Zobrazeno 1 - 10
of 69
pro vyhledávání: '"Falcini, G."'
Autor:
Guilluy, G., Andretta, V., Borsa, F., Giacobbe, P., Sozzetti, A., Covino, E., Bourrier, V., Fossati, L., Bonomo, A. S., Esposito, M., Giampapa, M. S., Harutyunyan, A., Rainer, M., Brogi, M., Bruno, G., Claudi, R., Frustagli, G., Lanza, A. F., Mancini, L., Pino, L., Poretti, E., Scandariato, G., Affer, L., Baffa, C., Baruffolo, A., Benatti, S., Biazzo, K., Bignamini, A., Boschin, W., Carleo, I., Cecconi, M., Cosentino, R., Damasso, M., Desidera, M., Falcini, G., Fiorenzano, A. F. Martinez, Ghedina, A., González-Álvarez, E., Guerra, J., Hernandez, N., Leto, G., Maggio, A., Malavolta, L., Maldonado, J., Micela, G., Molinari, E., Nascimbeni, V., Pagano, I., Pedani, M., Piotto, G., Reiners, A.
Publikováno v:
A&A 639, A49 (2020)
Exoplanets orbiting very close to their host star are strongly irradiated. This can lead the upper atmospheric layers to expand and evaporate into space. The metastable helium (HeI) triplet at 1083.3nm has recently been shown to be a powerful diagnos
Externí odkaz:
http://arxiv.org/abs/2005.05676
Autor:
Carleo, I., Malavolta, L., Lanza, A. F., Damasso, M., Desidera, S., Borsa, F., Mallonn, M., Pinamonti, M., Gratton, R., Alei, E., Benatti, S., Mancini, L., Maldonado, J., Biazzo, K., Esposito, M., Frustagli, G., González-Álvarez, E., Micela, G., Scandariato, G., Sozzetti, A., Affer, L., Bignamini, A., Bonomo, A. S., Claudi, R., Cosentino, R., Covino, E., Fiorenzano, A. F. M., Giacobbe, P., Harutyunyan, A., Leto, G., Maggio, A., Molinari, E., Nascimbeni, V., Pagano, I., Pedani, M., Piotto, G., Poretti, E., Rainer, M., Redfield, S., Baffa, C., Baruffolo, A., Buchschacher, N., Billotti, V., Cecconi, M., Falcini, G., Fantinel, D., Fini, L., Galli, A., Ghedina, A., Ghinassi, F., Giani, E., Gonzalez, C., Gonzalez, M., Guerra, J., Diaz, M. Hernandez, Hernandez, N., Iuzzolino, M., Lodi, M., Oliva, E., Origlia, L., Ventura, H. Perez, Puglisi, A., Riverol, C., Riverol, L., Juan, J. San, Sanna, N., Scuderi, S., Seemann, U., Sozzi, M., Tozzi, A.
Publikováno v:
A&A 638, A5 (2020)
The existence of hot Jupiters is still not well understood. Two main channels are thought to be responsible for their current location: a smooth planet migration through the proto-planetary disk or the circularization of an initial high eccentric orb
Externí odkaz:
http://arxiv.org/abs/2002.10562
Autor:
Claudi, R., Benatti, S., Carleo, I., Ghedina, A., Guerra, J., Ghinassi, F., Harutyunyan, A., Micela, G., Molinari, E., Oliva, E., Rainer, M., Tozzi, A., Baffa, C., Baruffolo, A., Biliotti, V., Buchschacher, N., Cecconi, M., Cosentino, R., Falcini, G., Fantinel, D., Fini, L., Giani, E., Gonzalez--Alvarez, E., Gonzalez, M., Gonzalez, C., Gratton, R., Hernandez, N., Iuzzolino, M., Lodi, M., Malavolta, L., Maldonado, J., Origlia, L., Puglisi, A., Sanna, N., Juan, J. San, Scuderi, S., Seemann, U., Sozzetti, A., Sozzi, M., Ventura, H. Perez, Diaz, M. Hernandez, Galli, A., Riverol, L., Riverol, C.
GIARPS (GIAno \& haRPS) is a project devoted to have on the same focal station of the Telescopio Nazionale Galileo (TNG) both high resolution spectrographs, HARPS-N (VIS) and GIANO-B (NIR), working simultaneously. This could be considered the first a
Externí odkaz:
http://arxiv.org/abs/1808.03184
Autor:
Carleo, I., Benatti, S., Lanza, A. F., Gratton, R., Claudi, R., Desidera, S., Mace, G. N., Messina, S., Sanna, N., Sissa, E., Ghedina, A., Ghinassi, F., Guerra, J., Harutyunyan, A., Micela, G., Molinari, E., Oliva, E., Tozzi, A., Baffa, C., Baruffolo, A., Bignamini, A., Buchschacher, N., Cecconi, M., Cosentino, R., Endl, M., Falcini, G., Fantinel, D., Fini, L., Fugazza, D., Galli, A., Giani, E., González, C., González-Álvarez, E., González, M., Hernandez, N., Diaz, M. Hernandez, Iuzzolino, M., Kaplan, K. F., Kidder, B. T., Lodi, M., Malavolta, L., Maldonado, J., Origlia, L., Ventura, H. Perez, Puglisi, A., Rainer, M., Riverol, L., Riverol, C., Juan, J. San, Scuderi, S., Seemann, U., Sokal, K. R., Sozzetti, A., Sozzi, M.
