Figure 4 from Microlensing Optical Depth and Event Rate in the OGLE-IV Galactic Plane Fields

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Microlensing Optical Depth and Event Rate in the OGLE-IV Galactic Plane Fields

Authors: Przemek Mróz, Andrzej Udalski, Michał K. Szymański, Igor Soszyński, Paweł Pietrukowicz, Szymon Kozłowski, Jan Skowron, Radosław Poleski, Krzysztof Ulaczyk, Mariusz Gromadzki, Krzysztof Rybicki, Patryk Iwanek, and Marcin Wrona

2020 The Astrophysical Journal Supplement Series 249 16.

Provider: AAS Journals

Caption: Figure 4.

Comparison between our completeness-corrected stellar luminosity functions (blue dots) and those derived from HST images (black histogram). Names and Galactic coordinates of analyzed fields are in the upper left corner. HST images u6fq1106m and u4829602r (lower panels) are incomplete for I ≳ 20 because of short exposure times (60 and 40 s, respectively).

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