428 citations
- Purdue University West LafayetteUS37 papers
- University of California, Los AngelesUS36 papers
- Centre National de la Recherche ScientifiqueFR31 papers
- Center for Astrophysics Harvard & SmithsonianUS30 papers
- University of California, Santa CruzUS30 papers
- Yale UniversityUS29 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di PadovaIT28 papers
- Lawrence Berkeley National LaboratoryUS26 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR25 papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR25 papers
- The Ohio State UniversityUS25 papers
- Heidelberg UniversityDE23 papers
17 papers · 1 filter
Line Intensity Mapping Prediction from the Cosmic Dawn (CoDa) III Simulation for H from Galaxies and the Intergalactic Medium during the Epoch of Reionization
Eugene Hyeonmin Lee, Joohyun Lee, Paul R. Shapiro +13
The evolution of large-scale structure, galaxies and the intergalactic medium (IGM) during the Epoch of Reionization (EoR) can be probed by upcoming Line Intensity Mapping (LIM) ex…
The Nature of LoBAL QSOs: II. HST/WFC3 Observations Reveal Host Galaxies Dominated by Mergers
Mariana S. Lazarova, Gabriela Canalizo, Mark Lacy +4
Low-ionization Broad Absorption Line QSOs (LoBALs) are suspected to be merging systems in which extreme, AGN-driven outflows have been triggered. Whether or not LoBALs are uniquely…
The Lick AGN Monitoring Project 2016: Dynamical Modeling of Velocity-Resolved H\b{eta} Lags in Luminous Seyfert Galaxies
Lizvette Villafaña, Peter R. Williams, Tommaso Treu +62
We have modeled the velocity-resolved reverberation response of the H\b{eta} broad emission line in nine Seyfert 1 galaxies from the Lick Active Galactic Nucleus (AGN) Monitioring…
LLAMA: The - Relation of the most luminous local AGNs
Turgay Caglar, Leonard Burtscher, Bernhard Brand +17
The - relation is considered a result of co-evolution between the host galaxies and their super-massive black holes. For elliptical-bulge hosting inactive gala…
The mass relations between supermassive black holes and their host galaxies at 1<z<2 with HST-WFC3
Xuheng Ding, John Silverman, Tommaso Treu +10
Correlations between the mass of a supermassive black hole and the properties of its host galaxy (e.g., total stellar mass (M*), luminosity (Lhost)) suggest an evolutionary connect…
Where do quasar hosts lie with respect to the size-mass relation of galaxies?
John D. Silverman, Tommaso Treu, Xuheng Ding +8
The evolution of the galaxy size - stellar mass (Mstellar) relation has been a puzzle for over a decade. High redshift galaxies are significantly more compact than galaxies observe…