Zobrazeno 1 - 10
of 123
pro vyhledávání: '"Lissauer, J."'
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:
Naponiello, L., Mancini, L., Sozzetti, A., Bonomo, A. S., Morbidelli, A., Dou, J., Zeng, L., Leinhardt, Z. M., Biazzo, K., Cubillos, P., Pinamonti, M., Locci, D., Maggio, A., Damasso, M., Lanza, A. F., Lissauer, J. J., Bignamini, A., Boschin, W., Bouma, L. G., Carter, P. J., Ciardi, D. R., Collins, K. A., Cosentino, R., Crossfield, I., Desidera, S., Dumusque, X., Fiorenzano, A. F. M., Fukui, A., Giacobbe, P., Gnilka, C. L., Ghedina, A., Gonzales, E., Guilluy, G., Harutyunyan, A., Howell, S. B., Jenkins, J. M., Lund, M. B., Jensen, E. L. N., Kielkopf, J. F., Lester, K. V., Malavolta, L., Mann, A. W., Matson, R. A., Matthews, E. C., Nardiello, D., Narita, N., Pace, E., Pagano, I., Palle, E., Pedani, M., Seager, S., Schlieder, J. E., Schwarz, R. P., Shporer, A., Twicken, J. D., Winn, J. N., Ziegler, C., Zingales, T.
Publikováno v:
Nature, published online on the 30th of August 2023 and printed the 12th of October 2023
Neptune-sized planets exhibit a wide range of compositions and densities, depending onf cators related to their formation and evolution history, such as the distance from their host stars and atmospheric escape processes. They can vary from relativel
Externí odkaz:
http://arxiv.org/abs/2309.01464
Autor:
Almenara, J. M., Bonfils, X., Forveille, T., Astudillo-Defru, N., Ciardi, D. R., Schwarz, R. P., Collins, K. A., Cointepas, M., Lund, M. B., Bouchy, F., Charbonneau, D., Díaz, R. F., Delfosse, X., Kidwell, R. C., Kunimoto, M., Latham, D. W., Lissauer, J. J., Murgas, F., Ricker, G., Seager, S., Vezie, M., Watanabe, D.
Publikováno v:
A&A 667, L11 (2022)
The Transiting Exoplanet Survey Satellite mission identified a deep and asymmetric transit-like signal with a periodicity of 4.5 days orbiting the M4 dwarf star TOI-3884. The signal has been confirmed by follow-up observations collected by the ExTrA
Externí odkaz:
http://arxiv.org/abs/2210.10909
Autor:
Naponiello, L., Mancini, L., Damasso, M., Bonomo, A. S., Sozzetti, A., Nardiello, D., Biazzo, K., Stognone, R. G., Lillo-Box, J., Lanza, A. F., Poretti, E., Lissauer, J. J., Zeng, L., Bieryla, A., Hébrard, G., Basilicata, M., Benatti, S., Bignamini, A., Borsa, F., Claudi, R., Cosentino, R., Covino, E., de Gurtubai, A., Delfosse, X., Desidera, S., Dragomir, D., Eastman, J. D., Essack, Z., Fiorenzano, A. F. M., Giacobbe, P., Harutyunyan, A., Heidari, N., Hellier, C., Jenkins, J. M., Knapic, C., König, P. -C., Latham, D. W., Magazzù, A., Maggio, A., Maldonado, J., Micela, G., Molinari, E., Molinaro, M., Morgan, E. H., Moutou, C., Nascimben, V., Pace, E., Pagano, I., Pedani, M., Piotto, G., Pinamonti, M., Quintana, E. V., Rainer, M., Ricker, G. R., Seager, S., Twicken, J. D., Vanderspek, R., Winn, J. N.
