Search Results - "Haywood, Raphaelle D."
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DETERMINING THE MASS OF KEPLER-78b WITH NONPARAMETRIC GAUSSIAN PROCESS ESTIMATION
Published in The Astrophysical journal (01-08-2015)“…ABSTRACT Kepler-78b is a transiting planet that is 1.2 times the radius of Earth and orbits a young, active K dwarf every 8 hr. The mass of Kepler-78b has been…”
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A temperate rocky super-Earth transiting a nearby cool star
Published in Nature (London) (20-04-2017)“…An Earth-sized planet is observed orbiting a nearby star within the liquid-water, habitable zone, the atmospheric composition of which could be determined from…”
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Characterizing Solar Center-to-limb Radial-velocity Variability with SDO
Published in The Astrophysical journal (01-09-2024)“…Abstract Stellar photospheric inhomogeneities are a significant source of noise, which currently precludes the discovery of Earth-mass planets orbiting…”
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The effect of stellar activity on the spectroscopic stellar parameters of the young solar twin HIP 36515
Published in Monthly notices of the Royal Astronomical Society. Letters (01-11-2019)“…ABSTRACT Spectroscopic equilibrium allows us to obtain precise stellar parameters in Sun-like stars. It relies on the assumption of the iron excitation and…”
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An Earth-sized planet with an Earth-like density
Published in Nature (London) (21-11-2013)“…Data from the Kepler spacecraft and the HARPS-N ground-based spectrograph indicate that the extrasolar planet Kepler-78b has a mean density similar to that of…”
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Leveraging Space-based Data from the Nearest Solar-type Star to Better Understand Stellar Activity Signatures in Radial Velocity Data
Published in The Astronomical journal (01-06-2022)“…Abstract Stellar variability is a key obstacle in reaching the sensitivity required to recover Earth-like exoplanetary signals using the radial velocity (RV)…”
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THE KEPLER-10 PLANETARY SYSTEM REVISITED BY HARPS-N: A HOT ROCKY WORLD AND A SOLID NEPTUNE-MASS PLANET
Published in The Astrophysical journal (10-07-2014)“…Kepler-10b was the first rocky planet detected by the Kepler satellite and confirmed with radial velocity follow-up observations from Keck-HIRES. The mass of…”
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Identifying Exoplanets with Deep Learning. IV. Removing Stellar Activity Signals from Radial Velocity Measurements Using Neural Networks
Published in The Astronomical journal (01-08-2022)“…Abstract Exoplanet detection with precise radial velocity (RV) observations is currently limited by spurious RV signals introduced by stellar activity. We show…”
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The magnetically quiet solar surface dominates HARPS-N solar RVs during low activity
Published in Monthly notices of the Royal Astronomical Society (01-01-2024)“…ABSTRACT Using images from the Helioseismic and Magnetic Imager aboard the Solar Dynamics Observatory, we extract the radial velocity (RV) signal arising from…”
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Masses, revised radii, and a third planet candidate in the ‘Inverted’ planetary system around TOI-1266
Published in Monthly notices of the Royal Astronomical Society (01-01-2024)“…ABSTRACT Is the population of close-in planets orbiting M dwarfs sculpted by thermally driven escape or is it a direct outcome of the planet formation process?…”
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Using HARPS-N to characterize the long-period planets in the PH-2 and Kepler-103 systems
Published in Monthly notices of the Royal Astronomical Society (01-12-2019)“…ABSTRACT We present confirmation of the planetary nature of PH-2b, as well as the first mass estimates for the two planets in the Kepler-103 system. PH-2b and…”
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Sensitivity of low-degree solar p modes to active and ephemeral regions: frequency shifts back to the Maunder minimum
Published in Monthly notices of the Royal Astronomical Society. Letters (01-10-2019)“…ABSTRACT We explore the sensitivity of the frequencies of low-degree solar p modes to near-surface magnetic flux on different spatial scales and strengths,…”
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ESD Ideas: Exoplanet, origins of life and biosphere researchers offer a perspective fundamental to ensuring humanity's future
Published in Earth system dynamics (25-07-2024)“…Studying the origin of life and its prevalence in the universe offers a perspective that compels us to look after our irreplaceable home in the cosmos. An…”
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A Kepler study of starspot lifetimes with respect to light-curve amplitude and spectral type
Published in Monthly notices of the Royal Astronomical Society (01-12-2017)“…Abstract Wide-field high-precision photometric surveys such as Kepler have produced reams of data suitable for investigating stellar magnetic activity of…”
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THE MASS OF Kepler-93b AND THE COMPOSITION OF TERRESTRIAL PLANETS
Published in The Astrophysical journal (20-02-2015)“…Kepler-93b is a 1.478 ± 0.019 R {sub ⊕} planet with a 4.7 day period around a bright (V = 10.2), astroseismically characterized host star with a mass of 0.911…”
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TOI-1695 b: A Water World Orbiting an Early-M Dwarf in the Planet Radius Valley
Published in The Astronomical journal (01-04-2023)“…Abstract Characterizing the bulk compositions of transiting exoplanets within the M dwarf radius valley offers a unique means to establish whether the radius…”
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The hot Jupiter of the magnetically active weak-line T Tauri star V830 Tau
Published in Monthly notices of the Royal Astronomical Society (01-03-2017)“…We report results of an extended spectropolarimetric and photometric monitoring of the weak-line T Tauri star V830 Tau and its recently detected newborn…”
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Leveraging space-based data from the nearest Solar-type star to better understand stellar activity signatures in radial velocity data
Published 19-04-2022“…Stellar variability is a key obstacle in reaching the sensitivity required to recover Earth-like exoplanetary signals using the radial velocity (RV) detection…”
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Using HARPS-N to characterise the long-period planets in the PH-2 and Kepler-103 systems
Published 08-10-2019“…We present confirmation of the planetary nature of PH-2b, as well as the first mass estimates for the two planets in the Kepler-103 system. PH-2b and…”
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Characterizing Solar Center-to-Limb Radial-Velocity Variability with SDO
Published 25-04-2024“…Stellar photospheric inhomogeneities are a significant source of noise which currently precludes the discovery of Earth-mass planets orbiting Sun-like stars…”
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