The IAU working definition of an exoplanet
AL Des Etangs, JJ Lissauer - New Astronomy Reviews, 2022 - Elsevier
In antiquity, all of the enduring celestial bodies that were seen to move relative to the
background sky of stars were considered planets. During the Copernican revolution, this …
background sky of stars were considered planets. During the Copernican revolution, this …
A Jovian analogue orbiting a white dwarf star
Studies, have shown that the remnants of destroyed planets and debris-disk planetesimals
can survive the volatile evolution of their host stars into white dwarfs,, but few intact planetary …
can survive the volatile evolution of their host stars into white dwarfs,, but few intact planetary …
An isolated mass-gap black hole or neutron star detected with astrometric microlensing
We present the analysis of five black hole candidates identified from gravitational
microlensing surveys. Hubble Space Telescope astrometric data and densely sampled light …
microlensing surveys. Hubble Space Telescope astrometric data and densely sampled light …
Predictions of the WFIRST microlensing survey. I. Bound planet detection rates
Abstract The Wide Field InfraRed Survey Telescope (WFIRST) is the next NASA
astrophysics flagship mission, to follow the James Webb Space Telescope. The WFIRST …
astrophysics flagship mission, to follow the James Webb Space Telescope. The WFIRST …
OGLE-2019-BLG-0960 Lb: the smallest microlensing planet
JC Yee, W Zang, A Udalski, YH Ryu… - The Astronomical …, 2021 - iopscience.iop.org
We report the analysis of OGLE-2019-BLG-0960, which contains the smallest mass-ratio
microlensing planet found to date (q= 1.2–1.6× 10− 5 at 1σ). Although there is substantial …
microlensing planet found to date (q= 1.2–1.6× 10− 5 at 1σ). Although there is substantial …
Systematic KMTNet Planetary Anomaly Search. II. Six New q< 2× 10− 4 Mass-ratio Planets
KH Hwang, W Zang, A Gould, A Udalski… - The Astronomical …, 2022 - iopscience.iop.org
We apply the automated AnomalyFinder algorithm of Paper I to 2018–2019 light curves from
the≃ 13 deg 2 covered by the six KMTNet prime fields, with cadences Γ≥ 2 hr− 1. We find a …
the≃ 13 deg 2 covered by the six KMTNet prime fields, with cadences Γ≥ 2 hr− 1. We find a …
WFIRST Exoplanet Mass-measurement Method Finds a Planetary Mass of 39±8 M⊕ for OGLE-2012-BLG-0950Lb
A Bhattacharya, JP Beaulieu, DP Bennett… - The Astronomical …, 2018 - iopscience.iop.org
WFIRST Exoplanet Mass-measurement Method Finds a Planetary Mass of 39 ± 8 M⊕ for
OGLE-2012-BLG-0950Lb - IOPscience This site uses cookies. By continuing to use this site you …
OGLE-2012-BLG-0950Lb - IOPscience This site uses cookies. By continuing to use this site you …
Systematic KMTNet Planetary Anomaly Search. VII. Complete Sample of q< 10− 4 Planets from the First 4 yr Survey
W Zang, YK Jung, H Yang, X Zhang… - The Astronomical …, 2023 - iopscience.iop.org
We present the analysis of seven microlensing planetary events with planet/host mass ratios
q< 10− 4: KMT-2017-BLG-1194, KMT-2017-BLG-0428, KMT-2019-BLG-1806, KMT-2017 …
q< 10− 4: KMT-2017-BLG-1194, KMT-2017-BLG-0428, KMT-2019-BLG-1806, KMT-2017 …
Systematic KMTNet Planetary Anomaly Search. IX. Complete Sample of 2016 Prime-field Planets
IG Shin, JC Yee, W Zang, H Yang… - The Astronomical …, 2023 - iopscience.iop.org
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 …
planets (namely, OGLE-2016-BLG-1635Lb, MOA-2016-BLG-532Lb, KMT-2016-BLG …
Modeling microlensing events with MulensModel
R Poleski, JC Yee - Astronomy and computing, 2019 - Elsevier
We introduce MulensModel, a software package for gravitational microlensing modeling.
The package provides a framework for calculating microlensing model magnification curves …
The package provides a framework for calculating microlensing model magnification curves …