Four infrared-selected young stellar objects are confirmed as FUor eruptions via CO and H2O absorption features, equivalent width diagrams, and disk models showing high extinction and accretion rates comparable to classical FUors.
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7 Pith papers cite this work. Polarity classification is still indexing.
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Planar very metal-poor stars exhibit chemical homogeneity and dwarf-galaxy-like abundance ratios, supporting origin from one ancient accreted system tentatively called Loki.
Combined TESS-CHEOPS data on 5620 flares shows ED-based FFDs follow power laws but bolometric-energy FFDs are best described by a truncated power law with break at 1.8e35 erg, with low-energy flattening attributed to detection biases rather than intrinsic lognormal behavior.
AnomalyMatch applied to JWST data identified 58 gravitational lenses, 37 new, graded by experts and spanning redshifts to zphot ~2.1.
Observations show a slight rise in stripped-envelope supernovae relative to hydrogen-rich ones at higher metallicities, with binary-interaction or rotation models able to match the trends though no unique scenario fits best.
Three new warm Jupiters (periods 11.3–44.4 days, masses 0.51–1.29 M_J, radii ~0.97–0.98 R_J) were confirmed via TESS photometry and follow-up radial velocities and light curves.
Uniform atmospheric parameters (Teff, log g, [Fe/H]) derived for 616 XSL stars via ULySS fitting to MILES, with reported precisions of 0.9-2.6% in Teff depending on stellar type.
citing papers explorer
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Characterizing and spectrally modeling embedded FUor eruptions in the near-infrared
Four infrared-selected young stellar objects are confirmed as FUor eruptions via CO and H2O absorption features, equivalent width diagrams, and disk models showing high extinction and accretion rates comparable to classical FUors.
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Extending TESS flare frequency distributions with CHEOPS: Power-law versus lognormal
Combined TESS-CHEOPS data on 5620 flares shows ED-based FFDs follow power laws but bolometric-energy FFDs are best described by a truncated power law with break at 1.8e35 erg, with low-energy flattening attributed to detection biases rather than intrinsic lognormal behavior.
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Stellar atmospheric parameters for 754 spectra from the X-shooter Spectral Library
Uniform atmospheric parameters (Teff, log g, [Fe/H]) derived for 616 XSL stars via ULySS fitting to MILES, with reported precisions of 0.9-2.6% in Teff depending on stellar type.