Tag Archives: BBH

16 May 2017

  • (abs, pdf) Kern et al., Emulating Simulations of Cosmic Dawn for 21cm Power Spectrum Constraints on Cosmology, Reionization, and X-ray Heating
  • (abs, pdf) McQuinn et al., Galactic Outflows, Star Formation Histories, and Timescales in Starburst Dwarf Galaxies from STARBIRDS
  • (abs, pdf) Shapiro, Black holes, disks and jets following binary mergers and stellar collapse: The narrow range of EM luminosities and accretion rates
  • (abs, pdf) Verstocken et al., SKIRT: hybrid parallelization of radiative transfer simulations

07 Nov 2016

  • (abs, pdf) Kovetz et al., The Black Hole Mass Function from Gravitational Wave Measurements
  • (abs, pdf) Gronke et al., From Mirrors to Windows: Lyman-Alpha Radiative Transfer in a Very Clumpy Medium
  • (abs, pdf) Furlanetto et al., A Minimalist Feedback-Regulated Model for Galaxy Formation During the Epoch of Reionization
  • (abs, pdf) Fialkov & Loeb, Jetted Tidal Disruptions of Stars as a Flag of Intermediate Mass Black Holes at High Redshifts

02 Nov 2016

  • (abs, pdf) Lovell et al., Addressing the too big to fail problem with baryon physics and sterile neutrino dark matter
  • (abs, pdf) Lovell et al., Properties of Local Group galaxies in hydrodynamical simulations of sterile neutrino dark matter cosmologies
  • (abs, pdf) Sarmento et al., Following The Cosmic Evolution Of Pristine Gas I: Implications For Milky Way Halo Stars
  • (abs, pdf) Ryan & MacFadyen, Minidisks in Binary Black Hole Accretion

28 Jun 2016

  • (abs, pdf) Fillingham et al., Under Pressure: Quenching Star Formation in Low-Mass Satellite Galaxies via Stripping
  • (abs, pdf) Wellons & Torrey, An improved probabilistic approach for linking progenitor and descendant galaxy populations using comoving number density
  • (abs, pdf) Madau & Fragos, Radiation Backgrounds at Cosmic Dawn: X-Rays from Compact Binaries
  • (abs, pdf) Meliani et al., Simulations of recoiling black holes: adaptive mesh refinement and radiative transfer
  • (abs, pdf) Chardin et al., Large scale opacity fluctuations in the Lyman alpha forest: evidence for QSOs dominating the ionising UV background at z ~ 5.5-6 ?