Journal: Monthly Notices of the Royal Astronomical Society
Publication
TESS asteroseismology of the Kepler red giants
Red giant asteroseismology can provide valuable information for studying the Galaxy as demonstrated by space missions like CoRoT and Kepler. However, previous...
TESS discovery of a sub-Neptune orbiting a mid-M dwarf TOI-2136
We present the discovery of TOI-2136 b, a sub-Neptune planet transiting a nearby M4.5V-type star every 7.85 d, identified through photometric measurements from...
Testing disc reprocessing models for AGN optical variability by comparison of X-ray and optical power spectra of NGC 4395
It is generally thought that active galactic nucleus (AGN) optical variability is produced, at least in part, by reprocessing of central X-rays by a surrounding...
Testing emission models on the extreme blazar 2WHSP J073326.7+515354 detected at very high energies with the MAGIC telescopes
Extreme high-energy-peaked BL Lac objects (EHBLs) are an emerging class of blazars. Their typical two-hump-structured spectral energy distribution (SED) peaks...
Testing models of stellar structure and evolution - I. Comparison with detached eclipsing binaries
We present the results of an analysis aimed at testing the accuracy and precision of the PARSEC v1.2S library of stellar evolution models, combined with a...
Testing red clump models with the asteroseismic binary KIC 10841730
Binaries in which both stars are pulsating are rare but extremely valuable. We present the first study of an asteroseismic binary system consisting of a core...
Testing the conditional mass function of dark matter haloes against numerical N-body simulations
We compare the predicted conditional mass function (CMF) of dark matter haloes from two theoretical prescriptions against numerical N-body simulations, both in...
Testing the existence of optical linear polarization in young brown dwarfs
Linear polarization can be used as a probe of the existence of atmospheric condensates in ultracool dwarfs. Models predict that the observed linear polarization...
Testing the fragmentation limit in the Upper Sco association
We present the results of a deep (J˜ 21 at 5σ) infrared photometric survey of a 0.95-deg2 area in the central region of the Upper Sco association. The...