activity
20082023
most citedInferences on the Timeline of Reionization at z~8 From the KMOS Lens-Amplified Spectroscopic Survey

244 citations · 1.9k across the 50 of their papers we have counts for

collaborators

48 papers

astro-ph.GA2023★ 10 cited

Constraints on Fluctuating Star Formation Rates for Intermediate-mass Galaxies with H and UV Luminosities

Shannon G. Patel, Daniel D. Kelson, Louis E. Abramson +2

We study the recent star formation histories (SFHs) of 575 intermediate-mass galaxies (IMGs, ) in COSMOS at by comparing their H$α…

astro-ph.GA2022

UV Slopes At All Redshifts Are Consistent with H=1 Stochastic Star Formation Histories

Daniel D. Kelson, Louis E. Abramson

Multiple investigations support describing galaxy growth as a stochastic process with correlations over a range of timescales governed by a parameter, , empirically and theoreti…

astro-ph.GA2022★ 36 cited

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…

astro-ph.GA2021

The Lick AGN Monitoring Project 2016: Velocity-Resolved Hβ Lags in Luminous Seyfert Galaxies

Vivian U, Aaron J. Barth, H. Alexander Vogler +61

We carried out spectroscopic monitoring of 21 low-redshift Seyfert 1 galaxies using the Kast double spectrograph on the 3-m Shane telescope at Lick Observatory from April 2016 to M…

astro-ph.GA2021★ 12 cited

Dynamical Modeling of the CIV Broad Line Region of the Multiply Imaged Quasar SDSS J2222+2745

Peter R. Williams, Tommaso Treu, Håkon Dahle +8

We present CIV BLR modeling results for the multiply imaged quasar SDSS J2222+2745. Using data covering a 5.3 year baseline after accounting for gravitational time delays…

astro-ph.GA2020

At Least One-in-Six Galaxies Is Always Dead

L. E. Abramson, D. D. Kelson

Via numerical experiments, we show that the 10%-20% passive fraction seen at is consistent with galaxy star formation histories being maximally correlated stochastic pr…