activity
20162026
most citedCOSMIC Variance in Binary Population Synthesis

300 citations · 2.3k across the 64 of their papers we have counts for

collaborators
Showing 2025Show all

10 papers · 1 filter

astro-ph.IM2025

Picture an Astronomer: Best Practices for Retaining Talent in Astrophysics

Ava Polzin, Katherine E. Whitaker, C. Megan Urry +85

Women are consistently underrepresented in astrophysics yet are simultaneously subject to disproportionate attrition at every career stage. This disparity between demonstrated effi…

astro-ph.HE2025

Lucky Strikes: On the Origins of GW190814 Through Isolated Binary Evolution

Ignacio Magaña Hernandez, Katelyn Breivik

The asymmetric nature of GW190814, particularly its mass ratio (), has made its astrophysical origin elusive. We explore isolated binary evolution as a potential ex…

astro-ph.SR2025

Gaia's promise to detect compact-object binaries: where we stand with the third data release

Chirag Chawla, Sourav Chatterjee, Katelyn Breivik

With its third data release (DR3), Gaia begins unveiling dormant candidate compact object (CO) binaries with luminous companions (LC) as predicted by several past theoretical studi…

astro-ph.SR2025★ 4 cited

Betelgeuse's Buddy: X-Ray Constraints on the Nature of Ori B

Anna J. G. O'Grady, Brendan O'Connor, Jared A. Goldberg +8

The d Long Secondary Period of Betelgeuse's optical lightcurve and radial velocity motivated the prediction of a low-mass stellar companion, expected to be at maximal a…

astro-ph.SR2025★ 1 cited

Betelgeuse, Betelgeuse, Betelgeuse, Betel-buddy? Constraints on the dynamical companion to Orionis from HST

Jared A. Goldberg, Anna J. G. O'Grady, Meridith Joyce +10

Recently, two independent analyses have asserted that the cause of the Long Secondary Period (LSP) observed in the variability spectrum of our nearest red supergiant, Betelgeuse ($…

astro-ph.SR2025

Delayed and Displaced: The Impact of Binary Interactions on Core-collapse SN Feedback

Tom Wagg, Julianne J. Dalcanton, Mathieu Renzo +7

Core-collapse supernova feedback models in hydrodynamical simulations typically assume that all stars evolve as single stars. However, the majority of massive stars are formed in b…