activity
20092019
most citedThe GAPS Programme with HARPS-N@TNG V. A comprehensive analysis of the XO-2 stellar and planetary systems

59 citations · 138 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2019★ 14 cited

Photometric rotation periods for 107 M dwarfs from the APACHE survey

P. Giacobbe, M. Benedetto, M. Damasso +13

We present rotation period measurements for 107 M dwarfs in the mass range observed within the context of the APACHE photometric survey. We measure rotation per…

astro-ph.SR2015

New Variable Stars Discovered by the APACHE Survey. II. Results After the Second Observing Season

M. Damasso, L. Gioannini, A. Bernagozzi +9

Routinely operating since July 2012, the APACHE survey has celebrated its second birthday. While the main goal of the Project is the detection of transiting planets around a large…

astro-ph.SR2015★ 59 cited

The GAPS Programme with HARPS-N@TNG V. A comprehensive analysis of the XO-2 stellar and planetary systems

M. Damasso, K. Biazzo, A. S. Bonomo +56

XO-2 is the first confirmed wide stellar binary system where the almost twin components XO-2N and XO-2S have planets. This stimulated a detailed characterization study of the stell…

astro-ph.SR2014

New Variable Stars Discovered by the APACHE Survey. I. Results After the First Observing Season

M. Damasso, A. Bernagozzi, E. Bertolini +9

We present more than 80 new variable stars discovered during the first observing season of the APACHE survey. APACHE is a project aimed at detecting extrasolar planets transiting n…

astro-ph.EP2013★ 28 cited

The APACHE Project

A. Sozzetti, A. Bernagozzi, E. Bertolini +9

First, we summarize the four-year long efforts undertaken to build the final setup of the APACHE Project, a photometric transit search for small-size planets orbiting bright, low-m…

astro-ph.EP2012★ 26 cited

Photometric transit search for planets around cool stars from the western Italian Alps: A pilot study

P. Giacobbe, M. Damasso, A. Sozzetti +7

[ABRIDGED] In this study, we set out to a) demonstrate the sensitivity to <4 R_E transiting planets with periods of a few days around our program stars, and b) improve our knowledg…