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pro vyhledávání: '"P. Coffinet"'
Akademický článek
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Autor:
Dubber, Sophie C., Mortier, Annelies, Rice, Ken, Nava, Chantanelle, Malavolta, Luca, Giles, Helen, Coffinet, Adrien, Charbonneau, David, Vanderburg, Andrew, Bonomo, Aldo S., Boschin, Walter, Buchhave, Lars A., Cameron, Andrew Collier, Cosentino, Rosario, Dumusque, Xavier, Ghedina, Adriano, Harutyunyan, Avet, Haywood, Raphaelle D., Latham, David, Lopez-Morales, Mercedes, Micela, Giusi, Molinari, Emilio, Pepe, Francesco A., Phillips, David, Piotto, Giampaolo, Poretti, Ennio, Sasselov, Dimitar, Sozzetti, Alessandro, Udry, Stephane
We present confirmation of the planetary nature of PH-2b, as well as the first mass estimates for the two planets in the Kepler-103 system. PH-2b and Kepler-103c are both long-period and transiting, a sparsely-populated category of exoplanet. We use
Externí odkaz:
http://arxiv.org/abs/1910.03518
Autor:
Mayo, Andrew W., Rajpaul, Vinesh M., Buchhave, Lars A., Dressing, Courtney D., Mortier, Annelies, Zeng, Li, Fortenbach, Charles D., Aigrain, Suzanne, Bonomo, Aldo S., Cameron, Andrew Collier, Charbonneau, David, Coffinet, Adrien, Cosentino, Rosario, Damasso, Mario, Dumusque, Xavier, Fiorenzano, A. F. Martinez, Haywood, Raphaëlle D., Latham, David W., López-Morales, Mercedes, Malavolta, Luca, Micela, Giusi, Molinari, Emilio, Pearce, Logan, Pepe, Francesco, Phillips, David, Piotto, Giampaolo, Poretti, Ennio, Rice, Ken, Sozzetti, Alessandro, Udry, Stephane
Publikováno v:
2019 AJ 158 4
Although several thousands of exoplanets have now been detected and characterized, observational biases have led to a paucity of long-period, low-mass exoplanets with measured masses and a corresponding lag in our understanding of such planets. In th
Externí odkaz:
http://arxiv.org/abs/1908.08585
Autor:
Cameron, A. Collier, Mortier, A., Phillips, D., Dumusque, X., Haywood, R. D., Langellier, N., Watson, C. A., Cegla, H. M., Costes, J., Charbonneau, D., Coffinet, A., Latham, D. W., Lopez-Morales, M., Malavolta, L., Maldonado, J., Micela, G., Milbourne, T., Molinari, E., Saar, S. H., Thompson, S., Buchschacher, N., Cecconi, M., Cosentino, R., Ghedina, A., Glenday, A., Li, M. Gonzalez C. -H., Lodi, M., Lovis, C., Pepe, F., Poretti, E., Rice, K., Sasselov, D., Sozzetti, A., Szentgyorgyi, A., Udry, S., Walsworth, R.
The time-variable velocity fields of solar-type stars limit the precision of radial-velocity determinations of their planets' masses, obstructing detection of Earth twins. Since 2015 July we have been monitoring disc-integrated sunlight in daytime us
Externí odkaz:
http://arxiv.org/abs/1904.12186
Autor:
Dumusque, X., Turner, O., Dorn, C., Eastman, J. D., Allart, R., Adibekyan, V., Sousa, S., Santos, N. C., Mordasini, C., Bourrier, V., Bouchy, F., Coffinet, A., Davies, M. D., Diaz, R. F., Fausnaugh, M. M., Glidden, A., Guerrero, N., Henze, C. E., Jenkins, J. M., Latham, D. W., Lovis, C., Mayor, M., Pepe, F., Quintana, E. V., Ricker, G. R., Rowden, P., Segransan, D., Mascareno, A. Suarez, Seager, S., Twicken, J . D., Udry, S., Vanderspek, R. K., Winn, J. N.
