the International Astronomical Union},
  number       = {14},
  pages        = {269--269},
  publisher    = {Cambridge University Press},
  title        = {{UV radiative feedback on high-redshift proto-galaxies}},
  doi          = {10.1017/s1743921307010526},
  volume       = {2},
  year         = {2006},
}