activity
20172021
most citedThe Hunt for Red Quasars: Luminous Obscured Black Hole Growth Unveiled in the Stripe 82 X-ray Survey

20 citations · 37 across the 3 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2021

Powerful winds in high-redshift obscured and red quasars

Andrey Vayner, Nadia L. Zakamska, Rogemar A. Riffel +10

Quasar-driven outflows must have made their most significant impact on galaxy formation during the epoch when massive galaxies were forming most rapidly. To study the impact of qua…

astro-ph.GA20207 cited

Discovery of a Low-Redshift Damped Ly System in a Foreground Extended Disk Using a Starburst Galaxy Background Illuminator

Christopher M. Dupuis, Sanchayeeta Borthakur, Mansi Padave +3

We present the discovery of a low-redshift damped Ly (DLA) system in the spectrum of background starburst galaxy SDSS J111323.88+293039.3 (). The DLA is at an impact…

astro-ph.GA202010 cited

Spatially-resolved UV diagnostics of AGN feedback: radiation pressure dominates in a prototypical quasar-driven superwind

Jean Somalwar, Sean D. Johnson, Jonathan Stern +5

Galactic-scale winds driven by active galactic nuclei (AGN) are often invoked to suppress star formation in galaxy evolution models, but the mechanisms driving these outflows are h…

astro-ph.GA2019

Host galaxies of high-redshift extremely red and obscured quasars

Nadia L. Zakamska, Ai-Lei Sun, Michael A. Strauss +9

We present Hubble Space Telescope 1.4-1.6 micron images of the hosts of ten extremely red quasars (ERQs) and six type 2 quasar candidates at z=2-3. ERQs, whose bolometric luminosit…

astro-ph.GA2019

ERQs are the BOSS of Quasar Samples: The Highest-Velocity [OIII] Quasar Outflows

S. Perrotta, F. Hamann, N. L. Zakamska +3

We investigate Extremely Red Quasars (ERQs), a remarkable population of heavily-reddened quasars at redshift z2 - 3 that might be caught during a short-lived 'blow-out' phase…

astro-ph.GA2019

Observing AGN feedback with CO intensity mapping

Patrick C. Breysse, Rachael M. Alexandroff

Current models of galaxy formation require star formation in high-mass galaxies to be limited by poorly understood mechanisms of quasar feedback. Feedback processes can be studied…