Publikováno v:
A&A, 627, A43 (2019)
TESS is revolutionising the search for planets orbiting bright and nearby stars. In sectors 3 and 4, TESS observed TOI-402 (TIC-120896927), a bright V=9.1 K1 dwarf also known as HD 15337, and found two transiting signals with period of 4.76 and 17.18
Externí odkaz:
http://arxiv.org/abs/1903.05419
Publikováno v:
A&A 624, A122 (2019)
The study of Earth-mass extrasolar planets via the radial-velocity technique and the measurement of the potential cosmological variability of fundamental constants call for very-high-precision spectroscopy at the level of $\updelta\lambda/\lambda<10^
Externí odkaz:
http://arxiv.org/abs/1903.01942
Autor:
Damasso, M., Zeng, L., Malavolta, L., Mayo, A., Sozzetti, A., Mortier, A., Buchhave, L. A., Vanderburg, A., Lopez-Morales, M., Bonomo, A. S., Cameron, A. C., Coffinet, A., Figueira, P., Latham, D. W., Mayor, M., Molinari, E., Pepe, F., Phillips, D. F., Poretti, E., Rice, K., Udry, S., Watson, C. A.
Publikováno v:
A&A 624, A38 (2019)
K2-36 is a K dwarf orbited by two small ($R_{\rm b}=1.43\pm0.08$ $R_\oplus$ and $R_{\rm c}=3.2\pm0.3$ $R_\oplus$), close-in ($a_{\rm b}$=0.022 AU and $a_{\rm c}$=0.054 AU) transiting planets discovered by Kepler/K2. They are representatives of two fa
Externí odkaz:
http://arxiv.org/abs/1902.01881
Autor:
Borsato, L., Malavolta, L., Piotto, G., Buchhave, L. A., Mortier, A., Rice, K., Cameron, A. C., Coffinet, A., Sozzetti, A., Charbonneau, D., Cosentino, R., Dumusque, X., Figueira, P., Latham, D. W., Lopez-Morales, M., Mayor, M., Micela, G., Molinari, E., Pepe, F., Phillips, D., Poretti, E., Udry, S., Watson, C.
We investigated the discrepancy between planetary mass determination using the transit timing variations (TTVs) and radial velocities (RVs), by analysing the multi-planet system Kepler-9. Despite being the first system characterised with TTVs, there
Externí odkaz:
http://arxiv.org/abs/1901.05471
Autor:
Kosiarek, Molly R., Blunt, Sarah, Lopez-Morales, Mercedes, Crossfield, Ian J. M., Sinukoff, Evan, Petigura, Erik A., Gonzales, Erica J., Poretti, Ennio, Malavolta, Luca, Howard, Andrew W., Isaacson, Howard, Haywood, Raphaelle D., Ciardi, David R., Bristow, Makennah, Cameron, Andrew Collier, Charbonneau, David, Dressing, Courtney D., Figueira, Pedro, Fulton, Benjamin J., Hardee, Bronwen J., Hirsch, Lea A., Latham, David W., Mortier, Annelies, Nava, Chantanelle, Schlieder, Joshua E., Vanderburg, Andrew, Weiss, Lauren, Bonomo, Aldo S., Bouchy, Francois, Buchhave, Lars A., Coffinet, Adrien, Damasso, Mario, Dumusque, Xavier, Lovis, Christophe, Mayor, Michel, Micela, Giusi, Molinari, Emilio, Pepe, Francesco, Phillips, David, Piotto, Giampaolo, Rice, Ken, Sasselov, Dimitar, Segransan, Damien, Sozzetti, Alessandro, Udry, Stephane, Watson, Chris
Publikováno v:
AJ 157, 116 (2019)
K2-291 (EPIC 247418783) is a solar-type star with a radius of R_star = 0.899 $\pm$ 0.034 R_sun and mass of M_star=0.934 $\pm$ 0.038 M_sun. From K2 C13 data, we found one super-Earth planet (R_p = 1.589+0.095-0.072 R_Earth) transiting this star on a s
Externí odkaz:
http://arxiv.org/abs/1901.04558
Publikováno v:
A&A 629, A27 (2019)
(abridged) Even if the HARPS spectrograph has been operational for more than 15 years and it provides among the most precise Doppler measurements, improvements are still possible. One known problem, for instance, is the non-fully regular block-stitch
Externí odkaz:
http://arxiv.org/abs/1901.03294