Figure 6. Near-IR luminosity functions and color

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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 6. Near-IR luminosity functions and color–magnitude diagrams

The complete figure set (7 images) is available in the online journal.

Near-IR LFs (left three panels) and CMDs (right two panels) from GNS (black points) in comparison to SP-H25 model catalogs (blue). In the CMDs, an orange line marks the roughly estimated 80% completeness limit. The “transition zone east” field is shown here as an example, and the six additional fields are available.

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