Zobrazeno 1 - 10
of 458
pro vyhledávání: '"Lódi M"'
Autor:
Sicilia, D., Malavolta, L., Scandariato, G., Fossati, L., Lanza, A. F., Bonomo, A. S., Borsa, F., Guilluy, G., Nascimbeni, V., Pino, L., Biassoni, F., D'Arpa, M. C., Pagano, I., Sozzetti, A., Stangret, M., Cosentino, R., Giacobbe, P., Lodi, M., Maldonado, J., Nardiello, D., Pedani, M.
The neutral sodium resonance doublet (Na i D) has been detected in the upper atmosphere of several close-in gas giants, through high-resolution transmission spectroscopy. We aim to investigate whether its variability is linked to the planets' propert
Externí odkaz:
http://arxiv.org/abs/2412.04330
Autor:
Milbourne, T. W., Phillips, D. F., Langellier, N., Mortier, A., Haywood, R. D., Saar, S. H., Cegla, H. M., Cameron, A. Collier, Dumusque, X., Latham, D. W., Malavolta, L., Maldonado, J., Thompson, S., Vanderburg, A., Watson, C. A., Buchhave, L. A., Cecconi, M., Cosentino, R., Ghedina, A., Gonzalez, M., Lodi, M., López-Morales, M., Sozzetti, A., Walsworth, R. L.
Publikováno v:
The Astrophysical Journal, Volume 920, Number 1, 2021
State of the art radial velocity (RV) exoplanet searches are limited by the effects of stellar magnetic activity. Magnetically active spots, plage, and network regions each have different impacts on the observed spectral lines, and therefore on the a
Externí odkaz:
http://arxiv.org/abs/2105.09113
Autor:
Rainer, M., Borsa, F., Pino, L., Frustagli, G., Brogi, M., Biazzo, K., Bonomo, A. S., Carleo, I., Claudi, R., Gratton, R., Lanza, A. F., Maggio, A., Maldonado, J., Mancini, L., Micela, G., Scandariato, G., Sozzetti, A., Buchschacher, N., Cosentino, R., Covino, E., Ghedina, A., Gonzalez, M., Leto, G., Lodi, M., Fiorenzano, A. F. Martinez, Molinari, E., Molinaro, M., Nardiello, D., Oliva, E., Pagano, I., Pedani, M., Piotto, G., Poretti, E.
Publikováno v:
A&A 649, A29 (2021)
Transiting ultra-hot Jupiters are ideal candidates to study the exoplanet atmospheres and their dynamics, particularly by means of high-resolution, high signal-to-noise ratio spectra. One such object is KELT-20b, orbiting the fast rotating A2-type st
Externí odkaz:
http://arxiv.org/abs/2103.10395
Autor:
Mathelin, C, Barranger, E, Boisserie-Lacroix, M, Boutet, G, Brousse, S, Chabbert-Buffet, N, Coutant, C, Daraï, E, Delpech, Y, Duraes, M, Espié, M, Golfier, F, Hamy, AS, Kermarrec, E, Lavoué, V, Lodi, M, Luporsi, É, Maugard, C, Molière, S, Seror, JY, Taris, N, Uzan, C, Vaysse, C, Fritel, X
Publikováno v:
In Innovative Practice in Breast Health March 2024 1
Autor:
Cameron, A. Collier, Ford, E. B., Shahaf, S., Aigrain, S., Dumusque, X., Haywood, R. D., Mortier, A., Phillips, D. F., Buchhave, L., Cecconi, M., Cegla, H., Cosentino, R., Cretignier, M., Ghedina, A., Gonzalez, M., Latham, D. W., Lodi, M., Lopez-Morales, M., Micela, G., Molinari, E., Pepe, F., Piotto, G., Poretti, E., Queloz, D., Juan, J. San, Segransan, D., Sozzetti, A., Szentgyorgyi, A., Thompson, S., Udry, S., Watson, C.
