activity
19992025
most citedMACHO Project Limits on Black Hole Dark Matter in the 1-30 Solar Mass Range

352 citations · 1.3k across the 25 of their papers we have counts for

collaborators

24 papers

astro-ph.GA2025

A Possible "Too-Many-Satellites" Problem in the Isolated Dwarf Galaxy DDO 161

Jiaxuan Li, Jenny E. Greene, Shany Danieli +2

The abundance of satellite galaxies provides a direct test of CDM and galaxy formation physics on small scales. While satellites of Milky Way-mass galaxies are well studied, tho…

astro-ph.GA2025

ELVES-Dwarf I: Satellites Systems of Eight Isolated Dwarf Galaxies in the Local Volume

Jiaxuan Li, Jenny E. Greene, Shany Danieli +4

The satellite populations of Milky Way--mass systems have been extensively studied, significantly advancing our understanding of galaxy formation and dark matter physics. In contra…

astro-ph.GA2025★ 2 cited

The Morphology of Dwarf Galaxies Hosting Variable Active Galactic Nuclei

Erin Kimbro, Vivienne Baldassare, Guy Worthey +2

We analyze Hubble Space Telescope (HST) optical imaging of eight low-mass galaxies hosting active galactic nuclei (AGN) identified via their photometric variability in \cite{baldas…

astro-ph.GA2024★ 1 cited

Multi-wavelength constraints on the local black hole occupation fraction

Colin J. Burke, Priyamvada Natarajan, Vivienne F. Baldassare +1

The fraction of dwarf galaxies hosting central, intermediate-mass black holes (IMBHs) at low redshifts is an important observational probe of black hole seeding at high redshift. D…

astro-ph.GA2024

SAGAbg II: the Low-Mass Star-Forming Sequence Evolves Significantly Between 0.05<z<0.21

Erin Kado-Fong, Marla Geha, Yao-Yuan Mao +8

The redshift-dependent relation between galaxy stellar mass and star formation rate (the Star-Forming Sequence, or SFS) is a key observational yardstick for galaxy assembly. We use…

astro-ph.GA2024★ 1 cited

Stellar Mass Calibrations for Local Low-Mass Galaxies

Mithi A. C. de los Reyes, Yasmeen Asali, Risa Wechsler +10

The stellar masses of galaxies are measured using integrated light via several methods -- however, few of these methods were designed for low-mass ($M_{\star}\lesssim10^{8}\rm{M_{\…