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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 5.

Examples of detection efficiency curves. Fields GD2410 and BLG822 have been observed for less than 500 days and so sensitivity to long-timescale events in these fields is low. The detection efficiency curves have different normalizations, because the analyzed fields were observed for different lengths of time. (The detection efficiencies measured in our simulations have been multiplied by a factor of (tmaxtmin)/ΔT, where tmin and tmax are moments of the first and last observation of a given field and ΔT = 2650 days is the duration of the survey.)

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