Results 91 to 100 of about 5,260 (217)
Gravitational Microlensing [PDF]
A gravitational microlensing event occurs when a foreground star passes near our line of site to a background source star. The foreground star acts as a lens, perturbing the image of the source star and amplifying the apparent intensity. Because the lens
Barnes, Wesley M
core +1 more source
How Rare Are TESS Free-floating Planets?
Recently, Kunimoto et al. claimed that a short-lived signal in the Transiting Exoplanet Survey Satellite (TESS) Sector 61 database was possibly caused by a microlensing event with a terrestrial-mass free-floating planet (FFP) lens.
Hongjing Yang +5 more
doaj +1 more source
The WFIRST Exoplanet Microlensing Survey
The Wide Field Infrared Survey Telescope (WFIRST) is a NASA space observatory designed to address key questions about the Universe and the population of extrasolar planets in our Galaxy. WFIRST is planned for launch in the mid-2020s.
Calchi Novati, Sebastiano (5481029) +1 more
core +2 more sources
Data intensive quasar microlensing
Quasar microlensing occurs when a distant quasar's light passes through a foreground galaxy on its way to Earth, providing a unique probe of the quasar's central supermassive black hole.
Georgios Vernardos (19106318)
core +1 more source
Historic microlensing events in the Euclid Galactic Bulge Survey
Context. Microlensing campaigns have a long history of observations covering the Galactic bulge, whereby thousands of detections have been obtained, including many exoplanetary systems.
Bozza V. +49 more
doaj +1 more source
Spin Precession Signatures as an Indicator of Microlensing in Strongly Lensed Gravitational Waves
Microlensing by the stellar field in a strong-lensing galaxy can introduce wave-optics distortions into the waveforms of strongly lensed gravitational waves (SLGWs).
Xikai Shan +3 more
doaj +1 more source
Gamma-Ray Variability Induced by Microlensing on Intermediate Size Structures in Lensed Blazars
Changes of the magnification ratio of images in a lensed blazar, caused by microlensing on individual stars, have been proposed as a probe of the size and velocity of the emission region in the lensed source.
Julian Sitarek, Włodek Bednarek
doaj +1 more source
A visual guide to planetary microlensing [PDF]
The microlensing technique has found 10 exoplanets to date and promises to discover more in the near future. While planetary transit light curves all show a familiar shape, planetary perturbations to microlensing light curves can manifest a wide variety ...
Paul L. Schechter, Leslie A. Rogers
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Single-epoch and Differential Astrometric Microlensing of Quasars
We propose and discuss a new experimental approach to measure the centroid shift induced by gravitational microlensing in the images of lensed quasars (astrometric microlensing).
R. Forés-Toribio +5 more
doaj +1 more source
Parallax Effect in Microlensing Events Due to Free-floating Planets
One of the most important applications of microlensing observations is the detection of free-floating planets (FFPs). The timescale of microlensing due to FFPs ( t _E ) is short (a few days). Discerning the annual parallax effect in observations of these
Parisa Sangtarash, Sedighe Sajadian
doaj +1 more source

