… clusters’ (PATHOS; Nardiello et al. 2019, hereafter Paper I), aimed at the extraction of
high-precision light curves for stars in stellar clusters (open and globular clusters) and young …

… the PSF-based approach to TESS data, in order to extract high-precision light curves of
sources in a very crowded field centred on the globular cluster NGC 104 (47 Tuc). In Section 2, …

… TESS data collected during Cycle 2 (Sectors 14–26) to obtain high-precision light curves of
cluster … cutting-edge tools (Section 2), find and characterize candidate exoplanets in stellar …

… PATHOS pipeline is used to extract and correct the TESS light curves of a sample of likely
young association members (Section 2… the procedure I followed to search and characterize the …

… clusters (PATHOS) only provide a subset of TESS data (… fields, we find that the weighted
average of the two versions of … ≲2% photometric precision for a 16th TESS magnitude star; TOI …

… the NASA TESS data along with ESA Gaia data to search for … N77-135 from TESS FFI
using tessipack, PATHOS and QLP. (… of the star to ensure that we know where the stellar light …

… rotational properties of the star. We find that TOI 451 is a young solar-mass star and has a
comoving … , abundances, stellar rotation, and activity. We model the planetary transits seen by …

… The PSF-based technique reduces dilution effects in … In this work, we have presented the
LCs of PATHOS data release. We … we did not find any signatures of variability using TESS data. …

… curves from A PSF-based Approach to TESS High Quality Data of Stellar Clusters (PATHOS; …
In the two clusters with literature data for F–G stars, we find few discrepancies between our …

… targeted detrending approach in young exoplanet searches by using information about the
… One of the additional benefits of the unsupervised clustering method used by the SOM is the …