activity
20242026
collaborators

7 papers

astro-ph.GA2026

An Acceleration is Worth a Hundred Thousand Phase Space Measurements

Thomas Donlon, Sukanya Chakrabarti, Elena D'Onghia

It is now possible to directly measure the accelerations that arise from the distribution of (dark) matter in the Milky Way. These acceleration-based measurements of the local dark…

astro-ph.GA2026

Weighing the Milky Way's Satellite Galaxies Using Pulsar Accelerations

Thomas Donlon, Sukanya Chakrabarti, Jason A. S. Hunt

The properties of dwarf galaxies orbiting the Milky Way (MW) are useful for testing models of the formation of our Galaxy, and by extension various theories of cosmology. Recent ef…

astro-ph.GA2026

Mean Mass Density near the Sun from the Divergence Theorem and Pulsar Accelerations

Thomas Donlon, Lawrence M. Widrow, Sukanya Chakrabarti

We introduce a new, non-parametric method for estimating the mass enclosed within a sphere of arbitrary radius centered on the Sun. The method is based on the divergence theorem as…

astro-ph.HE2025

Empirical Modeling of Magnetic Braking in Millisecond Pulsars to Measure the Local Dark Matter Density and Effects of Orbiting Satellite Galaxies

Thomas Donlon, Sukanya Chakrabarti, Sophia Vanderwaal +3

We present a novel method that enables us to estimate the acceleration of individual millisecond pulsars (MSPs) using only their spin period and its time derivative. For our binary…

astro-ph.GA2025

Chemical Components in the Virgo Overdensity and Hercules-Aquila Cloud: hints of more than one merger event in GSE-like debris

Haoyang Liu, Cuihua Du, Thomas Donlon +1

Using elemental abundances for 1.26 million K giants in the LAMOST DR8 value-added catalog, we analyze the chemical abundances of the Virgo Overdensity (VOD) and Hercules-Aquila Cl…

astro-ph.SR2025

The Anomalous Acceleration of PSR J2043+1711: Long-Period Orbital Companion or Stellar Flyby?

Thomas Donlon, Sukanya Chakrabarti, Michael T. Lam +53

Based on the rate of change of its orbital period, PSR J2043+1711 has a substantial peculiar acceleration of 3.5 0.8 mm/s/yr, which deviates from the acceleration predicted b…