Four transiting sub-Neptunes with radii measured to <1.7% precision and masses >3 sigma for three planets, plus an outer non-transiting companion, discovered around TOI-5624 via TESS, CHEOPS photometry, and ground-based RV data.
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7 Pith papers cite this work. Polarity classification is still indexing.
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FICO procedure yields average precisions of 2.3% mass, 0.82% radius, 6.9% age and 0.49% mean density for 95 solar-like stars, outperforming direct frequency fitting for stars above 1.15 solar masses or 6050 K.
Hybrid deep learning models recover large frequency separation, frequency of maximum power, and dipole period spacing from low-resolution Gaia XP spectra with accuracy comparable to moderate-resolution spectroscopy.
tPIC2.2 supplies a list of 217,741 stars for PLATO's LOPS2 field, including 202,315 FGK dwarfs/subgiants and 15,037 M dwarfs with uniformly estimated temperatures, radii, and masses.
Random forest classifiers classify Kepler targets and select analysis methods to measure surface rotation periods of solar-like stars.
Random Forest model classifies K2 stars into four categories with over 80% accuracy using effective temperature, luminosity, and FliPer features.
NSVS 10653195 is a detached eclipsing binary with two K-type stars of masses 0.6402 and 0.6511 solar masses and radii 0.687 and 0.672 solar radii, showing radius inflation relative to models.
citing papers explorer
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The multi-planet system TOI-5624: Four transiting sub-Neptunes with an outer companion revealed by transit-timing variations
Four transiting sub-Neptunes with radii measured to <1.7% precision and masses >3 sigma for three planets, plus an outer non-transiting companion, discovered around TOI-5624 via TESS, CHEOPS photometry, and ground-based RV data.
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Asteroseismic modelling of main-sequence solar-like stars and Kepler exoplanet host stars with the FICO procedure I. Catalogue of fundamental stellar properties
FICO procedure yields average precisions of 2.3% mass, 0.82% radius, 6.9% age and 0.49% mean density for 95 solar-like stars, outperforming direct frequency fitting for stars above 1.15 solar masses or 6050 K.
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Potential of Gaia XP Spectra in Red Giant Star Asteroseismology: A Deep-Learning Approach
Hybrid deep learning models recover large frequency separation, frequency of maximum power, and dipole period spacing from low-resolution Gaia XP spectra with accuracy comparable to moderate-resolution spectroscopy.
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The PLATO Input Catalogue of targets (tPIC) for the first Long Pointing Field
tPIC2.2 supplies a list of 217,741 stars for PLATO's LOPS2 field, including 202,315 FGK dwarfs/subgiants and 15,037 M dwarfs with uniformly estimated temperatures, radii, and masses.
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Determining surface rotation periods of solar-like stars observed by the Kepler mission using machine learning techniques
Random forest classifiers classify Kepler targets and select analysis methods to measure surface rotation periods of solar-like stars.
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Automatic classification of K2 pulsating stars using machine learning techniques
Random Forest model classifies K2 stars into four categories with over 80% accuracy using effective temperature, luminosity, and FliPer features.
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Absolute dimensions of the low-mass eclipsing binary system NSVS 10653195
NSVS 10653195 is a detached eclipsing binary with two K-type stars of masses 0.6402 and 0.6511 solar masses and radii 0.687 and 0.672 solar radii, showing radius inflation relative to models.