Zobrazeno 1 - 10
of 380
pro vyhledávání: '"Csizmadia, S."'
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.
Publikováno v:
A&A 671, A154 (2023)
The planetary system around the naked-eye star $\nu^2$ 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 rad
Externí odkaz:
http://arxiv.org/abs/2302.01853
Autor:
Morgado, B. E., Bruno, G., Gomes-Júnior, A. R., Pagano, I., Sicardy, B., Fortier, A., Desmars, J., Maxted, P. F. L., Braga-Ribas, F., Queloz, D., Sousa, S. G., Ortiz, J. L., Brandeker, A., Cameron, A. Collier, Pereira, C. L., Florén, H. G., Hara, N., Souami, D., Isaak, K. G., Olofsson, G., Santos-Sanz, P., Wilson, T. G., Broughton, J., Alibert, Y., Alonso, R., Anglada, G., Bárczy, T., Barrado, D., Barros, S. C. C., Baumjohann, W., Beck, M., Beck, T., Benz, W., Billot, N., Bonfils, X., Broeg, C., Cabrera, J., Charnoz, S., Csizmadia, S., Davies, M. B., Deleuil, M., Delrez, L., Demangeon, O. D. S., Demory, B. O., Ehrenreich, D., Erikson, A., Fossati, L., Fridlund, M., Gandolfi, D., Gillon, M., Güdel, M., Heng, K., Hoyer, S., Kiss, L. L., Laskar, J., Etangs, A. Lecavelier des, Lendl, M., Lovis, C., Magrin, D., Marafatto, L., Nascimbeni, V., Ottensamer, R., Pallé, E., Peter, G., Piazza, D., Piotto, G., Pollacco, D., Ragazzoni, R., Rando, N., Ratti, F., Rauer, H., Reimers, C., Ribas, I., Santos, N. C., Scandariato, G., Ségransan, D., Simon, A. E., Smith, A. M. S., Steller, M., Szabó, G. M., Thomas, N., Udry, S., Van Grootel, V., Walton, N. A., Westerdorff, K.
Publikováno v:
A&A 664, L15 (2022)
Stellar occultation is a powerful technique that allows the determination of some physical parameters of the occulting object. The result depends on the photometric accuracy, the temporal resolution, and the number of chords obtained. Space telescope
Externí odkaz:
http://arxiv.org/abs/2208.06204
Autor:
Van Eylen, Vincent, Astudillo-Defru, N., Bonfils, X., Livingston, J., Hirano, T., Luque, R., Lam, K. W. F., Justesen, A. B., Winn, J. N., Gandolfi, D., Nowak, G., Palle, E., Albrecht, S., Dai, F., Estrada, B. Campos, Owen, J. E., Foreman-Mackey, D., Fridlund, M., Korth, J., Mathur, S., Forveille, T., Mikal-Evans, T., Osborne, H. L. M., Ho, C. S. K., Almenara, J. M., Artigau, E., Barragán, O., Barros, S. C. C., Bouchy, F., Cabrera, J., Caldwell, D. A., Charbonneau, D., Chaturvedi, P., Cochran, W. D., Csizmadia, S., Damasso, M., Delfosse, X., De Medeiros, J. R., Díaz, R. F., Doyon, R., Esposito, M., Fűrész, G., Figueira, P., Georgieva, I., Goffo, E., Grziwa, S., Guenther, E., Hatzes, A. P., Jenkins, J. M., Kabath, P., Knudstrup, E., Latham, D. W., Lavie, B., Lovis, C., Mennickent, R. E., Mullally, S. E., Murgas, F., Narita, N., Pepe, F. A., Persson, C. M., Redfield, S., Ricker, G. R., Santos, N. C., Seager, S., Serrano, L. M., Smith, A. M. S., Mascareño, A. Suárez, Subjak, J., Twicken, J. D., Udry, S., Vanderspek, R., Osorio, M. R. Zapatero
We report on precise Doppler measurements of L231-32 (TOI-270), a nearby M dwarf ($d=22$ pc, $M_\star = 0.39$ M$_\odot$, $R_\star = 0.38$ R$_\odot$), which hosts three transiting planets that were recently discovered using data from the Transiting Ex
Externí odkaz:
http://arxiv.org/abs/2101.01593
Autor:
Esposito, M., Armstrong, D. J., Gandolfi, D., Adibekyan, V., Fridlund, M., Santos, N. C., Livingston, J. H., Mena, E. Delgado, Fossati, L., Lillo-Box, J., Barragán, O., Barrado, D., Cubillos, P. E., Cooke, B., Justesen, A. B., Meru, F., Díaz, R. F., Dai, F., Nielsen, L. D., Persson, C. M., Wheatley, P. J., Hatzes, A. P., Van Eylen, V., Musso, M. M., Alonso, R., Beck, P., Barros, S. C. C., Bayliss, D., Bonomo, A. S., Bouchy, F., Brown, D. J. A., Bryant, E., Cabrera, J., Cochran, W. D., Csizmadia, S., Deeg, H., Demangeon, O., Deleuil, M., Dumusque, X., Eigmüller, P., Endl, M., Erikson, A., Faedi, F., Figueira, P., Fukui, A., Grziwa, S., Guenther, E. W., Hidalgo, D., Hjorth, M., Hirano, T., Hojjatpanah, S., Knudstrup, E., Korth, J., Lam, K. W. F., de Leon, J., Lund, M. N., Luque, R., Mathur, S., Rodríguez, P. Montañés, Narita, N., Nespral, D., Niraula, P., Nowak, G., Osborn, H. P., Pallé, E., Pätzold, M., Pollacco, D., Prieto-Arranz, J., Rauer, H., Redfield, S., Ribas, I., Sousa, S. G., Smith, A. M. S., Tala-Pinto, M., Udry, S., Winn, J. N.
