Zobrazeno 1 - 10
of 678
pro vyhledávání: '"Bertolini E."'
Autor:
Lattanzi M.G., Lanteri L., Damasso M., Giacobbe P., Cenadelli D., Carbognani A., Calcidese P., Bertolini E., Bernagozzi A., Christille Jean-Marc, Sozzetti A., Smart R.
Publikováno v:
EPJ Web of Conferences, Vol 47, p 17001 (2013)
Small-size ground-based telescopes can effectively be used to look for transiting rocky planets around nearby low-mass M stars using the photometric transit method, as recently demonstrated for example by the MEarth project. Since 2008 at the Astrono
Externí odkaz:
https://doaj.org/article/428c870097494b3baeab7e52fa82d53d
Autor:
Giacobbe P., Christille J.-M., Damasso M., Cenadelli D., Carbognani A., Calcidese P., Bertolini E., Bernagozzi A., Sozzetti A., Lanteri L., Lattanzi M.G., Smart R.
Publikováno v:
EPJ Web of Conferences, Vol 47, p 03006 (2013)
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-mass M dwarfs. Next, we describe the present status of the APACHE surve
Externí odkaz:
https://doaj.org/article/12c329f7e54b46d8a908f1d29e2d5267
Autor:
Giacobbe, P., Benedetto, M., Damasso, M., Sozzetti, A., Christille, J. M., Lattanzi, M. G., Calcidese, P., Carbognani, A., Barbato, D., Pinamonti, M., Poggio, E., Lanza, A. F., Bernagozzi, A., Cenadelli, D., Lanteri, L., Bertolini, E.
We present rotation period measurements for 107 M dwarfs in the mass range $0.15-0.70 M_\odot$ observed within the context of the APACHE photometric survey. We measure rotation periods in the range 0.5-190 days, with the distribution peaking at $\sim
Externí odkaz:
http://arxiv.org/abs/1911.13113
Autor:
Damasso, M., Gioannini, L., Bernagozzi, A., Bertolini, E., Calcidese, P., Carbognani, A., Cenadelli, D., Christille, J. M., Giacobbe, P., Lanteri, L., Smart, M. G. Lattanzi. R., Sozzetti, A.
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 sample of bright, nearby M dwarfs in the northern hemisphere, the APAC
Externí odkaz:
http://arxiv.org/abs/1502.03651
Autor:
Damasso, M., Biazzo, K., Bonomo, A. S., Desidera, S., Lanza, A. F., Nascimbeni, V., Esposito, M., Scandariato, G., Sozzetti, A., Cosentino, R., Gratton, R., Malavolta, L., Rainer, M., Gandolfi, D., Poretti, E., Sanchez, R. Zanmar, Ribas, I., Santos, N., Affer, L., Andreuzzi, G., Barbieri, M., Bedin, L. R., Benatti, S., Bernagozzi, A., Bertolini, E., Bonavita, M., Borsa, F., Borsato, L., Boschin, W., Calcidese, P., Carbognani, A., Cenadelli, D., Christille, J. M., Claudi, R. U., Covino, E., Cunial, A., Giacobbe, P., Granata, V., Harutyunyan, A., Lattanzi, M. G., Leto, G., Libralato, M., Lodato, G., Lorenzi, V., Mancini, L., Fiorenzano, A. F. Martinez, Marzari, F., Masiero, S., Micela, G., Molinari, E., Molinaro, M., Munari, U., Murabito, S., Pagano, I., Pedani, M., Piotto, G., Rosenberg, A., Silvotti, R., Southworth, J.
Publikováno v:
A&A 575, A111 (2015)
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 stellar and planetary components based on new observations. We collected hi
Externí odkaz:
http://arxiv.org/abs/1501.01424
Autor:
Damasso, M., Bernagozzi, A., Bertolini, E., Calcidese, P., Carbognani, A., Cenadelli, D., Christille, J-M, Giacobbe, P., Lanteri, L., Lattanzi, M. G., Smart, R., Sozzetti, A.
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.
Externí odkaz:
http://arxiv.org/abs/1406.3260
Autor:
Sozzetti, A., Bernagozzi, A., Bertolini, E., Calcidese, P., Carbognani, A., Cenadelli, D., Christille, J. M., Damasso, M., Giacobbe, P., Lanteri, L., Lattanzi, M. G., Smart, R.
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-mass M dwarfs. Next, we describe the present status of the APACHE surve
Externí odkaz:
http://arxiv.org/abs/1303.1275
Autor:
Giacobbe, P., Damasso, M., Sozzetti, A., Toso, G., Perdoncin, M., Calcidese, P., Bernagozzi, A., Bertolini, E., Lattanzi, M. G., Smart, R. L.
[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 knowledge of some astrophysical properties(e.g., activity, rotation) of our ta
Externí odkaz:
http://arxiv.org/abs/1206.1729
Autor:
Damasso, M., Giacobbe, P., Calcidese, P., Sozzetti, A., Lattanzi, M. G., Bernagozzi, A., Bertolini, E., Smart, R. L.
We present the results of a site characterization study carried out at the Astronomical Observatory of the Autonomous Region of the Aosta Valley (OAVdA), in the Western Italian Alps, aimed at establishing its potential to host a photometric transit s
Externí odkaz:
http://arxiv.org/abs/1007.0252
Autor:
Damasso, M., Carbognani, A., Calcidese, P., Giacobbe, P., Bernagozzi, A., Bertolini, E., Lattanzi, M. G., Smart, R., Sozzetti, A.
We report the discovery of two new short-period variable stars in the Lyra constellation, GSC2.3 N208000326 and GSC2.3 N20B000251, observed at the Astronomical Observatory of Autonomous Region of the Aosta Valley. Photometric measurements collected d
Externí odkaz:
http://arxiv.org/abs/1003.1279