Zobrazeno 1 - 10
of 453
pro vyhledávání: '"Turrini, D"'
Autor:
Naponiello, L., Bonomo, A. S., Mancini, L., Steinmeyer, M. L., Biazzo, K., Polychroni, D., Dorn, C., Turrini, D., Lanza, A. F., Sozzetti, A., Desidera, S., Damasso, M., Collins, K. A., Carleo, I., Collins, K. I., Colombo, S., D'Arpa, M. C., Dumusque, X., Gonzalez, M., Guilluy, G., Lorenzi, V., Mantovan, G., Nardiello, D., Pinamonti, M., Schwarz, R. P., Singh, V., Watkins, C. N., Zingales, T.
We examined in depth the star BD+00 444 (GJ 105.5, TOI-2443; V = 9.5 mag; d = 23.9 pc), with the aim of characterizing and confirming the planetary nature of its small companion, the planet candidate TOI-2443.01, which was discovered by TESS. We moni
Externí odkaz:
http://arxiv.org/abs/2411.09417
Autor:
Filomeno, S., Biazzo, K., Baratella, M., Benatti, S., D'Orazi, V., Desidera, S., Mancini, L., Messina, S., Polychroni, D., Turrini, D., Cabona, L., Carleo, I., Damasso, M., Malavolta, L., Mantovan, G., Nardiello, D., Scandariato, G., Sozzetti, A., Zingales, T., Andreuzzi, G., Antoniucci, S., Bignamini, A., Bonomo, A. S., Claudi, R., Cosentino, R., Fiorenzano, A. F. M., Fonte, S., Harutyunyan, A., Knapic, C.
The study of exoplanets at different evolutionary stages can shed light on their formation, migration, and evolution. The determination of exoplanet properties depends on the properties of their host stars. It is therefore important to characterise t
Externí odkaz:
http://arxiv.org/abs/2409.00675
Autor:
da Silva, R., Danielski, C., Mena, E. Delgado, Magrini, L., Turrini, D., Biazzo, K., Tsantaki, M., Rainer, M., Helminiak, K. G., Benatti, S., Adibekyan, V., Sanna, N., Sousa, S., Casali, G., Van der Swaelmen, M.
Publikováno v:
A&A 688, A193 (2024)
One of the ultimate goals of the ESA Ariel space mission is to shed light on the formation pathways and evolution of planetary systems in the Solar neighbourhood. Such an endeavour is only possible by performing a large chemical survey of not only th
Externí odkaz:
http://arxiv.org/abs/2406.12393
TOI-837 b: characterisation, formation and evolutionary history of an infant warm Saturn-mass planet
Autor:
Damasso, M., Polychroni, D., Locci, D., Turrini, D., Maggio, A., Cubillos, P. E., Baratella, M., Biazzo, K., Benatti, S., Mantovan, G., Nardiello, D., Desidera, S., Bonomo, A. S., Pinamonti, M., Malavolta, L., Marzari, F., Sozzetti, A., Spinelli, R.
Publikováno v:
A&A 688, A15 (2024)
We aim to determine the fundamental properties of the $\sim$35 Myr old star TOI-837 and its close-in Saturn-sized planet, and to investigate the system's formation and evolutionary history. We analysed TESS photometry and HARPS spectroscopic data, me
Externí odkaz:
http://arxiv.org/abs/2406.08949
Autor:
Zak, J., Boffin, H. M. J., Sedaghati, E., Bocchieri, A., Changeat, Q., Fukui, A., Hatzes, A., Hillwig, T., Hornoch, K., Itrich, D., Ivanov, V. D., Jones, D., Kabath, P., Kawai, Y., Mugnai, L. V., Murgas, F., Narita, N., Palle, E., Pascale, E., Pravec, P., Redfield, S., Roccetti, G., Roth, M., Srba, J., Tian, Q., Tsiaras, A., Turrini, D., Vignes, J. P.
Planetary systems in mean motion resonances hold a special place among the planetary population. They allow us to study planet formation in great detail as dissipative processes are thought to have played an important role in their existence. Additio
Externí odkaz:
http://arxiv.org/abs/2405.12409
Autor:
Mantovan, G., Malavolta, L., Locci, D., Polychroni, D., Turrini, D., Maggio, A., Desidera, S., Spinelli, R., Benatti, S., Piotto, G., Lanza, A. F., Marzari, F., Sozzetti, A., Damasso, M., Nardiello, D., Cabona, L., D'Arpa, M., Guilluy, G., Mancini, L., Micela, G., Nascimbeni, V., Zingales, T.
Multi-planet systems exhibit remarkable architectural diversity. However, short-period giant planets are typically isolated. Compact systems like TOI-5398, with an outer close-orbit giant and an inner small-size planet, are rare among systems contain
Externí odkaz:
http://arxiv.org/abs/2404.02969
Autor:
Basilicata, M., Giacobbe, P., Bonomo, A. S., Scandariato, G., Brogi, M., Singh, V., Di Paola, A., Mancini, L., Sozzetti, A., Lanza, A. F., Cubillos, P. E., Damasso, M., Desidera, S., Biazzo, K., Bignamini, A., Borsa, F., Cabona, L., Carleo, I., Ghedina, A., Guilluy, G., Maggio, A., Mainella, G., Micela, G., Molinari, E., Molinaro, M., Nardiello, D., Pedani, M., Pino, L., Poretti, E., Southworth, J., Stangret, M., Turrini, D.
