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 nearby, bright M dwarfs by using an array of small-aperture telescopes. Despite the fact that the survey is targeted to a well-defined sample of cool stars, we also reduce and analyze data for all the detected field stars
Here, we present the results from our analysis of 6 yr of optical photometry taken by the Siding Spr...
Variable stars are those whose brightness changes over time. Astronomers (amateurs and professionals...
Recent wide field photometric surveys, which target a specific field for long durations, are ideal f...
Routinely operating since July 2012, the APACHE survey has celebrated its second birthday. While the...
Small-size ground-based telescopes can effectively be used to look for transiting rocky planets arou...
First, we summarize the four-year long efforts undertaken to build the final setup of the APACHE Pro...
This paper follows the previous publication of new variables discovered at Astronomical Observatory,...
We report on photometric I-band observations of 147 bright (8 < I < 13) periodic variable stars towa...
This work describes the most relevant steps undertaken for the development and installation of the s...
We report the detection of 3714 variable stars towards the Galactic bulge, including 2521 previously...
We report the detection of 3714 variable stars towards the Galactic bulge, including 2521 previously...
We have undertaken a long-term project, Planets in Stellar Clusters Extensive Search (PISCES), to se...
This PhD thesis presents the analysis of a large sample of photometric data relative to the super m...
We present the results of a photometric variability survey in the young open cluster Stock 14 and th...
Abstract. We present our joint efforts to study variable stars in open clusters. This includes a new...
Here, we present the results from our analysis of 6 yr of optical photometry taken by the Siding Spr...
Variable stars are those whose brightness changes over time. Astronomers (amateurs and professionals...
Recent wide field photometric surveys, which target a specific field for long durations, are ideal f...
Routinely operating since July 2012, the APACHE survey has celebrated its second birthday. While the...
Small-size ground-based telescopes can effectively be used to look for transiting rocky planets arou...
First, we summarize the four-year long efforts undertaken to build the final setup of the APACHE Pro...
This paper follows the previous publication of new variables discovered at Astronomical Observatory,...
We report on photometric I-band observations of 147 bright (8 < I < 13) periodic variable stars towa...
This work describes the most relevant steps undertaken for the development and installation of the s...
We report the detection of 3714 variable stars towards the Galactic bulge, including 2521 previously...
We report the detection of 3714 variable stars towards the Galactic bulge, including 2521 previously...
We have undertaken a long-term project, Planets in Stellar Clusters Extensive Search (PISCES), to se...
This PhD thesis presents the analysis of a large sample of photometric data relative to the super m...
We present the results of a photometric variability survey in the young open cluster Stock 14 and th...
Abstract. We present our joint efforts to study variable stars in open clusters. This includes a new...
Here, we present the results from our analysis of 6 yr of optical photometry taken by the Siding Spr...
Variable stars are those whose brightness changes over time. Astronomers (amateurs and professionals...
Recent wide field photometric surveys, which target a specific field for long durations, are ideal f...