Publikováno v:
A&A 613, A50 (2018)
Context. Stellar activity is currently challenging the detection of young planets via the radial velocity (RV) technique. Aims. We attempt to definitively discriminate the nature of the RV variations for the young active K5 star BD+20 1790, for which
Externí odkaz:
http://arxiv.org/abs/1805.01281
Autor:
Origlia, L., Oliva, E., Sanna, N., Mucciarelli, A., Dalessandro, E., Scuderi, S., Baffa, C., Biliotti, V., Carbonaro, L., Falcini, G., Giani, E., Iuzzolino, M., Massi, F., Sozzi, M., Tozzi, A., Ghedina, A., Ghinassi, F., Lodi, M., Harutyunyan, A., Pedani, M.
The Scutum complex in the inner disk of the Galaxy has a number of young star clusters dominated by red supergiants that are heavily obscured by dust extinction and observable only at infrared wavelengths. These clusters are important tracers of the
Externí odkaz:
http://arxiv.org/abs/1510.06870
Autor:
Oliva, E., Origlia, L., Scuderi, S., Benatti, S., Carleo, I., Lapenna, E., Mucciarelli, A., Baffa, C., Biliotti, V., Carbonaro, L., Falcini, G., Giani, E., Iuzzolino, M., Massi, F., Sanna, N., Sozzi, M., Tozzi, A, Ghedina, A., Ghinassi, F., Lodi, M., Harutyunyan, A., Pedani, M.
Publikováno v:
A&A 581, A47 (2015)
Aims Determining the intensity of lines and continuum airglow emission in the H-band is important for the design of faint-object infrared spectrographs. Existing spectra at low/medium resolution cannot disentangle the true sky-continuum from instrume
Externí odkaz:
http://arxiv.org/abs/1506.09004
Autor:
Tozzi, A., Oliva, E., Origlia, L., Baffa, C., Biliotti, V., Falcini, G., Giani, E., Iuzzolino, M., Massi, F., Sanna, N., Scuderi, S., Sozzi, M.
Giano is a Cryogenic Spectrograph located in T.N.G. (Spain) and commisioned in 2013. It works in the range 950-2500 nm with a resolving power of 50000. This instrument was designed and built for direct feeding from the telescope [2]. However, due to
Externí odkaz:
http://arxiv.org/abs/1407.3126
Autor:
Origlia, L., Oliva, E., Maiolino, R., Mucciarelli, A., Baffa, C., Biliotti, V., Bruno, P., Falcini, G., Gavriousev, V., Ghinassi, F., Giani, E., Gonzalez, M., Leone, F., Lodi, M., Massi, F., Montegriffo, P., Mochi, I., Pedani, M., Rossetti, E., Scuderi, S., Sozzi, M., Tozzi, A.
The inner disk of the Galaxy has a number of young star clusters dominated by red supergiants that are heavily obscured by dust extinction and observable only at infrared wavelengths. These clusters are important tracers of the recent star formation
Externí odkaz:
http://arxiv.org/abs/1311.1639
Autor:
Oliva, E., Origlia, L., Maiolino, R., Baffa, C., Biliotti, V., Bruno, P., Falcini, G., Gavriousev, V., Ghinassi, F., Giani, E., Gonzalez, M., Leone, F., Lodi, M., Massi, F., Montegriffo, P., Mochi, I., Pedani, M., Rossetti, E., Scuderi, S., Sozzi, M., Tozzi, A., Valenti, E.
A flux-calibrated high resolution spectrum of the airglow emission is a practical lambda-calibration reference for astronomical spectral observations. It is also useful for constraining the molecular parameters of the OH molecule and the physical con
Externí odkaz:
http://arxiv.org/abs/1305.3176
Autor:
Coyle, Laura E., Matsuura, Shuji, Perrin, Marshall D., Picchi, P., Tozzi, A., Brucalassi, A., Araiza, Antonio J., Pace, E., Chioetto, P., Zuppella, P., Scippa, A., Lilli, R., Gottini, D., Alvarez, J., García, A., Soler, Alejandro J., D'Anca, F., Guerriero, E., Del Vecchio, C., Falcini, G., Carbonaro, L., Eccleston, P., Caldwell, A., Ferruzzi, D., Malaguti, G., Micela, G., Pascale, E., Bocchieri, A., Preti, G., Piazzolla, R., Salatti, M., Brienza, D., Tommasi, E., Tinetti, G., Vernani, D., Morgante, G.
Publikováno v:
Proceedings of SPIE; August 2024, Vol. 13092 Issue: 1 p130924G-130924G-19, 12961496p
