JWST transit observations refine ephemerides of TOI 700 d and e by an order of magnitude in period precision but yield only upper limits on exomoons larger than Ganymede due to 46 ppm correlated noise attributed to stellar granulation.
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A new compact hierarchical triple main-sequence star system G1010 was discovered through combined low- and high-SNR spectroscopy, Gaia DR3 data, and TESS light curve analysis, showing an inner eclipsing binary rather than a compact object companion.
Proposes that synoptic time domain surveys can probe 10-100 times more Cosmic Haystack volume for technosignatures than traditional radio SETI by searching spatially resolved or multi-star signals over time.
MESA gains simultaneous binary star evolution, large nuclear networks, implicit hydrodynamics, and GYRE pulsation coupling for better massive star and supernova modeling.
ERA5 reanalysis yields a median seeing of 0.79 arcseconds at Timau with best conditions in March and December and higher variability in the dry season.
citing papers explorer
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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 transit observations refine ephemerides of TOI 700 d and e by an order of magnitude in period precision but yield only upper limits on exomoons larger than Ganymede due to 46 ppm correlated noise attributed to stellar granulation.
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Discovery of a compact hierarchical triple main-sequence star system while searching for binary stars with compact objects
A new compact hierarchical triple main-sequence star system G1010 was discovered through combined low- and high-SNR spectroscopy, Gaia DR3 data, and TESS light curve analysis, showing an inner eclipsing binary rather than a compact object companion.
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SETI in the Spatio-Temporal Survey Domain
Proposes that synoptic time domain surveys can probe 10-100 times more Cosmic Haystack volume for technosignatures than traditional radio SETI by searching spatially resolved or multi-star signals over time.
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Modules for Experiments in Stellar Astrophysics (MESA): Binaries, Pulsations, and Explosions
MESA gains simultaneous binary star evolution, large nuclear networks, implicit hydrodynamics, and GYRE pulsation coupling for better massive star and supernova modeling.
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Seeing at Timau National Observatory Based on ERA5 Dataset
ERA5 reanalysis yields a median seeing of 0.79 arcseconds at Timau with best conditions in March and December and higher variability in the dry season.