Exoplanet statistics and theoretical implications
In the past few years, significant advances have been made in understanding the
distributions of exoplanet populations and the architecture of planetary systems. We review …
distributions of exoplanet populations and the architecture of planetary systems. We review …
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 …
The Ophiuchus DIsc Survey Employing ALMA (ODISEA)–I: project description and continuum images at 28 au resolution
LA Cieza, D Ruíz-Rodríguez, A Hales… - Monthly Notices of …, 2019 - academic.oup.com
Abstract We introduce the Ophiuchus DIsc Survey Employing ALMA (ODISEA), a project
aiming to study the entire population of Spitzer-selected protoplanetary discs in the …
aiming to study the entire population of Spitzer-selected protoplanetary discs in the …
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 …
The exoplanet mass-ratio function from the MOA-II survey: discovery of a break and likely peak at a neptune mass
D Suzuki, DP Bennett, T Sumi, IA Bond… - The Astrophysical …, 2016 - iopscience.iop.org
We report the results of the statistical analysis of planetary signals discovered in MOA-II
microlensing survey alert system events from 2007 to 2012. We determine the survey …
microlensing survey alert system events from 2007 to 2012. We determine the survey …
Prediction of Planet Yields by the PRime-focus Infrared Microlensing Experiment Microlensing Survey
I Kondo, T Sumi, N Koshimoto… - The Astronomical …, 2023 - iopscience.iop.org
Abstract The PRime-focus Infrared Microlensing Experiment (PRIME) will be the first to
conduct a dedicated near-infrared microlensing survey by using a 1.8 m telescope with a …
conduct a dedicated near-infrared microlensing survey by using a 1.8 m telescope with a …
Unstable low-mass planetary systems as drivers of white dwarf pollution
At least of white dwarfs show atmospheric pollution by metals, sometimes accompanied by
detectable circumstellar dust/gas discs or (in the case of WD 1145+ 017) transiting …
detectable circumstellar dust/gas discs or (in the case of WD 1145+ 017) transiting …
JWST/NIRCam Coronagraphy of the Young Planet-hosting Debris Disk AU Microscopii
K Lawson, JE Schlieder, JM Leisenring… - The Astronomical …, 2023 - iopscience.iop.org
High-contrast imaging of debris disk systems permits us to assess the composition and size
distribution of circumstellar dust, to probe recent dynamical histories, and to directly detect …
distribution of circumstellar dust, to probe recent dynamical histories, and to directly detect …
The Large Array Survey Telescope—Science Goals
Abstract The Large Array Survey Telescope (LAST) is designed to survey the variable and
transient sky at high temporal cadence. The array is comprised of 48 F/2.2 telescopes of …
transient sky at high temporal cadence. The array is comprised of 48 F/2.2 telescopes of …
Systematic KMTNet planetary anomaly search. IV. Complete sample of 2019 prime-field
We report the complete statistical planetary sample from the prime fields (Γ≥ 2 h− 1) of the
2019 Korea Microlensing Telescope Network (KMTNet) microlensing survey. We develop …
2019 Korea Microlensing Telescope Network (KMTNet) microlensing survey. We develop …