Search Results - "Winn, Joshua N."
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Homogeneous Analysis of Hot Earths: Masses, Sizes, and Compositions
Published in The Astrophysical journal (20-09-2019)“…Terrestrial planets have been found orbiting Sun-like stars with extremely short periods-some as short as 4 hr. These "ultra-short-period planets" or "hot…”
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ARE TIDAL EFFECTS RESPONSIBLE FOR EXOPLANETARY SPIN-ORBIT ALIGNMENT?
Published in The Astrophysical journal (10-02-2016)“…ABSTRACT The obliquities of planet-hosting stars are clues about the formation of planetary systems. Previous observations led to the hypothesis that for…”
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3
EVIDENCE FOR THE TIDAL DESTRUCTION OF HOT JUPITERS BY SUBGIANT STARS
Published in The Astrophysical journal (01-08-2013)“…Tidal transfer of angular momentum is expected to cause hot Jupiters to spiral into their host stars. Although the timescale for orbital decay is very…”
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4
The Six-planet Resonant Chain of HD 110067
Published in Astrophysical journal. Letters (01-06-2024)“…HD 110067 is the brightest star known to have six transiting planets. Each adjacent pair of planets has a period ratio that is nearly equal to a ratio of small…”
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AESTRA: Deep Learning for Precise Radial Velocity Estimation in the Presence of Stellar Activity
Published in The Astronomical journal (01-01-2024)“…Abstract Stellar activity interferes with precise radial velocity measurements and limits our ability to detect and characterize planets, in particular…”
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THE TRANSITING EXOPLANET SURVEY SATELLITE: SIMULATIONS OF PLANET DETECTIONS AND ASTROPHYSICAL FALSE POSITIVES
Published in The Astrophysical journal (10-08-2015)“…ABSTRACT The Transiting Exoplanet Survey Satellite (TESS) is a NASA-sponsored Explorer mission that will perform a wide-field survey for planets that transit…”
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The California-Kepler Survey. X. The Radius Gap as a Function of Stellar Mass, Metallicity, and Age
Published in The Astronomical journal (01-04-2022)“…Abstract In 2017, the California-Kepler Survey (CKS) published its first data release (DR1) of high-resolution optical spectra of 1305 planet hosts. Refined…”
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On a Possible Solution to the Tidal Realignment Problem for Hot Jupiters
Published in The Astrophysical journal (10-06-2021)“…Hot stars with hot Jupiters have a wide range of obliquities, while cool stars with hot Jupiters tend to have low obliquities. An enticing explanation for this…”
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Ponderings on the Possible Preponderance of Perpendicular Planets
Published in Astrophysical journal. Letters (01-06-2023)“…Abstract Misalignments between planetary orbits and the equatorial planes of their host stars are clues about the formation and evolution of planetary systems…”
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ORBITAL CIRCULARIZATION OF HOT AND COOL KEPLER ECLIPSING BINARIES
Published in The Astrophysical journal (10-06-2016)“…ABSTRACT The rate of tidal circularization is predicted to be faster for relatively cool stars with convective outer layers, compared to hotter stars with…”
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Occurrence Rate of Hot Jupiters Around Early-type M Dwarfs Based on Transiting Exoplanet Survey Satellite Data
Published in The Astronomical journal (01-01-2023)“…Abstract We present an estimate of the occurrence rate of hot Jupiters (7 R ⊕ ≤ R p ≤ 2 R J , 0.8 ≤ P b ≤ 10 days) around early-type M dwarfs based on stars…”
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IMPROVED SPECTROSCOPIC PARAMETERS FOR TRANSITING PLANET HOSTS
Published in The Astrophysical journal (01-10-2012)“…We report homogeneous spectroscopic determinations of the effective temperature, metallicity, and projected rotational velocity for the host stars of 56…”
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The Period Distribution of Hot Jupiters Is Not Dependent on Host Star Metallicity
Published in Astrophysical journal. Letters (01-06-2023)“…Abstract The probability that a Sun-like star has a close-orbiting giant planet (period ≲1 yr) increases with stellar metallicity. Previous work provided…”
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OBLIQUITIES OF HOT JUPITER HOST STARS: EVIDENCE FOR TIDAL INTERACTIONS AND PRIMORDIAL MISALIGNMENTS
Published in The Astrophysical journal (20-09-2012)“…We provide evidence that the obliquities of stars with close-in giant planets were initially nearly random, and that the low obliquities that are often…”
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15
Variability Catalog of Stars Observed during the TESS Prime Mission
Published in The Astrophysical journal. Supplement series (01-09-2023)“…Abstract During its 2 yr Prime Mission, TESS observed over 232,000 stars at a 2 minute cadence across ∼70% of the sky. These data provide a record of…”
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Further Evidence for Tidal Spin-up of Hot Jupiter Host Stars
Published in The Astrophysical journal (01-10-2021)“…Abstract For most hot Jupiters around main-sequence Sun-like stars, tidal torques are expected to transfer angular momentum from the planet’s orbit to the…”
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The Featureless Transmission Spectra of Two Super-puff Planets
Published in The Astrophysical journal (01-02-2020)“…The Kepler mission revealed a class of planets known as "super-puffs," with masses only a few times larger than Earth's but radii larger than Neptune, giving…”
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Stellar Spin-Orbit Misalignment in a Multiplanet System
Published in Science (American Association for the Advancement of Science) (18-10-2013)“…Stars hosting hot Jupiters are often observed to have high obliquities, whereas stars with multiple coplanar planets have been seen to have low obliquities…”
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A rocky composition for an Earth-sized exoplanet
Published in Nature (London) (21-11-2013)“…Doppler spectroscopic measurements of the mass of the Earth-sized planet Kepler-78b reveal that its mean density is similar to Earth’s, suggesting a…”
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The Warm Neptune GJ 3470b Has a Polar Orbit
Published in Astrophysical journal. Letters (01-06-2022)“…The warm Neptune GJ 3470b transits a nearby (d = 29 pc) bright slowly rotating M1.5-dwarf star. Using spectroscopic observations during two transits with the…”
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