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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3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
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2026 3representative citing papers
Asteroseismic ages from TESS calibrate [Y/Mg] and [C/N] chemical clocks, revealing a radially dependent [Y/Mg]-age relation that is steeper in the outer Galactic disc and flatter inward, with NLTE corrections and evolutionary stage accounting required for accuracy.
Asteroseismic characterisation of 32 bright stars in PLATO LOP fields using TESS data yields mode parameters for 26 stars extracted for the first time, with comparisons across three pipelines.
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 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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Calibration of the [C/N] and [Y/Mg] chemical clocks with asteroseismic ages from the TESS space mission
Asteroseismic ages from TESS calibrate [Y/Mg] and [C/N] chemical clocks, revealing a radially dependent [Y/Mg]-age relation that is steeper in the outer Galactic disc and flatter inward, with NLTE corrections and evolutionary stage accounting required for accuracy.
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Luminaries in the Sky: The TESS LEGACY Sample of Bright Stars. II. In-depth seismic characterisation of 32 naked-eye stars in the PLATO LOP fields
Asteroseismic characterisation of 32 bright stars in PLATO LOP fields using TESS data yields mode parameters for 26 stars extracted for the first time, with comparisons across three pipelines.