Zobrazeno 1 - 10
of 656
pro vyhledávání: '"Doty J"'
Gliese 12 b: A temperate Earth-sized planet at 12 pc ideal for atmospheric transmission spectroscopy
Autor:
Kuzuhara, M., Fukui, A., Livingston, J. H., Caballero, J. A., de Leon, J. P., Hirano, T., Kasagi, Y., Murgas, F., Narita, N., Omiya, M., Orell-Miquel, Jaume, Palle, E., Changeat, Q., Esparza-Borges, E., Harakawa, H., Hellier, C., Hori, Yasunori, Ikuta, Kai, Ishikawa, H. T., Kodama, T., Kotani, T., Kudo, T., Morales, J. C., Mori, M., Nagel, E., Parviainen, H., Perdelwitz, V., Reiners, A., Ribas, I., Sanz-Forcada, J., Sato, B., Schweitzer, A., Tabernero, H. M., Takarada, T., Uyama, T., Watanabe, N., Zechmeister, M., García, N. Abreu, Aoki, W., Beichman, C., Béjar, V. J. S., Brandt, T. D., Calatayud-Borras, Y., Carleo, I., Charbonneau, D., Collins, K. A., Currie, T., Doty, J. P., Dreizler, S., Fernández-Rodríguez, G., Fukuda, I., Galán, D., Geraldía-González, S., González-Garcia, J., Hayashi, Y., Hedges, C., Henning, T., Hodapp, K., Ikoma, M., Isogai, K., Jacobson, S., Janson, M., Jenkins, J. M., Kagetani, T., Kambe, E., Kawai, Y., Kawauchi, K., Kokubo, E., Konishi, M., Korth, J., Krishnamurthy, V., Kurokawa, T., Kusakabe, N., Kwon, J., Laza-Ramos, A., Libotte, F., Luque, R., Madrigal-Aguado, A., Matsumoto, Y., Mawet, D., McElwain, M. W., Gallardo, P. P. Meni, Morello, G., Torres, S. Mu~noz, Nishikawa, J., Nugroho, S. K., Ogihara, M., Pel'aez-Torres, A., Rapetti, D., S'anchez-Benavente, M., Schlecker, M., Seager, S., Serabyn, E., Serizawa, T., Stangret, M., Takahashi, A., Teng, H., Tamura, M., Terada, Y., Ueda, A., Usuda, T., Vanderspek, R., Vievard, S., Watanabe, D., Winn, J. N., Osorio, M. R. Zapatero
Publikováno v:
Published on 2024 May 23 by Astrophysical Journal Letters (ApJL) 967 L21
Recent discoveries of Earth-sized planets transiting nearby M dwarfs have made it possible to characterize the atmospheres of terrestrial planets via follow-up spectroscopic observations. However, the number of such planets receiving low insolation i
Externí odkaz:
http://arxiv.org/abs/2405.14708
Autor:
Brady, M., Bean, J., Seifahrt, A., Kasper, D., Luque, R., Stefánsson, G., Stürmer, J., Charbonneau, D., Collins, K., Doty, J., Essack, Z., Fukui, A., Horta, F. Grau, Hedges, C., Hellier, C., Jenkins, J., Narita, N., Quinn, S., Shporer, A., Schwarz, R., Seager, S., Stassun, K., Striegel, S., Watkins, C., Winn, J., Zambelli, R.
M dwarf stars provide us with an ideal opportunity to study nearby small planets. The HUMDRUM (HUnting for M Dwarf Rocky planets Using MAROON-X) survey uses the MAROON-X spectrograph, which is ideally suited to studying these stars, to measure precis
Externí odkaz:
http://arxiv.org/abs/2405.10400
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:
Almenara, J. M., Bonfils, X., Otegi, J. F., Attia, O., Turbet, M., Astudillo-Defru, N., Collins, K. A., Polanski, A. S., Bourrier, V., Hellier, C., Ziegler, C., Bouchy, F., Briceño, C., Charbonneau, D., Cointepas, M., Collins, K. I., Crossfield, I., Delfosse, X., Díaz, R. F., Dorn, C., Doty, J. P., Forveille, T., Gaisné, G., Gan, T., Helled, R., Hesse, K., Jenkins, J. M., Jensen, E. L. N., Latham, D. W., Law, N., Mann, A. W., Mao, S., McLean, B., Murgas, F., Myers, G., Seager, S., Shporer, A., Tan, T. G., Twicken, J. D., Winn, J.
