Zobrazeno 1 - 10
of 363
pro vyhledávání: '"{Affer} L."'
Autor:
Nardiello, D., Murphy, J. M. Akana, Spinelli, R., Baratella, M., Desidera, S., Nascimbeni, V., Malavolta, L., Biazzo, K., Maggio, A., Locci, D., Benatti, S., Batalha, N. M., D'Orazi, V., Borsato, L., Piotto, G., Oelkers, R. J., Mallonn, M., Sozzetti, A., Bedin, L. R., Mantovan, G., Zingales, T., Affer, L., Bignamini, A., Bonomo, A. S., Cabona, L., Collins, K. A., Damasso, M., Filomeno, S., Ghedina, A., Harutyunyan, A., Lanza, A. F., Mancini, L., Rainer, M., Scandariato, G., Schwarz, R. P., Sefako, R., Srdoc, G.
Small-sized exoplanets in tight orbits around young stars (10-1000 Myr) give us the opportunity to investigate the mechanisms that led to their formation, the evolution of their physical and orbital properties and, especially, of their atmospheres. T
Externí odkaz:
http://arxiv.org/abs/2411.12795
Autor:
D'Arpa, M. C., Guilluy, G., Mantovan, G., Biassoni, F., Spinelli, R., Sicilia, D., Locci, D., Maggio, A., Lanza, A. F., Petralia, A., Di Maio, C., Benatti, S., Bonomo, A. S., Borsa, F., Cabona, L., Desidera, S., Fossati, L., Micela, G., Malavolta, L., Mancini, L., Scandariato, G., Sozzetti, A., Stangret, M., Affer, L., Amadori, F., Basilicata, M., Bignamini, A., Boschin, W., Ghedina, A.
Publikováno v:
A&A 692, A77 (2024)
Atmospheric characterization is key to understanding exoplanetary systems, offering insights into the planets current and past conditions. By analyzing key lines like H alpha and the He I triplet, we can trace the evolution of planets through atmosph
Externí odkaz:
http://arxiv.org/abs/2410.15917
Autor:
D'Arpa, M. C., Saba, A., Borsa, F., Fossati, L., Micela, G., Di Maio, C., Stangret, M., Tripodo, G., Affer, L., Bonomo, A. S., Benatti, S., Brogi, M., Fardella, V., Lanza, A. F., Guilluy, G., Maldonado, J., Mantovan, G., Nascimbeni, V., Pino, L., Scandariato, G., Sicilia, D., Sozzetti, A., Spinelli, R., Andreuzzi, G., Bignamini, A., Claudi, R., Desidera, S., Ghedina, A., Knapic, C., Lorenzi, V.
Publikováno v:
A&A 690, A237 (2024)
We analysed six primary transits of the ultra-hot Jupiter KELT-9,b obtained with the HARPS-N high-resolution spectrograph in the context of the Global Architecture of Planetary Systems (GAPS2) project, to characterise the atmosphere via single-line a
Externí odkaz:
http://arxiv.org/abs/2409.01779
The GAPS Programme at TNG. XXX: Characterization of the low-density gas giant HAT-P-67 b with GIARPS
Autor:
Sicilia, D., Scandariato, G., Guilluy, G., Esposito, M., Borsa, F., Stangret, M., Di Maio, C., Lanza, A. F., Bonomo, A. S., Desidera, S., Fossati, L., Nardiello, D., Sozzetti, A., Malavolta, L., Nascimbeni, V., Rainer, M., D'Arpa, M. C., Mancini, L., Singh, V., Zingales, T., Affer, L., Bignamini, A., Claudi, R., Colombo, S., Cosentino, R., Ghedina, A., Micela, G., Molinari, E., Molinaro, M., Pagano, I., Piotto, G.
Publikováno v:
A&A 687, A143 (2024)
HAT-P-67 b is one of the lowest-density gas giants known to date, making it an excellent target for atmospheric characterization through the transmission spectroscopy technique. In the framework of the GAPS large programme, we collected four transit
Externí odkaz:
http://arxiv.org/abs/2404.03317
Autor:
Palethorpe, L., John, A. Anna, Mortier, A., Davoult, J., Wilson, T. G., Rice, K., Cameron, A. C., Alibert, Y., Buchhave, L. A., Malavolta, L., Cadman, J., López-Morales, M., Dumusque, X., Silva, A. M., Quinn, S. N., Van Eylen, V., Vissapragada, S., Affer, L., Charbonneau, D., Cosentino, R., Ghedina, A., Haywood, R. D., Latham, D. W., Lienhard, F., Fiorenzano, A. F. Martínez, Pedani, M., Pepe, F., Pinamonti, M., Sozzetti, A., Stalport, M., Udry, S., Vanderburg, A.