Publikováno v:
A&A 667, A8 (2022)
We investigate the exoplanet candidate TOI-1422b, which was discovered by the TESS space telescope around the high proper-motion G2V star TOI-1422 ($V=10.6$ mag), 155pc away, with the primary goal of confirming its planetary nature and characterising
Externí odkaz:
http://arxiv.org/abs/2207.03293
Autor:
Luque, R., Fulton, B. J., Kunimoto, M., Amado, P. J., Gorrini, P., Dreizler, S., Hellier, C., Henry, G. W., Molaverdikhani, K., Morello, G., Peña-Moñino, L., Pérez-Torres, M., Pozuelos, F. J., Shan, Y., Anglada-Escudé, G., Béjar, V. J. S., Bergond, G., Boyle, A. W., Caballero, J. A., Charbonneau, D., Ciardi, D. R., Dufoer, S., Espinoza, N., Everett, M., Fischer, D., Hatzes, A. P., Henning, Th., Hesse, K., Howard, A., Howell, S. B., Isaacson, H., Jeffers, S. V., Jenkins, J. M., Kane, S. R., Kemmer, J., Khalafinejad, S., Kidwell Jr., R. C., Kossakowski, D., Latham, D. W., Lillo-Box, J., Lissauer, J. J., Montes, D., Orell-Miquel, J., Pallé, E., Pollacco, D., Quirrenbach, A., Reffert, S., Reiners, A., Ribas, I., Ricker, G. R., Rogers, L. A., Sanz-Forcada, J., Schlecker, M., Schweitzer, A., Seager, S., Shporer, A., Stassun, K. G., Stock, S., Tal-Or, L., Ting, E. B., Trifonov, T., Vanaverbeke, S., Vanderspek, R., Villaseñor, J., Winn, J. N., Winters, J. G., Osorio, M. R. Zapatero
Publikováno v:
A&A 664, A199 (2022)
We report the discovery of a multi-planetary system transiting the M0 V dwarf HD 260655 (GJ 239, TOI-4599). The system consists of at least two transiting planets, namely HD 260655 b, with a period of 2.77 d, a radius of R$_b$ = 1.240$\pm$0.023 R$_\o
Externí odkaz:
http://arxiv.org/abs/2204.10261
Autor:
Almenara, J. M., Hébrard, G., Díaz, R. F., Laskar, J., Correia, A. C. M., Anderson, D. R., Boisse, I., Bonfils, X., Brown, D. J. A., Casanova, V., Cameron, A. Collier, Fernández, M., Jenkins, J. M., Kiefer, F., Étangs, A. Lecavelier des, Lissauer, J. J, Maciejewski, G., McCormac, J., Osborn, H., Pollacco, D., Ricker, G., Sánchez, J., Seager, S., Udry, S., Verilhac, D., Winn, J.
Publikováno v:
A&A 663, A134 (2022)
WASP-148 is a recently announced extra-solar system harbouring at least two giant planets. The inner planet transits its host star. The planets travel on eccentric orbits and are near the 4:1 mean-motion resonance, which implies significant mutual gr
Externí odkaz:
http://arxiv.org/abs/2204.06656
Autor:
Šubjak, J., Endl, M., Chaturvedi, P., Karjalainen, R., Cochran, W. D., Esposito, M., Gandolfi, D., Lam, K. W. F., Stassun, K., Žák, J., Lodieu, N., Boffin, H. M. J., MacQueen, P. J., Hatzes, A., Guenther, E. W., Georgieva, I., Grziwa, S., Schmerling, H., Skarka, M., Blažek, M., Karjalainen, M., Špoková, M., Isaacson, H., Howard, A. W., Burke, C. J., Van Eylen, V., Falk, B., Fridlund, M., Goffo, E., Jenkins, J. M., Korth, J., Lissauer, J. J., Livingston, J. H., Luque, R., Muresan, A., Osborn, H. P., Pallé, E., Persson, C. M., Redfield, S., Ricker, G. R., Seager, S., Serrano, L. M., Smith, A. M. S., Kabáth, P.
Publikováno v:
A&A 662, A107 (2022)
We report the discovery of TOI-1268b, a transiting Saturn-mass planet from the TESS space mission. With an age of less than one Gyr, derived from various age indicators, TOI-1268b is the youngest Saturn-mass planet known to date and contributes to th
Externí odkaz:
http://arxiv.org/abs/2201.13341
Autor:
Cloutier, R., Charbonneau, D., Stassun, K. G., Murgas, F., Mortier, A., Massey, R., Lissauer, J. J., Latham, D. W., Irwin, J., Haywood, R. D., Guerra, P., Girardin, E., Giacalone, S. A., Bosch-Cabot, P., Bieryla, A., Winn, J., Watson, C. A., Vanderspek, R., Udry, S., Tamura, M., Sozzetti, A., Shporer, A., Ségransan, D., Seager, S., Savel, A. B., Sasselov, D., Rose, M., Ricker, G., Rice, K., Quintana, E. V., Quinn, S. N., Piotto, G., Phillips, D., Pepe, F., Pedani, M., Parviainen, H., Palle, E., Narita, N., Molinari, E., Micela, G., McDermott, S., Mayor, M., Matson, R. A., Fiorenzano, A. F. Martinez, Lovis, C., López-Morales, M., Kusakabe, N., Jensen, E. L. N., Jenkins, J. M., Huang, C. X., Howell, S. B., Harutyunyan, A., Fűrész, G., Fukui, A., Esquerdo, G. A., Esparza-Borges, E., Dumusque, X., Dressing, C. D., Di Fabrizio, L., Collins, K. A., Cameron, A. Collier, Christiansen, J. L., Cecconi, M., Buchhave, L. A., Boschin, W., Andreuzzi, G.
