Zobrazeno 1 - 10
of 15
pro vyhledávání: '"Barros, S. C. C."'
Autor:
Ehrenreich, D., Delrez, L., Akinsanmi, B., Wilson, T. G., Bonfanti, A., Beck, M., Benz, W., Hoyer, S., Queloz, D., Alibert, Y., Charnoz, S., Cameron, A. Collier, Deline, A., Hooton, M., Lendl, M., Olofsson, G., Sousa, S. G., Adibekyan, V., Alonso, R., Anglada, G., Barrado, D., Barros, S. C. C., Baumjohann, W., Beck, T., Bekkelien, A., Bergomi, M., Billot, N., Bonfils, X., Brandeker, A., Broeg, C., Bárczy, T., Berta-Thompson, Z. K., Cabrera, J., Van Damme, C. Corral, Csizmadia, S., Davies, M. B., Deleuil, M., Demangeon, O., Demory, B. -O., Doty, J. P., Erikson, A., Fausnaugh, M. M., Florén, H. G., Fortier, A., Fossati, L., Fridlund, M., Futyan, D., Gandolfi, D., Gillon, M., Guterman, P., Güdel, M., Heng, K., Isaak, K. G., Jäckel, A., Jenkins, J. M., Kiss, L. L., Laskar, J., Latham, D. W., Etangs, A. Lecavelier des, Levine, A. M., Lovis, C., Magrin, D., Maxted, P. F. L., Morgan, E. H., Nascimbeni, V., Osborn, H. P., Ottensamer, R., Pagano, I., Pallé, E., Peter, G., Piotto, G., Pollacco, D., Ragazzoni, R., Rando, N., Rauer, H., Ribas, I., Ricker, G. R., Salmon, S., Santos, N. C., Scandariato, G., Simon, A. E., Smith, A. M. S., Steinberger, M., Steller, M., Szabó, G. M., Ségransan, D., Shporer, A., Thomas, N., Tschentscher, M., Udry, S., Vanderspek, R., Van Grootel, V., Walton, N. A.
The planetary system around the naked-eye star $ν^2$ Lupi (HD 136352; TOI-2011) is composed of three exoplanets with masses of 4.7, 11.2, and 8.6 Earth masses. The TESS and CHEOPS missions revealed that all three planets are transiting and have radi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8a8113a528c781a88fea4b9e0fb8ed4f
Autor:
Valdés, E. A. Meier, Morris, B. M., Demory, B. -O., Brandeker, A., Kitzmann, D., Benz, W., Deline, A., Florén, H. -G., Sousa, S. G., Bourrier, V., Singh, V., Heng, K., Strugarek, A., Bower, D. J., Jäggi, N., Carone, L., Lendl, M., Jones, K., Oza, A. V., Demangeon, O. D. S., Alibert, Y., Alonso, R., Anglada, G., Asquier, J., Bárczy, T., Navascues, D. Barrado, Barros, S. C. C., Baumjohann, W., Beck, M., Beck, T., Billot, N., Bonfils, X., Borsato, L., Broeg, C., Cabrera, J., Charnoz, S., Cameron, A. Collier, Csizmadia, Sz., Cubillos, P. E., Davies, M. B., Deleuil, M., Delrez, L., Ehrenreich, D., Erikson, A., Fortier, A., Fossati, L., Fridlund, M., Gandolfi, D., Gillon, M., Güdel, M., Günther, M. N., Hoyer, S., Isaak, K. G., Kiss, L. L., Laskar, J., Etangs, A. Lecavelier des, Lovis, C., Magrin, D., Maxted, P. F. L., Mordasini, C., Nascimbeni, V., Olofsson, G., Ottensamer, R., Pagano, I., Pallé, E., Peter, G., Piotto, G., Pollacco, D., Queloz, D., Ragazzoni, R., Rando, N., Rauer, H., Ribas, I., Santos, N. C., Sarajlic, M., Scandariato, G., Ségransan, D., Sicilia, D., Simon, A. E., Smith, A. M. S., Steller, M., Szabó, Gy. M., Thomas, N., Udry, S., Ulmer, B., Van Grootel, V., Venturini, J., Walton, N. A., Wilson, T. G., Wolter, D.
