Solar active region components show reduced darkening toward the limb compared to the quiet Sun, with faculae and network contrasts peaking near mu=0.3 at ~4% and ~2% excess, unlike PHOENIX and ATLAS model predictions.
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7 Pith papers cite this work. Polarity classification is still indexing.
7
Pith papers citing it
representative citing papers
Three new candidate ancient planetary nebulae, each several arcminutes across with extremely low [O iii] surface brightness around 30 mag arcsec^{-2}, were discovered using amateur telescopes, with candidate central stars yielding age estimates of 50-100 thousand years.
JWST transits of TOI 700 d and e yield no exomoons, refined ephemerides, and identify 16-minute correlated noise that currently blocks Luna-analog moon detection.
VLBA observations of Orion young stellar binaries yield Keplerian orbits and dynamical masses for four systems, with two showing agreement to SED-based estimates and one confirming an intermediate-mass star with nonthermal emission.
A JWST MIRI LRS eclipse of HD 3167 b is 38±11 ppm, >5σ below a dark bare-rock prediction, implying an atmosphere on this ultra-short-period super-Earth.
Neural network derives LAMOST instrumental profiles from arc lamps and reduces RV dispersion by ~3 km/s.
Derives Teff, log g and metallicity for 282 M dwarfs via χ² fits of updated PHOENIX models to simultaneous visible+NIR CARMENES spectra, finding visible and combined ranges superior to NIR alone.
citing papers explorer
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Center-to-limb variations of solar active regions: Observations of spots, faculae, and network in the 6173 \AA\ continuum
Solar active region components show reduced darkening toward the limb compared to the quiet Sun, with faculae and network contrasts peaking near mu=0.3 at ~4% and ~2% excess, unlike PHOENIX and ATLAS model predictions.
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Ancient 'ghost' planetary nebulae discovered with amateur telescopes
Three new candidate ancient planetary nebulae, each several arcminutes across with extremely low [O iii] surface brightness around 30 mag arcsec^{-2}, were discovered using amateur telescopes, with candidate central stars yielding age estimates of 50-100 thousand years.
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The JWST Search for Earth-Luna Analogs: Upper Limits on Exomoons and Refined Ephemerides for TOI 700 d and e
JWST transits of TOI 700 d and e yield no exomoons, refined ephemerides, and identify 16-minute correlated noise that currently blocks Luna-analog moon detection.
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Dynamical masses of young stellar objects with the VLBA: DYNAMO-VLBA: Radio binary stars in Orion
VLBA observations of Orion young stellar binaries yield Keplerian orbits and dynamical masses for four systems, with two showing agreement to SED-based estimates and one confirming an intermediate-mass star with nonthermal emission.
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Evidence for an Atmosphere on the Ultra-Short Period super-Earth HD 3167 b
A JWST MIRI LRS eclipse of HD 3167 b is 38±11 ppm, >5σ below a dark bare-rock prediction, implying an atmosphere on this ultra-short-period super-Earth.
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Characterizing the Instrumental Profile of LAMOST
Neural network derives LAMOST instrumental profiles from arc lamps and reduces RV dispersion by ~3 km/s.
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The CARMENES search for exoplanets around M dwarfs -- Photospheric parameters of target stars from high-resolution spectroscopy. II. Simultaneous multiwavelength range modeling of activity insensitive lines
Derives Teff, log g and metallicity for 282 M dwarfs via χ² fits of updated PHOENIX models to simultaneous visible+NIR CARMENES spectra, finding visible and combined ranges superior to NIR alone.