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Black Hole Astrometric Binaries in the Roman Galactic Bulge Time Domain Survey

  • Authors: Casey Y. Lam, Jessica R. Lu, Kareem El-Badry, Anil Seth, Joshua D. Simon, Natasha S. Abrams, Andrea Bellini, Matthew W. Hosek, Peter McGill

Casey Y. Lam et al 2026 The Astrophysical Journal Supplement Series 287 .

  • Provider: AAS Journals

Caption: Figure 2.

Schematic of the observational structure of the GBTDS. Six fields toward the Galactic bulge are observed sequentially in a cycle; this is a GBTDS mosaic. During high-cadence observing seasons (the first three and last three seasons), this mosaic is observed continuously; during low-cadence observing seasons (the middle four seasons), this mosaic is observed roughly every 5 days. The filters in which this mosaic is observed are schematically shown; blue is F087, purple is F146, and red is F213. Note that the temporal axis is not drawn to scale.

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