55 Cnc e is an ultra-short period super-Earth transiting a Sun-like star. Past observations in the optical range detected a time-variable flux modulation phased with the planetary orbital period whose amplitude is too large to be explained by reflect
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::249cee961d6b3e54a6513e8a7d4faa93
Autor:
Barros, S. C. C., Demangeon, O. D. S., Alibert, Y., Leleu, A., Adibekyan, V., Lovis, C., Bossini, D., Sousa, S. G., Hara, N., Bouchy, F., Lavie, B., Rodrigues, J., da Silva, J. Gomes, Lillo-Box, J., Pepe, F. A., Tabernero, H. M., Osorio, M. R. Zapatero, Sozzetti, A., Mascareño, A. Suárez, Micela, G., Prieto, C. Allende, Cristiani, S., Damasso, M., Di Marcantonio, P., Ehrenreich, D., Faria, J., Figueira, P., Hernández, J. I. González, Jenkins, J., Lo Curto, G., Martins, C. J. A. P., Nunes, N. J., Pallé, E., Santos, N. C., Rebolo, R., Seager, S., Twicken, J. D., Udry, S., Vanderspek, R., Winn, J. N.
Publikováno v:
Barros, S. C. C.; Demangeon, O. D. S.; Alibert, Y.; Leleu, A.; Adibekyan, V.; Lovis, C.; Bossini, D.; Sousa, S. G.; Hara, N.; Bouchy, F.; Lavie, B.; Rodrigues, J.; da Silva, J. Gomes; Lillo-Box, J.; Pepe, F. A.; Tabernero, H. M.; Osorio, M. R. Zapatero; Sozzetti, A.; Mascareño, A. Suárez; Micela, G.; ... (2022). HD 23472: a multi-planetary system with three super-Earths and two potential super-Mercuries. Astronomy and astrophysics, 665, A154. EDP Sciences 10.1051/0004-6361/202244293
We report the characterisation of a multi-planetary system composed of five exoplanets orbiting the K-dwarf HD~23472 (TOI-174). In addition to the two super-Earths that were previously confirmed, we confirm and characterise three Earth-size planets i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::da0e2ef0f65e80ca5859b83f5f35f6c3
Autor:
Barros, S. C. C., Akinsanm, B., Bou��, G., Smith, A. M. S., Laskar, J., Ulmer-Moll, S., Lillo-Box, J., team, the CHEOPS
WASP-103b is the exoplanet with the highest expected deformation signature in its transit light curve and one of the shortest expected spiral-in times. Measuring the tidal deformation of the planet would allow us to estimate the second degree fluid L
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::410d95968504745ecb6d81912b18fe58
Autor:
Adibekyan, V., Santos, N. C., Demangeon, O. D. S., Faria, J. P., Barros, S. C. C., Oshagh, M., Figueira, P., Mena, E. Delgado, Sousa, S. G., Israelian, G., Campante, T., Hakobyan, A. A.
Revealing the mechanisms shaping the architecture of planetary systems is crucial for our understanding of their formation and evolution. In this context, it has been recently proposed that stellar clustering might be the key in shaping the orbital a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1769dea51814d59ba4d8d5a5569e45ae
Autor:
Damasso, M., Sozzetti, A., Lovis, C., Barros, S. C. C., Sousa, S. G., Demangeon, O. D. S., Faria, J. P., Lillo-Box, J., Cristiani, S., Pepe, F., Rebolo, R., Santos, N. C., Osorio, M. R. Zapatero, Hern��ndez, J. I. Gonz��lez, Amate, M., Pasquini, L., Zerbi, F. M., Adibekyan, V., Abreu, M., Affolter, M., Alibert, Y., Aliverti, M., Allart, R., Prieto, C. Allende, ��lvarez, D., Alves, D., Avila, G., Baldini, V., Bandy, T., Benz, W., Bianco, A., Borsa, F., Bossini, D., Bourrier, V., Bouchy, F., Broeg, C., Cabral, A., Calderone, G., Cirami, R., Coelho, J., Conconi, P., Coretti, I., Cumani, C., Cupani, G., D'Odorico, V., Deiries, S., Dekker, H., Delabre, B., Di Marcantonio, P., Dumusque, X., Ehrenreich, D., Figueira, P., Fragoso, A., Genolet, L., Genoni, M., Santos, R. G��nova, Hughes, I., Iwert, O., Kerber, F., Knudstrup, J., Landoni, M., Lavie, B., Lizon, J. -L., Curto, G. Lo, Maire, C., Martins, C. J . A. P., M��gevand, D., Mehner, A., Micela, G., Modigliani, A., Molaro, P., Monteiro, M. A., Monteiro, M. J. P. F. G., Moschetti, M., Mueller, E., Murphy, M. T., Nunes, N., Oggioni, L., Oliveira, A., Oshagh, M., Pall��, E., Pariani, G., Poretti, E., Rasilla, J. L., Rebord��o, J., Redaelli, E. M., Riva, M., Tschudi, S. Santana, Santin, P., Santos, P., S��gransan, D., Schmidt, T. M., Segovia, A., Sosnowska, D., Span��, P., Mascare��o, A. Su��rez, Tabernero, H., Tenegi, F., Udry, S., Zanutta, A.
