Latest Images
The radio and X-ray light curves of the 2025 fl...
Averaged PDS, averaged LS periodogram, and dyna...
The distributions of the maximum TR from each s...
The basic geometry of a point-source, point-len...
The BAGLE Python package includes microlensing ...
A microlensing event as viewed from heliocentri...
A BAGLE model for a PSPL with a parallax with a...
The on-sky photometry (top) and astrometry (mid...
Top: reproduced from Figure 1 of V. A. Belokuro...
Comparison of a simulated PSPL event without a ...
Comparison between BAGLE, VBMicrolensing, and p...
Comparison of an FSPL lightcurve with a PSPL li...
Comparison of a simulated PSPL event’s amplific...
Comparison of the source’s centroid shift betwe...
The impact of blending on the photometry (top p...
Comparison between BAGLE, pyLIMA, and VBMicrole...
The impact of changing the lens mass in BAGLE m...
The impact of changing the lens parallax in BAG...
Comparison between BAGLE and VBMicrolensing’s a...
Mock photometric (left) and astrometric (middle...
Predicted SNR on the measurement of πE based on...
Heliocentric SSB (⊙) vs. geo-tr (⊕r) parameters...
The observed trajectory on the sky is significa...
Geometry parameterization for our astrometric s...
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