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Light curve follow up of MOA-2020-BLG-208L
We analyze the MOA-2020-BLG-208 gravitational microlensing event and present the discovery and characterization of a new planet, MOA-2020-BLG-208Lb, with an estimated sub-Saturn... -
Terrestrial planets in the Venus zone
Understanding the physical characteristics of Venus, including its atmosphere, interior, and its evolutionary pathway with respect to Earth, remains a vital component for... -
HARPS-N radial velocities of TOI-1695
Characterizing the bulk compositions of transiting exoplanets within the M-dwarf radius valley offers a unique means to establish whether the radius valley emerges from an... -
Tull RVels, rotation periods and Inclinations
The orientation between a star's spin axis and a planet's orbital plane provides valuable information about the system's formation and dynamical history. For non-transiting... -
List of Exoplanet Radial Velocity "green prime"
Future direct imaging missions similar to the HabEx and LUVOIR mission concepts aim to catalog and characterize Earth-mass analogs around nearby stars. The exoplanet yield of... -
Planetary Orbit Eccentricity Trends (POET). I.
Orbital eccentricity is one of the basic planetary properties, whose distribution may shed light on the history of planet formation and evolution. Here, in a series of works on... -
g and i'-band light curve of TOI-5205 with SDSS
We present the discovery of TOI-5205b, a transiting Jovian planet orbiting a solar metallicity M4V star, which was discovered using Transiting Exoplanet Survey Satellite... -
KPIC radial velocity follow up of HR 7672 B
The detection of satellites around extrasolar planets, so called exomoons, remains a largely unexplored territory. In this work, we study the potential of detecting these... -
Emergent spectral IR fluxes of 122 hot Jupiters
We study the emergent spectral fluxes of transiting hot Jupiters, using secondary eclipses from Spitzer. To achieve a large and uniform sample, we have reanalyzed all secondary... -
Systematic KMTNet Planetary Anomaly Search. VII.
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,... -
TESS-Keck Survey. XIII. TOI-1272 radial velocity
We report the discovery of an eccentric hot Neptune and a non-transiting outer planet around TOI-1272. We identified the eccentricity of the inner planet, with an orbital period... -
SPIRou and IRD radial velocity of TOI-1452
Exploring the properties of exoplanets near or inside the radius valley provides insight on the transition from the rocky super-Earths to the larger, hydrogen-rich atmosphere... -
Elemental abundances of JWST target. I. FGK stars
With the launch of the JWST, we will obtain more precise data for exoplanets than ever before. However, these data can only inform and revolutionize our understanding of... -
Radial velocity and photometric flux of TOI-3757
We present the discovery of a new Jovian-sized planet, TOI-3757b, the lowest-density transiting planet known to orbit an M dwarf (M0V). This planet was discovered around a... -
Light curve of microlensing MOA-2019-BLG-008L
We report on the observations, analysis and interpretation of the microlensing event MOA-2019-BLG-008. The observed anomaly in the photometric light curve is best described... -
The TESS Grand Unified Hot Jupiter Survey I. 10 planets
Hot Jupiters-short-period giant planets-were the first extrasolar planets to be discovered, but many questions about their origin remain. NASA's Transiting Exoplanet Survey... -
Chemical abundances in 849 exoplanet hosts stars
The imprints of stellar nucleosynthesis and chemical evolution of the galaxy can be seen in different stellar populations, with older generation stars showing higher... -
GJ1132b planet/stellar radius at 0.7-4.5{mu}m
Orbiting an M dwarf 12pc away, the transiting exoplanet GJ1132b is a prime target for transmission spectroscopy. With a mass of 1.7M{Earth} and radius of 1.1R{Earth}, GJ1132b's... -
102 hot Jupiters isochrone analyse & stellar modeling
It has been shown that hot Jupiters systems with massive, hot stellar primaries exhibit a wide range of stellar obliquities. On the other hand, hot Jupiter systems with... -
IR light curve of VHS1256-1257b in 2018 & 2020 epochs
The photometric and spectral variability of brown dwarfs probes heterogeneous temperature and cloud distributions and traces the atmospheric circulation patterns. We present a...