Publikováno v:
MNRAS, 529, 3323-3341 (2024)
We report on the detailed characterization of the HD 77946 planetary system. HD 77946 is an F5 ($M_*$ = 1.17 M$_{\odot}$, $R_*$ = 1.31 R$_{\odot}$) star, which hosts a transiting planet recently discovered by NASA's Transiting Exoplanet Survey Satell
Externí odkaz:
http://arxiv.org/abs/2403.04464
Autor:
Guilluy, G., D'Arpa, M. C., Bonomo, A. S., Spinelli, R., Biassoni, F., Fossati, L., Maggio, A., Giacobbe, P., Lanza, A. F., Sozzetti, A., Borsa, F., Rainer, M., Micela, G., Affer, L., Andreuzzi, G., Bignamini, A., Boschin, W., Carleo, I., Cecconi, M., Desidera, S., Fardella, V., Ghedina, A., Mantovan, G., Mancini, L., Nascimbeni, V., Knapic, C., Pedani, M., Petralia, A., Pino, L., Scandariato, G., Sicilia, D., Stangret, M., Zingales, T.
Atmospheric escape plays a fundamental role in shaping the properties of exoplanets. The metastable near-infrared helium triplet at 1083.3 nm (HeI) is a powerful proxy of extended and evaporating atmospheres. We used the GIARPS (GIANO-B+HARPS-N) obse
Externí odkaz:
http://arxiv.org/abs/2403.00608
Autor:
Di Maio, C., Petralia, A., Micela, G., Lanza, A. F., Rainer, M., Malavolta, L., Benatti, S., Affer, L., Maldonado, J., Colombo, S., Damasso, M., Maggio, A., Biazzo, K., Bignamini, A., Borsa, F., Boschin, W., Cabona, L., Cecconi, M., Claudi, R., Covino, E., Di Fabrizio, L., Gratton, R., Lorenzi, V., Mancini, L., Messina, S., Molinari, E., Molinaro, M., Nardiello, D., Poretti, E., Sozzetti, A.
The intrinsic variability due to the magnetic activity of young active stars is one of the main challenges in detecting and characterising exoplanets. We present a method able to model the stellar photosphere and its surface inhomogeneities (starspot
Externí odkaz:
http://arxiv.org/abs/2312.14269
Autor:
Nicholson, B. A., Aigrain, S., Eisner, N. L., Cretignier, M., Barragán, O., Kaye, L., Taylor, J., Owen, J., Mortier, A., Affer, L., Boschin, W., Cameron, A. Collier, Damasso, M., Di Fabrizio, L., DiTomasso, V., Dumusque, X., Gehdina, A., Harutyunyan, A., Latham, D. W., Lopez-Morales, M., Lorenzi, V., Fiorenzano, A. F. Martínez, Molinari, E., Pedani, M., Pinamonti, M., Sozzetti, A., Rice, K.
We present the characterisation of the two transiting planets around HD 152843 (TOI 2319, TIC 349488688) using an intensive campaign of HARPS-N radial velocities, and two sectors of TESS data. These data reveal a unique and fascinating system: HD 152
Externí odkaz:
http://arxiv.org/abs/2310.15068
Autor:
Rescigno, F., Hébrard, G., Vanderburg, A., Mann, A. W., Mortier, A., Morrell, S., Buchhave, L. A., Collins, K. A., Mann, C. R., Hellier, C., Haywood, R. D., West, R., Stalport, M., Heidari, N., Anderson, D., Huang, C. X., López-Morales, M., Cortés-Zuleta, P., Lewis, H. M., Dumusque, X., Boisse, I., Rowden, P., Cameron, A. Collier, Deleuil, M., Vezie, M., Pepe, F. A., Delfosse, X., Charbonneau, D., Rice, K., Demangeon, O., Quinn, S. N., Udry, S., Forveille, T., Winn, J. N., Sozzetti, A., Hoyer, S., Seager, S., Wilson, T. G., Dalal, S., Martioli, E., Striegel, S., Boschin, W., Dragomir, D., Fiorenzano, A. F. Martínez, Cosentino, R., Ghedina, A., Malavolta, L., Affer, L., Lakeland, B. S., Nicholson, B. A., Foschino, S., Wünsche, A., Barkaoui, K., Srdoc, G., Randolph, J., Guillet, B., Conti, D. M., Ghachoui, M., Gillon, M., Benkhaldoun, Z., Pozuelos, F. J., Timmermans, M., Girardin, E., Matutano, S., Bosch-Cabot, P., Muñoz, J. A., Forés-Toribio, R.
We present the characterisation of an inner mini-Neptune in a 9.2292005$\pm$0.0000063 day orbit and an outer mono-transiting sub-Saturn planet in a 95.50$^{+0.36}_{-0.25}$ day orbit around the moderately active, bright (mv=8.9 mag) K5V star TOI-2134.
Externí odkaz:
http://arxiv.org/abs/2310.13623
Autor:
Rainer, M., Desidera, S., Borsa, F., Barbato, D., Biazzo, K., Bonomo, A., Gratton, R., Messina, S., Scandariato, G., Affer, L., Benatti, S., Carleo, I., Cabona, L., Covino, E., Lanza, A. F., Ligi, R., Maldonado, J., Mancini, L., Nardiello, D., Sicilia, D., Sozzetti, A., Bignamini, A., Cosentino, R., Knapic, C., Fiorenzano, A. F. Martínez, Molinari, E., Pedani, M., Poretti, E.
Publikováno v:
A&A 676, A90 (2023)
The leading spectrographs used for exoplanets' sceince offer online data reduction softwares (DRS) that yield as an ancillary result the full-width at half-maximum (FWHM) of the cross-correlation function (CCF) that is used to estimate the radial vel
Externí odkaz:
http://arxiv.org/abs/2306.13468