An HST Wide Field Survey of the Galactic Bulge: Overview, Strategy, and First Results
Sean K. Terry, Jay Anderson, Charles A. Beichman, David P. Bennett, Aparna Bhattacharya, Jean-Philippe Beaulieu, B. Scott Gaudi, Joel Green, Macy J. Huston, Jessica R. Lu, Ray A. Lucas, David M. Nataf, Matthew T. Penny, Natalia E. Rektsini, Carolina Rodriguez Sanchez-Vahamonde, Aikaterini Vandorou
astro-ph.GA, astro-ph.EP, astro-ph.SR
Submitted: 2026-05-07
Comments: 20 pages, 6 figures, published in ApJL
License: http://creativecommons.org/licenses/by/4.0/
The gist: We present an HST imaging survey of a 1.1 sq.
Terminology
Abstract
We present an HST imaging survey of a 1.1 sq. degree sky area toward the Milky Way Galactic Bulge. This field significantly overlaps with the upcoming Nancy Grace Roman Galactic Bulge Time Domain Survey (GBTDS). High angular resolution imaging of this area with HST before the start of the Roman Galactic Exoplanet Survey (RGES) will greatly strengthen Roman's ability to characterize detected exoplanet systems, as well as provide a rich and wide-field archive for use as a legacy dataset toward the Galactic Bulge for the broader community. We conduct coordinated-parallel imaging with both wide-field cameras on HST, Wide-field Camera 3 (WFC3) and Advanced Camera for Surveys (ACS), utilizing the F606W and F814W passbands. Approximately 70% of the survey was conducted during HST Cycle 32, with the remaining 30% conducted during Cycle 33. In this paper, the first in a series, we give a general overview of the program and the observing strategy, and present early results. This campaign secures HST's lasting impact on the high-precision study of stellar populations, dynamics, exoplanet systems, interstellar extinction, metallicities, cluster associations, and more toward the center of our Galaxy.
Sources
- "Auxiliary" Science with the WFIRST Microlensing Survey
- WFIRST Ultra-Precise Astrometry I: Kuiper Belt Objects
- WFIRST Ultra-Precise Astrometry II: Asteroseismology
- An isolated mass gap black hole or neutron star detected with astrometric microlensing
- Introduction to Gravitational Microlensing
- Microlensing optical depth and event rate toward the Galactic bulge from 8 yr of OGLE-IV observations
- Predictions of the Nancy Grace Roman Space Telescope Galactic Exoplanet Survey. V. Detection Rates of Multiplanetary Systems in High Magnification Microlensing Events
- Deriving Stellar Properties, Distances, and Reddenings using Photometry and Astrometry with BRUTUS
- Wide-Field InfrarRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA 2015 Report
- The Galactic Center with Roman
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