Publikováno v:
A&A 686, A127 (2024)
The atmospheric characterisation of hot and warm Neptune-size exoplanets is challenging due to their small radius and atmospheric scale height. The warm-Neptune HAT-P-11b is a remarkable target for such characterisation due to the large brightness of
Externí odkaz:
http://arxiv.org/abs/2403.01527
Autor:
Carleo, I., Malavolta, L., Desidera, S., Nardiello, D., Wang, S., Turrini, D., Lanza, A. F., Baratella, M., Marzari, F., Benatti, S., Biazzo, K., Bieryla, A., Brahm, R., Bonavita, M., Collins, K. A., Hellier, C., Locci, D., Hobson, M. J., Maggio, A., Mantovan, G., Pinamonti, S. Messina M., Rodriguez, J. E., Sozzetti, A., Stassun, K., Wang, X. Y., Ziegler, C., Damasso, M., Giacobbe, P., Murgas, F., Parviainen, H., Andreuzzi, G., Barkaoui, K., Berlind, P., Bignamini, A., Borsa, F., Briceño, C., Brogi, M., Cabona, L., Calkins, M. L., Capuzzo-Dolcetta, R., Cecconi, M., Colon, K. D., Cosentino, R., Dragomir, D., Esquerdo, G. A., Henning, T., Ghedina, A., Goeke, R. F., Gratton, R., Horta, F. Grau, Gupta, A. F., Jenkins, J. M., Jordán, A., Knapic, C., Latham, D. W., Mireles, I., Law, N., Lorenzi, V., Lund, M. B., Maldonado, J., Mann, A. W., Molinari, E., Pallé, E., Paegert, M., Pedani, M., Quinn, S. N., Scandariato, G., Seager, S., Winn, J. N., Wohler, B., Zingales, T.
Context. Different theories have been developed to explain the origins and properties of close-in giant planets, but none of them alone can explain all of the properties of the warm Jupiters (WJs, Porb = 10 - 200 days). One of the most intriguing cha
Externí odkaz:
http://arxiv.org/abs/2311.11903
Autor:
Mantovan, G., Malavolta, L., Desidera, S., Zingales, T., Borsato, L., Piotto, G., Maggio, A., Locci, D., Polychroni, D., Turrini, D., Baratella, M., Biazzo, K., Nardiello, D., Stassun, K., Nascimbeni, V., Benatti, S., John, A. Anna, Watkins, C., Bieryla, A., Lissauer, J. J., Twicken, J. D., Lanza, A. F., Winn, J. N., Messina, S., Montalto, M., Sozzetti, A., Boffin, H., Cheryasov, D., Strakhov, I., Murgas, F., D'Arpa, M., Barkaoui, K., Benni, P., Bignamini, A., Bonomo, A., Borsa, F., Cabona, L., Cameron, A. C., Claudi, R., Cochran, W., Collins, K. A., Damasso, M., Dong, J., Endl, M., Fukui, A., Furész, G., Gandolfi, D., Ghedina, A., Jenkins, J., Kabáth, P., Latham, D. W., Lorenzi, V., Luque, R., Maldonado, J., McLeod, K., Molinaro, M., Narita, N., Nowak, G., Orell-Miquel, J., Pallé, E., Parviainen, H., Pedani, M., Quinn, S. N., Relles, H., Rowden, P., Scandariato, G., Schwarz, R., Seager, S., Shporer, A., Vanderburg, A., Wilson, T. G.
Short-period giant planets are frequently found to be solitary compared to other classes of exoplanets. Small inner companions to giant planets with $P \lesssim$ 15 days are known only in five compact systems: WASP-47, Kepler-730, WASP-132, TOI-1130,
Externí odkaz:
http://arxiv.org/abs/2310.16888
Autor:
Damasso, M., Scandariato, G., Nascimbeni, V., Nardiello, D., Mancini, L., Marino, G., Bruno, G., Brandeker, A., Leto, G., Marzari, F., Lanza, A. F., Benatti, S., Desidera, S., Béjar, V. J. S., Biagini, A., Borsato, L., Cabona, L., Claudi, R., Lodieu, N., Maggio, A., Díaz, M. Mallorquín, Messina, S., Micela, G., Ricci, D., Sozzetti, A., Mascareño, A. Suárez, Turrini, D., Osorio, M. R. Zapatero
V1298 Tau hosts at least four planets. Since its discovery, this system has been a target of intensive photometric and spectroscopic monitoring. The characterisation of its architecture and planets' fundamental properties turned out to be very challe
Externí odkaz:
http://arxiv.org/abs/2309.14131