Publikováno v:
A&A 665, A91 (2022)
We report the detection of GJ 3090 b (TOI-177.01), a mini-Neptune on a 2.9-day orbit transiting a bright (K = 7.3 mag) M2 dwarf located at 22 pc. The planet was identified by the Transiting Exoplanet Survey Satellite and was confirmed with the High A
Externí odkaz:
http://arxiv.org/abs/2207.14121
Autor:
Hoyer, S., Gandolfi, D., Armstrong, D. J., Deleuil, M., Acuña, L., de Medeiros, J. R., Goffo, E., Lillo-Box, J., Mena, E. Delgado, Lopez, T. A., Santerne, A., Sousa, S., Fridlund, M., Adibekyan, V., Collins, K. A., Serrano, L. M., Cortés-Zuleta, P., Howell, S. B., Deeg, H., Aguichine, A., Barragán, O., Bryant, E. M., Martins, B. L. Canto, Collins, K. I., Cooke, B. F., Díaz, R. F., Esposito, M., Furlan, E., Hojjatpanah, S., Jackman, J., Jenkins, J. M., Jensen, E. L. N., Latham, D. W., Leão, I. C., Matson, R. A., Nielsen, L. D., Osborn, A., Otegi, J. F., Rodler, F., Sabotta, S., Scott, N. J., Seager, S., Stockdale, C., Strøm, P. A., Vanderspek, R., Van Eylen, V., Wheatley, P. J., Winn, J. N., Almenara, J. M., Barrado, D., Barros, S. C. C., Bayliss, D., Bouchy, F., Boyd, P. T., Cabrera, J., Cochran, W. D., Demangeon, O., Doty, J. P., Dumusque, X., Figueira, P., Fong, W., Grziwa, S., Hatzes, A. P., Kabáth, P., Knudstrup, E., Korth, J., Livingston, J. H., Luque, R., Mousis, O., Mullally, S. E., Osborn, H. P., Pallé, E., Persson, C. M., Redfield, S., Santos, N. C., Smith, J., Šubjak, J., Twicken, J. D., Udry, S., Yahalomi, D. A.
In this paper we report the discovery of TOI-220 $b$, a new sub-Neptune detected by the Transiting Exoplanet Survey Satellite (TESS) and confirmed by radial velocity follow-up observations with the HARPS spectrograph. Based on the combined analysis o
Externí odkaz:
http://arxiv.org/abs/2105.01944
Autor:
Parviainen, H., Palle, E., Zapatero-Osorio, M. R., Nowak, G., Fukui, A., Murgas, F., Narita, N., Stassun, K. G., Livingston, J. H., Collins, K. A., Soto, D. Hidalgo, Béjar, V. J. S., Korth, J., Monelli, M., Rodriguez, P. Montanes, Casasayas-Barris, N., Chen, G., Crouzet, N., de Leon, J. P., Hernandez, A., Kawauchi, K., Klagyivik, P., Kusakabe, N., Luque, R., Mori, M., Nishiumi, T., Prieto-Arranz, J., Tamura, M., Watanabe, N., Gan, T., Collins, K. I., Jensen, E. L. N., Barclay, T., Doty, J. P., Jenkins, J. M., Latham, D. W., Paegert, M., Ricker, G., Rodriguez, D. R., Seager, S., Shporer, A., Vanderspek, R., Villaseñor, J., Winn, J. N., Wohler, B., Wong, I.
Publikováno v:
A&A 645, A16 (2021)
Context: We report the discovery of TOI-519 b (TIC 218795833), a transiting substellar object (R = 1.07 RJup) orbiting a faint M dwarf (V = 17.35) on a 1.26 d orbit. Brown dwarfs and massive planets orbiting M dwarfs on short-period orbits are rare,
Externí odkaz:
http://arxiv.org/abs/2011.11458
Autor:
Younes, G., Baring, M. G., Kouveliotou, C., Arzoumanian, Z., Enoto, T., Doty, J., Gendreau, K. C., Göğüş, E., Guillot, S., Güver, T., Harding, A. K., Ho, W. C. G., van der Horst, A. J., Jaisawal, G. K., Kaneko, Y., LaMarr, B. J., Lin, L., Majid, W., Okajima, T., Pope, J., Ray, P. S., Roberts, O. J., Saylor, M., Steiner, J. F., Wadiasingh, Z.
Magnetars are young, magnetically-powered neutron stars possessing the strongest magnetic fields in the Universe. Fast Radio Bursts (FRBs) are extremely intense millisecond-long radio pulses of primarily extragalactic origin, and a leading attributio
Externí odkaz:
http://arxiv.org/abs/2006.11358