Stellar magnetic activity produces time-varying distortions in the photospheric line profiles of solar-type stars. These lead to systematic errors in high-precision radial-velocity measurements, which limit efforts to discover and measure the masses
Externí odkaz:
http://arxiv.org/abs/2011.00018
Autor:
Dumusque, X., Cretignier, M., Sosnowska, D., Buchschacher, N., Lovis, C., Phillips, D. F., Pepe, F., Alesina, F., Buchhave, L. A., Burnier, J., Cecconi, M., Cegla, H. M., Cloutier, R., Cameron, A. Collier, Cosentino, R., Ghedina, A., Gonzalez, M., Haywood, R. D., Latham, D. W., Lodi, M., Lopez-Morales, M., Maldonado, J., Malavolta, L., Micela, G., Molinari, E., Mortier, A., Ventura, H. Perez, Pinamonti, M., Poretti, E., Rice, K., Riverol, L., Riverol, C., Juan, J. San, Segransan, D., Sozzetti, A., Thompson, S. J., Udry, S., Wilson, T. G
Publikováno v:
A&A 648, A103 (2021)
The solar telescope connected to HARPS-N has been observing the Sun since the summer of 2015. Such high-cadence, long-baseline data set is crucial for understanding spurious radial-velocity signals induced by our Sun and by the instrument. On the ins
Externí odkaz:
http://arxiv.org/abs/2009.01945
Autor:
Langellier, N., Milbourne, T. W., Phillips, D. F., Haywood, R. D., Saar, S. H., Mortier, A., Malavolta, L., Thompson, S., Cameron, A. Collier, Dumusque, X., Cegla, H. M., Latham, D. W., Maldonado, J., Watson, C. A., Buchschacher, N., Cecconi, M., Charbonneau, D., Cosentino, R., Ghedina, A., Gonzalez, M., Li, C-H., Lodi, M., López-Morales, M., Micela, G., Molinari, E., Pepe, F., Poretti, E., Rice, K., Sasselov, D., Sozzetti, A., Udry, S., Walsworth, R. L.
Publikováno v:
AJ 161 287 (2021)
Radial velocity (RV) searches for Earth-mass exoplanets in the habitable zone around Sun-like stars are limited by the effects of stellar variability on the host star. In particular, suppression of convective blueshift and brightness inhomogeneities
Externí odkaz:
http://arxiv.org/abs/2008.05970
Autor:
Benatti, S., Damasso, M., Desidera, S., Marzari, F., Biazzo, K., Claudi, R., Di Mauro, M. P., Lanza, A. F., Pinamonti, M., Barbato, D., Malavolta, L., Poretti, E., Sozzetti, A., Affer, L., Bignamini, A., Bonomo, A. S., Borsa, F., Brogi, M., Bruno, G., Carleo, I., Cosentino, R., Covino, E., Frustagli, G., Giacobbe, P., Gonzalez, M., Gratton, R., Harutyunyan, A., Knapic, C., Leto, G., Lodi, M., Maggio, A., Maldonado, J., Mancini, L., Fiorenzano, A. Martinez, Micela, G., Molinari, E., Molinaro, M., Nardiello, D., Nascimbeni, V., Pagano, I., Pedani, M., Piotto, G., Rainer, M., Scandariato, G.
Publikováno v:
A&A 639, A50 (2020)
In the framework of the Global Architecture of Planetary Systems (GAPS) project we collected more than 300 spectra with HARPS-N at the TNG for the bright G9V star HD164922. This target is known to host one gas giant planet in a wide orbit (Pb~1200 da
Externí odkaz:
http://arxiv.org/abs/2005.03368
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:
Molière, S., Boutet, G., Azuar, A.-S., Boisserie-Lacroix, M., Brousse, S., Golfier, F., Kermarrec, É., Lavoué, V., Seror, J-Y, Uzan, C., Vaysse, C., Lodi, M., Mathelin, C.
Publikováno v:
In Gynécologie Obstétrique Fertilité & Sénologie October 2023 51(10):471-480