Microlensing searches for exoplanets
Y Tsapras - Geosciences, 2018 - mdpi.com
Gravitational microlensing finds planets through their gravitational influence on the light
coming from a more distant background star. The presence of the planet is then inferred from …
coming from a more distant background star. The presence of the planet is then inferred from …
Mid-to-late M Dwarfs Lack Jupiter Analogs
Cold Jovian planets play an important role in sculpting the dynamical environment in which
inner terrestrial planets form. The core accretion model predicts that giant planets cannot …
inner terrestrial planets form. The core accretion model predicts that giant planets cannot …
Gravitational microlensing I: A unique astrophysical tool
S Rahvar - International Journal of Modern Physics D, 2015 - World Scientific
In this paper, we review the astrophysical application of gravitational microlensing. After
introducing the history of gravitational lensing, we present the key equations and concept of …
introducing the history of gravitational lensing, we present the key equations and concept of …
KMT-2021-BLG-0171Lb and KMT-2021-BLG-1689Lb: two microlensing planets in the KMTNet high-cadence fields with followup observations
H Yang, W Zang, A Gould, JC Yee… - Monthly Notices of …, 2022 - academic.oup.com
Follow-up observations of high-magnification gravitational microlensing events can fully
exploit their intrinsic sensitivity to detect extrasolar planets, especially those with small mass …
exploit their intrinsic sensitivity to detect extrasolar planets, especially those with small mass …
The first Neptune analog or super-earth with a Neptune-like orbit: MOA-2013-BLG-605LB
T Sumi, A Udalski, DP Bennett, A Gould… - The Astrophysical …, 2016 - iopscience.iop.org
We present the discovery of the first Neptune analog exoplanet or super-Earth with a
Neptune-like orbit, MOA-2013-BLG-605Lb. This planet has a mass similar to that of Neptune …
Neptune-like orbit, MOA-2013-BLG-605Lb. This planet has a mass similar to that of Neptune …
OGLE-2012-BLG-0563Lb: a Saturn-mass planet around an M dwarf with the mass constrained by Subaru AO imaging
A Fukui, A Gould, T Sumi, DP Bennett… - The Astrophysical …, 2015 - iopscience.iop.org
OGLE-2012-BLG-0563Lb: A SATURN-MASS PLANET AROUND AN M DWARF WITH THE
MASS CONSTRAINED BY SUBARU AO IMAGING - IOPscience Skip to content IOP Science …
MASS CONSTRAINED BY SUBARU AO IMAGING - IOPscience Skip to content IOP Science …
Microlensing constraints on the mass of single stars from HST astrometric measurements
We report on the first results from a large-scale observing campaign aiming to use
astrometric microlensing to detect and place limits on the mass of single objects, including …
astrometric microlensing to detect and place limits on the mass of single objects, including …
Predictions for microlensing planetary events from core accretion theory
We conduct the first microlensing simulation in the context of a planet formation model. The
planet population is taken from the Ida & Lin core accretion model for 0.3 M☉ stars. With …
planet population is taken from the Ida & Lin core accretion model for 0.3 M☉ stars. With …
Is the galactic bulge devoid of planets?
MT Penny, CB Henderson… - The Astrophysical Journal, 2016 - iopscience.iop.org
We consider a sample of 31 exoplanetary systems detected by gravitational microlensing
and investigate whether or not the estimated distances to these systems conform to the …
and investigate whether or not the estimated distances to these systems conform to the …
MOA-2011-BLG-322Lb: a 'second generation survey'microlensing planet
Y Shvartzvald, D Maoz, S Kaspi, T Sumi… - Monthly Notices of …, 2014 - academic.oup.com
Global 'second-generation'microlensing surveys aim to discover and characterize extrasolar
planets and their frequency, by means of round-the-clock high-cadence monitoring of a …
planets and their frequency, by means of round-the-clock high-cadence monitoring of a …