ABSTRACT As the James Webb Space Telescope (JWST) has become fully operational,
early release data are now available to begin building the tools and calibrations for …

We present k2sc (K2 Systematics Correction), a python pipeline to model instrumental
systematics and astrophysical variability in light curves from the K2 mission. k2sc uses …

We present an update to the EVEREST K2 pipeline that addresses various limitations in the
previous version and improves the photometric precision of the light curves. We develop a …

In the third paper of this series aimed at developing the tools for analysing resolved stellar
populations using the cameras on board of the James Webb Space Telescope (JWST), we …

Aims. Our scientific goal is to provide revised membership lists of the α Per, Pleiades, and
Praesepe clusters exploiting the second data release of Gaia and produce five-dimensional …

The TESS mission will survey∼ 85 per cent of the sky, giving us the opportunity of extracting
high-precision light curves of millions of stars, including stellar cluster members. In this work …

The most powerful tests of stellar models come from the brightest stars in the sky, for which
complementary techniques, such as astrometry, asteroseismology, spectroscopy and …

Photometry from the Kepler mission is optimized to detect small, short-duration signals like
planet transits at the expense of long-term trends. This long-term variability can be …

The scope of the project 'A PSF-based Approach to TESS High Quality data Of Stellar
clusters'(PATHOS) is the extraction and analysis of high-precision light curves of stars in …

Abstract The Transiting Exoplanet Survey Satellite (TESS) is providing precise time-series
photometry for most star clusters in the solar neighborhood. Using the TESS images, we …