In this work, we keep pushing K2 data to a high photometric precision, close to that of the
Kepler main mission, using a point-spread function (PSF)-based, neighbour-subtraction …

In the third paper of this series we continue the exploitation of Kepler/K2 data in dense
stellar fields using our PSF-based method. This work is focused on a∼ 720-arcmin2 region …

Kepler and K2 data analysis reported in the literature is mostly based on aperture
photometry. Because of Kepler's large, undersampled pixels and the presence of nearby …

We present a multiyear survey aimed at collecting (1) high-precision (∼ 5 milli-mag),(2) fast-
cadence (∼ 3 min), and (3) relatively long duration (∼ 10 d) multiband photometric series …

In this paper, we continue the release of high-level data products from the multiyear
photometric survey collected at the 67/92 cm Schmidt Telescope in Asiago. The primary goal …

We present results from spectroscopic follow-up observations of stars identified in the Kepler
field and carried out by teams of the Kepler Follow-up Observation Program. Two samples of …

High-precision time series photometry with the Kepler satellite has been crucial to our
understanding both of exoplanets, and via asteroseismology, of stellar physics. After the …

ABSTRACT KIC 1571511 is a 14-d eclipsing binary (EB) in the Kepler data set. The
secondary of this EB is a very low mass star with a mass of and a radius of (statistical errors …

While hundreds of planets have been discovered around field stars, only a few are known in
star clusters. To explain the lack of short-period giant planets in globular clusters (GCs) …

Aims. We present first results of our efforts to re-analyze the Kepler photometric dataset,
searching for planetary transits using an alternative processing pipeline to the one used by …