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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UNVERDICTED 4representative citing papers
A new 3D dust reddening map with finer distance resolution, a spatial correlation prior, and Gaia-based distances covering the sky north of -30 degrees declination out to several kiloparsecs.
Alpha-element distributions in Fornax, Sextans, Draco, and Carina correlate with galaxy luminosity while nitrogen-rich stars in Fornax suggest destroyed globular cluster relics.
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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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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A 3D Dust Map Based on Gaia, Pan-STARRS 1 and 2MASS
A new 3D dust reddening map with finer distance resolution, a spatial correlation prior, and Gaia-based distances covering the sky north of -30 degrees declination out to several kiloparsecs.
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APOGEE chemical abundances of stars in the MW satellites Fornax, Sextans, Draco and Carina
Alpha-element distributions in Fornax, Sextans, Draco, and Carina correlate with galaxy luminosity while nitrogen-rich stars in Fornax suggest destroyed globular cluster relics.
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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.