Results 71 to 80 of about 11,137 (251)
Systematic KMTNet Planetary Anomaly Search. X. Complete Sample of 2017 Prime-field Planets
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
Residual Test to Search for Microlensing Signatures in Strongly Lensed Gravitational Wave Signals
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
Systematic KMTNet Planetary Anomaly Search. IX. Complete Sample of 2016 Prime-field Planets
As a part of the “Systematic KMTNet Planetary Anomaly Search” series, we report five new planets (namely, OGLE-2016-BLG-1635Lb, MOA-2016-BLG-532Lb, KMT-2016-BLG-0625Lb, OGLE-2016-BLG-1850Lb, and KMT-2016-BLG-1751Lb) and one planet candidate (KMT-2016-BLG-
In-Gu Shin +64 more
doaj +1 more source
The influence of gravitational lensing on the spectra of lensed QSOs
We consider the influence of (milli/micro)lensing on the spectra of lensed QSOs. We propose a method for the observational detection of microlensing in the spectra of lensed QSOs and apply it to the spectra of the three lensed QSOs (PG 1115+080, QSO 1413+
Abajas +42 more
core +1 more source
Detectability of microlensed gravitational waves
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
Diffractive Microlensing I: Flickering Planetesimals at the Edge of the Solar System
Microlensing and occultation are generally studied in the geometric optics limit. However, diffraction may be important when recently discovered Kuiper-Belt objects (KBOs) occult distant stars.
Agol +21 more
core +1 more source
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
Compact object detection in self-lensing binary systems with a main-sequence star
Detecting compact objects by means of their gravitational lensing effect on an observed companion in a binary system has already been suggested almost four decades ago.
A. Mehrabi +38 more
core +1 more source
GRAVITATIONAL MICROLENSING IN THE LOCAL GROUP [PDF]
▪ Abstract The status of searches for gravitational microlensing events of the stars in our galaxy and in other galaxies of the Local Group, the interpretation of the results, some theory, and prospects for the future are reviewed. The searches have already unveiled ∼ 100 events, at least two of them caused by binaries, and have already proven to be ...
openaire +2 more sources
Estimating Microlensing Parameters from Observables and Stellar Isochrones with pyLIMASS
We present pyLIMASS, a novel algorithm for estimating the physical properties of the lensing system in microlensing events. The main idea of pyLIMASS is to combine all available information regarding the microlensing event, defined as observables , and ...
E. Bachelet +2 more
doaj +1 more source

