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Hydrodynamic simulations of cool stellar atmospheres with MANCHA |
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Solid state debromination of C 60 Br 24 back to C 60 with cesium iodide: kinetics, thermodynamics and mechanism |
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Green, solventless debromination of C 70 Br 10 to C 70 with CsI |
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Revisiting the warm sub-Saturn TOI-1710b. The impact of stellar activity on the mass measurement |
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Cool and data-driven: an exploration of optical cool dwarf chemistry with both data-driven and physical models |
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Evaluation of a Magnetic Field Inversion Method Using Only Stokes I |
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TOI-5126: a hot super-Neptune and warm Neptune pair discovered by TESS and CHEOPS |
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Black hole masses for 14 gravitationally lensed quasars |
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Workshop Summary: Exoplanet Orbits and Dynamics |
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Thermochemical properties of C60Br24 |
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joshspeagle/dynesty: v2.1.2 |
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OGLE-2019-BLG-0825: Constraints on the Source System and Effect on Binary-lens Parameters Arising from a Five-day Xallarap Effect in a Candidate Planetary Microlensing Event |
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An eclipsing 47 min double white dwarf binary at 400 pc |
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Everything that glitters is not gold: V1315 Cas is not a dormant black hole |
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Dynamical mass of the white dwarf in XY Ari: a test for intermediate polar X-ray spectral models |
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A Blueprint for the Milky Way's Stellar Populations. IV. A String of Pearls-the Galactic Starburst Sequence |
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KMT-2021-BLG-1150Lb: Microlensing planet detected through a densely covered planetary-caustic signal |
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Gaia colour-magnitude diagrams of young open clusters. Identification in the UBC catalogue and comparison between manual and automated analyses |
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Pyodine: an open, flexible reduction software for iodine-calibrated precise radial velocities |
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BAWLAS: a Catalog of Chemical abundances for Weak and Blended Elements in APOGEE Spectra |
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Evidence of a flare ignited above a low-latitude spotted active region in the ultrafast rotator HK Aqr |
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Four sub-Jovian-mass planets detected by high-cadence microlensing surveys |
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Photometric and spectroscopic study of the burst-like brightening of two Gaia-alerted young stellar objects |
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The relic galaxy NGC 1277 rules out intermediate-age stellar populations origin of CO-strong absorptions in massive early-type galaxies |
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