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An Updated SYNTHPOP Model for Microlensing Simulations. I. Model Description and Evaluation

  • Authors: Macy J. Huston, Alison L. Crisp, Marz Newman, Riley Patlak, Matthew T. Penny, Jonas Klüter, Samson A. Johnson, Peter McGill, Leigh C. Smith, Victor Karkour, Natasha S. Abrams, Tabetha S. Boyajian, Rachel B. Fernandes, B. Scott Gaudi, Eamonn Kerins, Casey Y. Lam, Jessica R. Lu, Carissma McGee, Sebastiano Calchi Novati, Keivan G. Stassun, Sean K. Terry, Emelly D. Tiburcio, Himanshu Verma, Farzaneh Zohrabi

Macy J. Huston et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 11.

The mean RVs (top row) and mean velocity dispersions (bottom row) of simulated SP-H25 catalogs compared to the observed values from the Bulge Radial Velocity Assay (BRAVA) survey. Each color represents a different galactic latitude, b. In the mean RV panels, the solid black lines represent the best-fit line of the SYNTHPOP data, while the dashed black lines represent the best-fit line of the BRAVA data. The slope of each is given at the top of the respective panels.

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