Publikováno v:
A&A 623, A165 (2019)
We report on the confirmation and mass determination of a transiting planet orbiting the old and inactive G7 dwarf star HD219666 (Mstar = 0.92 +/- 0.03 MSun, Rstar = 1.03 +/- 0.03 RSun, tau_star = 10 +/- 2 Gyr). With a mass of Mb = 16.6 +/- 1.3 MEart
Externí odkaz:
http://arxiv.org/abs/1812.05881
Autor:
Van Eylen, V., Dai, F., Mathur, S., Gandolfi, D., Albrecht, S., Fridlund, M., García, R. A., Guenther, E., Hjorth, M., Justesen, A. B., Livingston, J., Lund, M. N., Hernández, F. Pérez, Prieto-Arranz, J., Regulo, C., Bugnet, L., Everett, M. E., Hirano, T., Nespral, D., Nowak, G., Palle, E., Aguirre, V. Silva, Trifonov, T., Winn, J. N., Barragán, O., Beck, P. G., Chaplin, W. J., Cochran, W. D., Csizmadia, S., Deeg, H., Endl, M., Heeren, P., Grziwa, S., Hatzes, A. P., Hidalgo, D., Korth, J., Mathis, S., Rodriguez, P. Montañes, Narita, N., Patzold, M., Persson, C. M., Rodler, F., Smith, A. M. S.
We report the discovery and characterization of HD 89345b (K2-234b; EPIC 248777106b), a Saturn-sized planet orbiting a slightly evolved star. HD 89345 is a bright star ($V = 9.3$ mag) observed by the K2 mission with one-minute time sampling. It exhib
Externí odkaz:
http://arxiv.org/abs/1805.01860
Autor:
Bordé, P., Bouchy, F., Deleuil, M., Cabrera, J., Jorda, L., Lovis, C., Csizmadia, S., Aigrain, S., Almenara, J. M., Alonso, R., Auvergne, M., Baglin, A., Barge, P., Benz, W., Bonomo, A. S., Bruntt, H., Carone, L., Carpano, S., Deeg, H., Dvorak, R., Erikson, A., Ferraz-Mello, S., Fridlund, M., Gandolfi, D., Gazzano, J. -C., Gillon, M., Guenther, E., Guillot, T., Guterman, P., Hatzes, A., Havel, M., Hébrard, G., Lammer, H., Léger, A., Mayor, M., Mazeh, T., Moutou, C., Pätzold, M., Pepe, F., Ollivier, M., Queloz, D., Rauer, H., Rouan, D., Samuel, B., Santerne, A., Schneider, J., Tingley, B., Udry, S., Weingrill, J., Wuchterl, G.
We report the discovery of CoRoT-8b, a dense small Saturn-class exoplanet that orbits a K1 dwarf in 6.2 days, and we derive its orbital parameters, mass, and radius. We analyzed two complementary data sets: the photometric transit curve of CoRoT-8b a
Externí odkaz:
http://arxiv.org/abs/1008.0325
Publikováno v:
Astron.Astrophys. 456 (2006) 131-139
The large majority of BL Lacertae objects belonging to the 1 Jy sample, the class prototype for radio-selected sources, are thought to emit most of their synchrotron power in the far IR band. Ironically, this spectral region is very sparsely sampled,
Externí odkaz:
http://arxiv.org/abs/astro-ph/0606219
Autor:
Hamilton, C. M., Herbst, W., Vrba, F. J., Ibrahimov, M. A., Mundt, R., Bailer-Jones, C. A. L., Filippenko, A. V., Li, W., Bejar, V. J. S., Abraham, P., Kun, M., Moor, A., Benko, J., Csizmadia, S., DePoy, D. L., Pogge, R. W., Marshall, J. L.
Publikováno v:
Astron.J.130:1896-1915,2005
We present results from the most recent (2002-2004) observing campaigns of the eclipsing system KH 15D, in addition to re-reduced data obtained at Van Vleck Observatory (VVO) between 1995 and 2000. Phasing nine years of photometric data shows substan
Externí odkaz:
http://arxiv.org/abs/astro-ph/0507578
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Akademický článek
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