Results 111 to 120 of about 11,137 (251)
Introduction to Gravitational Microlensing
The basic concepts of gravitational microlensing are introduced. We start with the lens equation, and then derive the image positions and magnifications. The statistical quantities of optical depth and event rate are then described. We finish with a summary and a list of challenges and open questions. A problem set is given for students to practice.
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Gravitational Microlensing by Rotating Stars
12 pages, 4 figures, AAS ...
Rahbari, Habib Ebrahimnejad +2 more
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Gravitational microlensing: A parallel, large-data implementation [PDF]
Hugh Garsden, Geraint F. Lewis
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Some previous studies have suggested that massive and intermediate-mass primordial black holes (PBHs) could comprise a substantial fraction of dark matter in the Universe.
Przemek Mróz +14 more
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OGLE-2017-BLG-0448Lb: A Low Mass–Ratio Wide-orbit Microlensing Planet?
The gravitational microlensing technique is most sensitive to planets in a Jupiter-like orbit and has detected more than 200 planets. However, only a few wide-orbit ( s > 2) microlensing planets have been discovered, where s is the planet-to-host ...
Ruocheng Zhai +44 more
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Limits on compact halo objects as dark matter from gravitational microlensing [PDF]
Philippe Jetzer
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A Rapid Microlensing Event in the Q0957+561A, B Gravitational Lens System [PDF]
Wesley N. Colley, Rudolph E. Schild
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Investigating the Binary Source Degeneracy for Wide-orbit Planets
Wide-orbit planets are particularly sensitive to detection by the Roman Galactic Bulge Time Domain Survey (GBTDS). This study investigates the degeneracy of these events with binary sources, focusing on how observation cadence affects the resolution of ...
Parisa Sangtarash, Jennifer C. Yee
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Gravitational Microlensing: Black Holes, Planets; OGLE, VLTI, HST and\n Space Probes [PDF]
B. Paczyński
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Gravitational Microlensing by Globular Clusters
Stars in globular clusters can act either as sources for MACHOs (Massive Astrophysical Compact Halo Objects) located along the line of sight or as lenses for more distant background stars. Although the expected rate of microlensing events is small, such observations can lead to very useful results.
Jetzer, P., Strässle, M., Wandeler, U.
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