activity
19962023
most citedLSST: from Science Drivers to Reference Design and Anticipated Data Products

3.5k citations · 42.3k across the 239 of their papers we have counts for

collaborators

241 papers

astro-ph.GA2023★ 4 cited

Accretion onto disk galaxies via hot and rotating CGM inflows

Jonathan Stern, Drummond Fielding, Zachary Hafen +5

Observed accretion rates onto the Milky-Way and other local spirals fall short of that required to sustain star formation for cosmological timescales. A potential avenue for this u…

astro-ph.GA2023

The Halo21 Absorption Modeling Challenge: Lessons From "Observing" Synthetic Circumgalactic Absorption Spectra

Zachary Hafen, Sameer, Cameron Hummels +7

In the Halo21 absorption modeling challenge we generated synthetic absorption spectra of the circumgalactic medium (CGM), and attempted to estimate the metallicity, temperature, an…

astro-ph.GA2023

The Hubble Space Telescope Survey of M31 Satellite Galaxies II. The Star Formation Histories of Ultra-Faint Dwarf Galaxies

A. Savino, D. R. Weisz, E. D. Skillman +34

We present the lifetime star formation histories (SFHs) for six ultra-faint dwarf (UFD; , ) satellite galaxies of M31 based on…

astro-ph.CO2023

An analytic surface density profile for CDM halos and gravitational lensing studies

Alexandres Lazar, James S. Bullock, Anna Nierenberg +2

We introduce an analytic surface density profile for dark matter halos that accurately reproduces the structure of simulated halos of mass , makin…

astro-ph.GA2023★ 3 cited

The JWST Resolved Stellar Populations Early Release Science Program II. Survey Overview

Daniel R. Weisz, Kristen B. W. McQuinn, Alessandro Savino +39

We present the JWST Resolved Stellar Populations Early Release Science (ERS) science program. We obtained 27.5 hours of NIRCam and NIRISS imaging of three targets in the Local Grou…

astro-ph.GA2023★ 95 cited

What Causes The Formation of Disks and End of Bursty Star Formation?

Philip F. Hopkins, Alexander B. Gurvich, Xuejian Shen +17

As they grow, galaxies can transition from irregular/spheroidal with 'bursty' star formation histories (SFHs), to disky with smooth SFHs. But even in simulations, the direct physic…