Zobrazeno 1 - 10
of 49
pro vyhledávání: '"Relles, H."'
Autor:
Mantovan, G., Wilson, T. G., Borsato, L., Zingales, T., Biazzo, K., Nardiello, D., Malavolta, L., Desidera, S., Marzari, F., Cameron, A. Collier, Nascimbeni, V., Majidi, F. Z., Montalto, M., Piotto, G., Stassun, K. G., Winn, J. N., Jenkins, J. M., Mignon, L., Bieryla, A., Latham, D. W., Barkaoui, K., Collins, K. A., Evans, P., Fausnaugh, M. M., Granata, V., Kostov, V., Mann, A. W., Pozuelos, F. J., Radford, D. J., Relles, H. M., Rowden, P., Seager, S., Tan, T. -G., Timmermans, M., Watkins, C. N.
Publikováno v:
A&A 691, A67 (2024)
Recent observations of giant planets have revealed unexpected bulk densities. Hot Jupiters, in particular, appear larger than expected for their masses compared to planetary evolution models, while warm Jupiters seem denser than expected. These diffe
Externí odkaz:
http://arxiv.org/abs/2409.07520
Autor:
Barkaoui, K., Schwarz, R. P., Narita, N., Mistry, P., Magliano, C., Hirano, T., Maity, M., Burgasser, A. J., Rackham, B. V., Murgas, F., Pozuelos, F. J., Stassun, K. G., Everett, M. E., Ciardi, D. R., Lamman, C., Pass, E. K., Bieryla, A., Aganze, C., Esparza-Borges, E., Collins, K. A., Covone, G., de Leon, J., D'evora-Pajares, M., de Wit, J., Fukuda, Izuru, Fukui, A., Gerasimov, R., Gillon, M., Hayashi, Y., Howell, S. B., Ikoma, M., Ikuta, K., Jenkins, J. M., Karpoor, P. R., Kawai, Y., Kimura, T., Kotani, T., Latham, D. W., Mori, M., Palle, E., Parviainen, H., Patel, Y. G., Ricker, G., Relles, H. M., Shporer, A., Seager, S., Softich, E., Srdoc, G., Tamura, M., Theissen, C. A., Twicken, J. D., Vanderspek, R., Watanabe, N., Watkins, C. N., Winn, J. N., Wohler, B.
One of the main goals of the NASA's TESS (Transiting Exoplanet Survey Satellite) mission is the discovery of Earth-like planets around nearby M-dwarf stars. Here, we present the discovery and validation of three new short-period Earth-sized planets o
Externí odkaz:
http://arxiv.org/abs/2405.06350
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:
Nielsen, L. D., Brahm, R., Bouchy, F., Espinoza, N., Turner, O., Rappaport, S., Pearce, L., Ricker, G., Vanderspek, R., Latham, D. W., Seager, S., Winn, J. N., Jenkins, J. M., Acton, J. S., Bakos, G., Barclay, T., Barkaoui, K., Bhatti, W., Briceño, C., Bryant, E. M., Burleigh, M. R., Ciardi, D. R., Collins, K. A., Collins, K. I., Cooke, B. F., Csubry, Z., Santos, L. A. dos, Eigmüller, Ph., Fausnaugh, M. M., Gan, T., Gillon, M., Goad, M. R., Guerrero, N., Hagelberg, J., Hart, R., Henning, T., Huang, C. X., Jehin, E., Jenkins, J. S., Jordàn, A., Kielkopf, J. F., Kossakowski, D., Lavie, B., Law, N., Lendl, M., de Leon, J. P., Lovis, C., Mann, A. W., Marmier, M., McCormac, J., Mori, M., Moyano, M., Narita, N., Osip, D., Otegi, J. F., Pepe, F., Pozuelos, F. J., Raynard, L., Relles, H. M., Sarkis, P., Segransan, D., Seidel, J. V., Shporer, A., Stalport, M., Stockdale, C., Suc, V., Tamura, M., Tan, T. G., Tilbrook, R. H., Ting, E. B., Trifonov, T., Udry, S., Vanderburg, A., Wheatley, P. J., Wingham, G., Zhan, Z., Ziegler, C.
Publikováno v:
A&A 639, A76 (2020)
We report the confirmation and mass determination of three hot Jupiters discovered by the Transiting Exoplanet Survey Satellite (TESS) mission: HIP 65Ab (TOI-129, TIC-201248411) is an ultra-short-period Jupiter orbiting a bright (V=11.1 mag) K4-dwarf
Externí odkaz:
http://arxiv.org/abs/2003.05932
Autor:
Astudillo-Defru, N., Cloutier, R., Wang, S. X., Teske, J., Brahm, R., Hellier, C., Ricker, G., Vanderspek, R., Latham, D., Seager, S., Winn, J. N., Jenkins, J. M., Collins, K. A., Stassun, K. G., Ziegler, C., Almenara, J. M., Anderson, D. R., Artigau, E., Bonfils, X., Bouchy, F., Briceño, C., Butler, R. P., Charbonneau, D., Conti, D. M., Crane, J., Crossfield, I. J . M., Davies, M., Delfosse, X., Díaz, R. F., Doyon, R., Dragomir, D., Eastman, J. D., Espinoza, N., Essack, Z., Feng, F., Figueira, P., Forveille, T., Gan, T., Glidden, A., Guerrero, N., Hart, R., Henning, Th., Horch, E. P., Isopi, G., Jenkins, J. S., Jordán, A., Kielkopf, J. F., Law, N., Lovis, C., Mallia, F., Mann, A. W., de Medeiros, J. R., Melo, C., Mennickent, R. E., Mignon, L., Murgas, F., Nusdeo, D. A., Pepe, F., Relles, H. M., Rose, M., Santos, N. C., Ségransan, D., Shectman, S., Shporer, A., Smith, J. C., Torres, P., Udry, S., Villasenor, J., Winters, J . G., Zhou, G.