Studies of close-in planets orbiting M dwarfs have suggested that the M dwarf radius valley may be well-explained by distinct formation timescales between enveloped terrestrials, and rocky planets that form at late times in a gas-depleted environment
Externí odkaz:
http://arxiv.org/abs/2103.12790
Autor:
Luque, R., Serrano, L. M., Molaverdikhani, K., Nixon, M. C., Livingston, J. H., Guenther, E. W., Pallé, E., Madhusudhan, N., Nowak, G., Korth, J., Cochran, W. D., Hirano, T., Chaturvedi, P., Goffo, E., Albrecht, S., Barragán, O., Briceño, C, Cabrera, J., Charbonneau, D., Cloutier, R., Collins, K. A., Collins, K. I., Colón, K. D., Crossfield, I. J. M., Csizmadia, Sz., Dai, F., Deeg, H. J., Esposito, M., Fridlund, M., Gandolfi, D., Georgieva, I., Glidden, A., Goeke, R. F., Grziwa, S., Hatzes, A. P., Henze, C. E., Howell, S. B., Irwin, J., Jenkins, J. M., Jensen, E. L. N., Kábath, P., Kidwell Jr., R. C., Kielkopf, J. F., Knudstrup, E., Lam, K. W. F., Latham, D. W., Lissauer, J. J., Mann, A. W., Matthews, E. C., Mireles, I., Narita, N., Paegert, M., Persson, C. M., Redfield, S., Ricker, G. R., Rodler, F., Schlieder, J. E., Scott, N. J., Seager, S., Šubjak, J., Tan, T. G., Ting, E. B., Vanderspek, R., Van Eylen, V., Winn, J. N., Ziegler, C.
Publikováno v:
A&A 645, A41 (2021)
We report the discovery and characterization of two transiting planets around the bright M1 V star LP 961-53 (TOI-776, J = 8.5 mag, M = 0.54+-0.03 Msun) detected during Sector 10 observations of the Transiting Exoplanet Survey Satellite (TESS). Combi
Externí odkaz:
http://arxiv.org/abs/2009.08338
Autor:
Demory, B. -O., Pozuelos, F. J., Chew, Y. Gomez Maqueo, Sabin, L., Petrucci, R., Schroffenegger, U., Grimm, S. L., Sestovic, M., Gillon, M., McCormac, J., Barkaoui, K., Benz, W., Bieryla, A., Bouchy, F., Burdanov, A., Collins, K. A., de Wit, J., Dressing, C. D., Garcia, L. J., Giacalone, S., Guerra, P., Haldemann, J., Heng, K., Jehin, E., Jofre, E., Kane, S. R., Lillo-Box, J., Maigne, V., Mordasini, C., Morris, B. M., Niraula, P., Queloz, D., Rackham, B. V., Savel, A. B., Soubkiou, A., Srdoc, G., Stassun, K. G., Triaud, A. H. M. J., Zambelli, R., Ricker, G., Latham, D. W., Seager, S., Winn, J. N., Jenkins, J. M., Calvario-Velasquez, T., Herrera, J. A. Franco, Colorado, E., Zepeda, E. O. Cadena, Figueroa, L., Watson, A. M., Lugo-Ibarra, E. E., Carigi, L., Guisa, G., Herrera, J., Diaz, G. Sierra, Suarez, J. C., Barrado, D., Batalha, N. M., Benkhaldoun, Z., Chontos, A., Dai, F., Essack, Z., Ghachoui, M., Huang, C. X., Huber, D., Isaacson, H., Lissauer, J. J., Morales-Calderon, M., Robertson, P., Roy, A., Twicken, J. D., Vanderburg, A., Weiss, L. M.
Publikováno v:
A&A 642, A49 (2020)
We report the discovery and characterisation of a super-Earth and a sub-Neptune transiting the bright ($K=8.8$), quiet, and nearby (37 pc) M3V dwarf TOI-1266. We validate the planetary nature of TOI-1266 b and c using four sectors of TESS photometry
Externí odkaz:
http://arxiv.org/abs/2009.04317