activity
20162025
most citedNew constraints on the structure of the nuclear stellar cluster of the Milky Way from star counts and MIR imaging

70 citations · 70 across the 3 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2025

The Hubble Space Telescope Survey of M31 Satellite Galaxies IV. Survey Overview and Lifetime Star Formation Histories

A. Savino, D. R. Weisz, A. E. Dolphin +35

From orbits of HST imaging, we present deep homogeneous resolved star color-magnitude diagrams that reach the oldest main sequence turnoff and uniformly measured star forma…

astro-ph.GA2024

The JWST Resolved Stellar Populations Early Release Science Program V. DOLPHOT Stellar Photometry for NIRCam and NIRISS

Daniel R. Weisz, Andrew E. Dolphin, Alessandro Savino +38

We present NIRCam and NIRISS modules for DOLPHOT, a widely-used crowded field stellar photometry package. We describe details of the modules including pixel masking, astrometric al…

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.GA2020★ 70 cited

New constraints on the structure of the nuclear stellar cluster of the Milky Way from star counts and MIR imaging

E. Gallego-Cano, R. Schödel, F. Nogueras-Lara +5

The Milky Way nuclear star cluster (MWNSC) is a crucial laboratory for studying the galactic nuclei of other galaxies, but its properties have not been determined unambiguously unt…

astro-ph.GA2017

The Orbit and Origin of the Ultra-faint Dwarf Galaxy Segue 1

T. K. Fritz, M. Lokken, N. Kallivayalil +4

We present the first proper motion measurement for an ultra-faint dwarf spheroidal galaxy, Segue 1, using SDSS and LBC data as the first and second epochs separated by a baseline o…

astro-ph.GA2016

The Proper Motion of Pyxis: the first use of Adaptive Optics in tandem with HST on a faint halo object

Tobias K. Fritz, Sean T. Linden, Paul Zivick +13

We present a proper motion measurement for the halo globular cluster Pyxis, using HST/ACS data as the first epoch, and GeMS/GSAOI Adaptive Optics data as the second, separated by a…