Publikováno v:
A&A 636, A58 (2020)
We report the detection of a transiting super-Earth-sized planet (R=1.39+-0.09 Rearth) in a 1.4-day orbit around L 168-9 (TOI-134),a bright M1V dwarf (V=11, K=7.1) located at 25.15+-0.02 pc. The host star was observed in the first sector of the Trans
Externí odkaz:
http://arxiv.org/abs/2001.09175
Autor:
Zhou, G., Huang, C. X., Bakos, G. Á., Hartman, J. D., Latham, David W., Quinn, S. N., Collins, K. A., Winn, J. N., Wong, I., Kovács, G., Csubry, Z., Bhatti, W., Penev, K., Bieryla, A., Esquerdo, G. A., Berlind, P., Calkins, M. L., de Val-Borro, M., Noyes, R. W., Lázár, J., Papp, I., Sári, P., Kovács, T., Buchhave, Lars A., Szklenár, T., Beky, B., Johnson, M. C., Cochran, W. D., Kniazev, A. Y., Stassun, K. G., Fulton, B. J., Shporer, A., Espinoza, N., Bayliss, D., Everett, M., Howell, S. B., Hellier, C., Anderson, D. R., Cameron, A. Collier, West, R. G., Brown, D. J. A., Schanche, N., Barkaoui, K., Pozuelos, F., Gillon, M., Jehin, E., Benkhaldoun, Z., Daassou, A., Ricker, G., Vanderspek, R., Seager, S., Jenkins, J. M., Lissauer, Jack J., Armstrong, J. D., Collins, K. I., Gan, T., Hart, R., Horne, K., Kielkopf, J. F., Nielsen, L. D., Nishiumi, T., Narita, N., Palle, E., Relles, H. M., Sefako, R., Tan, T. G., Davies, M., Goeke, Robert F., Guerrero, N., Haworth, K., Villanueva, S.
Wide field surveys for transiting planets are well suited to searching diverse stellar populations, enabling a better understanding of the link between the properties of planets and their parent stars. We report the discovery of HAT-P-69b (TOI 625.01
Externí odkaz:
http://arxiv.org/abs/1906.00462
Autor:
Bakos, G. Á., Bayliss, D., Bento, J., Bhatti, W., Brahm, R., Csubry, Z., Espinoza, N., Hartman, J. D., Henning, Th., Jordán, A., Mancini, L., Penev, K., Rabus, M., Sarkis, P., Suc, V., de Val-Borro, M., Zhou, G., Butler, R. P., Crane, J., Durkan, S., Shectman, S., Kim, J., Lázár, J., Papp, I., Sári, P., Ricker, G., Vanderspek, R., Latham, D. W., Seager, S., Winn, J. N., Jenkins, J., Chacon, A. D., Fűrész, G., Goeke, B., Li, J., Quinn, S., Quintana, E. V., Tenenbaum, P., Teske, J., Vezie, M., Yu, L., Stockdale, C., Evans, P., Relles, H. M.
We report the discovery of HATS-71b, a transiting gas giant planet on a P = 3.7955 day orbit around a G = 15.35 mag M3 dwarf star. HATS-71 is the coolest M dwarf star known to host a hot Jupiter. The loss of light during transits is 4.7%, more than a
Externí odkaz:
http://arxiv.org/abs/1812.09406
Akademický článek
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Autor:
Jones, M. I., Brahm, R., Espinoza, N., Wang, S., Shporer, A., Henning, T., Jordan, A., Sarkis, P., Paredes, L. A., Hodari-Sadiki, J., Henry, T., Cruz, B., Nielsen, L. D., Bouchy, F., Pepe, F., Segransan, D., Turner, O., Udry, S., Bakos, G., Osip, D., Suc, V., Ziegler, C., Tokovinin, A., Law, N. M., Mann, A. W., Relles, H., Collins, K. A., Bayliss, D., Sedaghati, E., Latham, D. W., Seager, S., Winn, J. N., Jenkins, J. M., Smith, J. C., Davies, M., Tenenbaum, P., Dittmann, J., Vanderburg, A., Christiansen, J. L., Haworth, K., Doty, J., Furesz, G., Laughlin, G.
We report on the confirmation of a transiting giant planet around the relatively hot (Teff = 6801 $\pm$ 56 K) star HD2685, whose transit signal was detected in Sector 1 data of the TESS mission. We confirmed the planetary nature of the transit signal
Externí odkaz:
http://arxiv.org/abs/1811.05518
Autor:
Borkovits, T., Rappaport, S., Kaye, T., Isaacson, H., Vanderburg, A., Howard, A. W., Kristiansen, M. H., Omohundro, M. R., Schwengeler, H. M., Terentev, I. A., Shporer, A., Relles, H., Villanueva Jr., S., Tan, T. G., Colón, K. D., Blex, J., Haas, M., Cochran, W., Endl, M.
Using Campaign 15 data from the K2 mission, we have discovered a triply-eclipsing triple star system: EPIC 249432662. The inner eclipsing binary system has a period of 8.23 days, with shallow $\sim$3% eclipses. During the entire 80-day campaign, ther
Externí odkaz:
http://arxiv.org/abs/1809.04366