Results 71 to 80 of about 168,724 (208)

Detectability of microlensed gravitational waves

open access: yesMonthly Notices of the Royal Astronomical Society, 2023
ABSTRACT Gravitational lensing describes the bending of the trajectories of light and gravitational waves due to the gravitational potential of a massive object. Strong lensing by galaxies can create multiple images with different overall amplifications, arrival times, and image types. If, furthermore, the gravitational wave encounters a
Simon M C Yeung   +5 more
openaire   +2 more sources

Gravitational Microlensing timeline

open access: yes, 2016
An infographic about how gravitational microlensing, the warping of spacetime, can be used to discover new ...
Edward Gomez (3093198)
core   +1 more source

Microlensing of circumstellar envelopes: II. emission lines from radial and azimuthal flow during fold caustic crossings [PDF]

open access: yes, 2003
This paper examines the line profile evolution due to bulk motion in circumstellar envelopes during microlensing fold caustic crossing events. These events have recently been shown to be a sensitive probe of stellar surface brightness profiles, thus ...
Bryce, H.M.   +5 more
core   +1 more source

Systematic KMTNet Planetary Anomaly Search. X. Complete Sample of 2017 Prime-field Planets

open access: yesThe Astronomical Journal
We complete the analysis of planetary candidates found by the KMT AnomalyFinder for the 2017 prime fields that cover ∼13 deg ^2 . We report three unambiguous planets: OGLE-2017-BLG-0640, OGLE-2017-BLG-1275, and OGLE-2017-BLG-1237.
Yoon-Hyun Ryu   +45 more
doaj   +1 more source

Degeneracies in triple gravitational microlensing [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2013
We study microlensing light curves by a triple lens, in particular, by a primary star plus two planets. A four-fold degeneracy is confirmed in the light curves, similar to the close and wide degeneracy found in a double lens. Furthermore, we derive a set of equations for triple-lens in the external shear approximation.
Mao, Shude   +3 more
openaire   +3 more sources

Gravitational microlensing: Results and perspectives in brief [PDF]

open access: yesPhysics of Particles and Nuclei, 2008
8 pages, 1 figure, An invited lecture at the Helmholtz International Summer School "Dense Matter in Heavy Ion Collisions and Astrophysics", Bogoliubov Laboratory of Theoretical Physics, Joint Institute for Nuclear Research, Dubna, Russia, August 21 - September 1, 2006, added reference, corrected ...
openaire   +2 more sources

Accretion Disk Size and Updated Time-delay Measurements in the Gravitationally Lensed Quasar SDSS J165043.44+425149.3

open access: yesThe Astrophysical Journal
We analyze variability in 15-season optical lightcurves from the doubly imaged lensed quasar SDSS J165043.44+425149.3 (SDSS1650), comprising five seasons of monitoring data from the Maidanak Observatory (277 nights in total, including the two seasons of ...
A. B. Rivera   +12 more
doaj   +1 more source

The gravitational microlens influence on X-ray spectral line generated by an AGN accretion disc [PDF]

open access: yesSerbian Astronomical Journal, 2001
The influence of gravitational microlensing on the X-ray spectral line profiles originated from a relativistic accretion disc has been studied. Using a disc model, we show that microlensing can induce noticeable changes in the line shapes when the ...
Popović L.Č.   +4 more
doaj   +1 more source

Gravitational Microlensing by a Galactic Bar

open access: yesThe Astronomical Journal, 1995
Observations have found that the microlensing optical depth in the direction of the galactic center is larger than theoretical predictions. Here we investigate the effect a galactic bar has on microlensing. We use two models for the bar in order to find the range of microlensing predications.
openaire   +1 more source

Residual Test to Search for Microlensing Signatures in Strongly Lensed Gravitational Wave Signals

open access: yesThe Astrophysical Journal
When a gravitational wave signal encounters a massive object, such as a galaxy or galaxy cluster, it undergoes strong gravitational lensing, producing multiple copies of the original signal.
Eungwang Seo   +5 more
doaj   +1 more source

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