The bright star $��$ Men was chosen as the first target for a radial velocity follow-up to test the performance of ESPRESSO, the new high-resolution spectrograph at the ESO's Very-Large Telescope (VLT). The star hosts a multi-planet system (a tra
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a9e9312350108966d2c2d00d34cc20a2
Autor:
Santerne, A., Malavolta, L., Kosiarek, M. R., Dai, F., Dressing, C. D., Dumusque, X., Hara, N. C., Lopez, T. A., Mortier, A., Vanderburg, A., Adibekyan, V., Armstrong, D. J., Barrado, D., Barros, S. C. C., Bayliss, D., Berardo, D., Boisse, I., Bonomo, A. S., Bouchy, F., Brown, D. J. A., Buchhave, L. A., Butler, R. P., Cameron, A. Collier, Cosentino, R., Crane, J. D., Crossfield, I. J. M., Damasso, M., Deleuil, M. R., Mena, E. Delgado, Demangeon, O., Díaz, R. F., Donati, J. -F., Figueira, P., Fulton, B. J., Ghedina, A., Harutyunyan, A., Hébrard, G., Hirsch, L. A., Hojjatpanah, S., Howard, A. W., Isaacson, H., Latham, D. W., Lillo-Box, J., López-Morales, M., Lovis, C., Fiorenzano, A. F. Martinez, Molinari, E., Mousis, O., Moutou, C., Nava, C., Nielsen, L. D., Osborn, H. P., Petigura, E. A., Phillips, D. F., Pollacco, D. L., Poretti, E., Rice, K., Santos, N. C., Ségransan, D., Shectman, S. A., Sinukoff, E., Sousa, S. G., Sozzetti, A., Teske, J. K., Udry, S., Vigan, A., Wang, S. X., Watson, C. A., Weiss, L. M., Wheatley, P. J., Winn, J. N.
Transiting extrasolar planets are key objects in the study of the formation, migration, and evolution of planetary systems. In particular, the exploration of the atmospheres of giant planets, through transmission spectroscopy or direct imaging, has r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1b675ade6eac05cdaa1ec48dbb90d5f0
Autor:
Rey, J., Bouchy, F., Stalport, M., Deleuil, M., Hébrard, G., Almenara, J. M., Alonso, R., Barros, S. C. C., Bonomo, A., Cazalet, G., Delisle, J. B., Díaz, R. F., Fridlund, M., Guenther, E. W., Guillot, T., Montagnier, G., Moutou, C., Lovis, C., Queloz, D., Santerne, A., Udry, S.
We report the discovery of an additional substellar companion in the CoRoT-20 system based on six years of HARPS and SOPHIE radial velocity follow-up. CoRoT-20 c has a minimum mass of 17 $\pm$ 1 $M_{Jup}$ and it orbits the host star in 4.59$\pm 0.05$
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8fcf1209a46e1bc3df409259da08ca20
With only two functional reaction wheels, Kepler cannot maintain stable pointing at its original target field and entered a new mode of observation called K2. Our method is based on many years of experience in planet hunting for the CoRoT mission. Du
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::57b6cdb5780a9267e984c25932c87654
Autor:
Smalley, B., Southworth, J., Pintado, O. I., Gillon, M., Holdsworth, D. L., Anderson, D. R., Barros, S. C. C., Cameron, A. Collier, Delrez, L., Faedi, F., Haswell, C. A., Hellier, C., Horne, K., Jehin, E., Maxted, P. F. L., Norton, A. J., Pollacco, D., Skillen, I., Smith, A. M. S., West, R. G., Wheatley, P. J.
The results of a search for eclipsing Am star binaries using photometry from the SuperWASP survey are presented. The light curves of 1742 Am stars fainter than V = 8.0 were analysed for the presences of eclipses. A total of 70 stars were found to exh
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::236e94bd5586ae0b1e4746769298f6a0