Zobrazeno 1 - 10
of 531
pro vyhledávání: '"Marmier, P."'
Autor:
Anderson, Richard I., Viviani, Giordano, Shetye, Shreeya S., Mowlavi, Nami, Eyer, Laurent, Palaversa, Lovro, Holl, Berry, Blanco-Cuaresma, Sergi, Kravchenko, Kateryna, Pawlak, Michał, Reyes, Mauricio Cruz, Khan, Saniya, Netzel, Henryka E., Löbling, Lisa, Pápics, Péter I., Postel, Andreas, Roelens, Maroussia, Spetsieri, Zoi T., Thoul, Anne, Zák, Jiří, Bonvin, Vivien, Martin, David V., Millon, Martin, Saesen, Sophie, Wyttenbach, Aurélien, Figueira, Pedro, Marmier, Maxime, Prins, Saskia, Raskin, Gert, van Winckel, Hans
Publikováno v:
A&A 686, A177 (2024)
This first VELOCE data release comprises 18,225 high-precision RV measurements of 258 bona fide classical Cepheids on both hemispheres collected mainly between 2010 and 2022, alongside 1161 additional observations of 164 other stars. The median per-o
Externí odkaz:
http://arxiv.org/abs/2404.12280
Autor:
Hagelberg, J., Nielsen, L. D., Attia, O., Bourrier, V., Pearce, L., Venturini, J., Winn, J. N., Bouchy, F., Bouma, L. G., Briceño, C., Collins, K. A., Davis, A. B., Eastman, J. D., Evans, P., Grieves, N., Guerrero, N. M., Hellier, C., Jones, M. I., Latham, D. W., Law, N., Mann, A. W., Marmier, M., Ottoni, G., Radford, D. J., Restori, N., Rudat, A., Santos, L. Dos, Seager, S., Stassun, K., Stockdale, C., Udry, S., Wang, Songhu, Ziegler, C.
Publikováno v:
A&A 679, A70 (2023)
We report the discovery of a hot Jupiter on a 3.28-day orbit around a 1.08 M$_{Sun}$ G0 star that is the secondary component in a loose binary system. Based on follow-up radial velocity observations of TOI-858 B with CORALIE on the Swiss 1.2 m telesc
Externí odkaz:
http://arxiv.org/abs/2309.11390
Autor:
Barbato, D., Ségransan, D., Udry, S., Unger, N., Bouchy, F., Lovis, C., Mayor, M., Pepe, F., Queloz, D., Santos, N. C., Delisle, J. B., Figueira, P., Marmier, M., Matthews, E. C., Curto, G. Lo, Venturini, J., Chaverot, G., Cretignier, M., Otegi, J. F., Stalport, M.
Publikováno v:
A&A 674, A114 (2023)
A historical planet-search on a sample of 1647 nearby southern main sequence stars has been ongoing since 1998 with the CORALIE spectrograph at La Silla Observatory, with a backup subprogram dedicated to the monitoring of binary stars. We review 25 y
Externí odkaz:
http://arxiv.org/abs/2303.16717
Autor:
Pezzotti, C., Ottoni, G., Buldgen, G., Lyttle, A., Eggenberger, P., Udry, S., Ségransan, D., Mayor, M., Lovis, C., Marmier, M., Miglio, A., Elsworth, Y., Davies, G. R., Ball, W. H.
Context. Increasing the number of detected exoplanets is far from anecdotal, especially for long-period planets that require a long duration of observation. More detections imply a better understanding of the statistical properties of exoplanet popul
Externí odkaz:
http://arxiv.org/abs/2201.01553
Autor:
Ottoni, G., Udry, S., Ségransan, D., Buldgen, G., Lovis, C., Eggenberger, P., Pezzotti, C., Adibekyan, V., Marmier, M., Mayor, M., Santos, N. C., Sousa, S. G., Lagarde, N., Charbonnel, C.
Publikováno v:
A&A 657, A87 (2022)
Context. Following the first discovery of a planet orbiting a giant star in 2002, we started the CORALIE radial-velocity search for companions around evolved stars (CASCADES). We present the observations of three stars conducted at the 1.2 m Leonard
Externí odkaz:
http://arxiv.org/abs/2201.01528
Autor:
Barragán, O., Armstrong, D. J., Gandolfi, D., Carleo, I., Vidotto, A. A., D'Angelo, C. Villarreal, Oklopčić, A., Isaacson, H., Oddo, D., Collins, K., Fridlund, M., Sousa, S. G., Persson, C. M., Hellier, C., Howell, S., Howard, A., Redfield, S., Eisner, N., Georgieva, I. Y., Dragomir, D., Bayliss, D., Nielsen, L. D., Klein, B., Aigrain, S., Zhang, M., Teske, J., Twicken, J D., Jenkins, J., Esposito, M., Van Eylen, V., Rodler, F., Adibekyan, V., Alarcon, J., Anderson, D. R., Murphy, J. M. Akana, Barrado, D., Barros, S. C. C., Benneke, B., Bouchy, F., Bryant, E. M., Butler, P., Burt, J., Cabrera, J., Casewell, S., Chaturvedi, P., Cloutier, R., Cochran, W. D., Crane, J., Crossfield, I., Crouzet, N., Collins, K. I., Dai, F., Deeg, H. J., Deline, A., Demangeon, O. D. S., Dumusque, X., Figueira, P., Furlan, E., Gnilka, C., Goad, M. R., Goffo, E., Gutiérrez-Canales, F., Hadjigeorghiou, A., Hartman, Z., Hatzes, A. P., Harris, M., Henderson, B., Hirano, T., Hojjatpanah, S., Hoyer, S., Kabáth, P., Korth, J., Lillo-Box, J., Luque, R., Marmier, M., Močnik, T., Muresan, A., Murgas, F., Nagel, E., Osborne, H. L. M., Osborn, A., Osborn, H. P., Palle, E., Raimbault, M., Ricker, G. R., Rubenzahl, R A., Stockdale, C., Santos, N. C., Scott, N., Schwarz, R. P., Shectman, S., Seager, S., Ségransan, D., Serrano, L. M., Skarka, M., Smith, A. M. S., Šubjak, J., Tan, T. G., Udry, S., Watson, C., Wheatley, P. J., West, R., Winn, J. N., Wang, S. X., Wolfgang, A., Ziegler, C.
We present the discovery and characterisation of two transiting planets observed by \textit{TESS} in the light curves of the young and bright (V=9.67) star HD73583 (TOI-560). We perform an intensive spectroscopic and photometric space- and ground-bas
Externí odkaz:
http://arxiv.org/abs/2110.13069
Autor:
Unger, N., Ségransan, D., Queloz, D., Udry, S., Lovis, C., Mordasini, C., Ahrer, E., Benz, W., Bouchy, F., Delisle, J. -B., Díaz, R. F., Dumusque, X., Curto, G. Lo, Marmier, M., Mayor, M., Pepe, F., Santos, N. C., Stalport, M., Alonso, R., Cameron, A. Collier, Deleuil, M., Figueira, P., Gillon, M., Moutou, C., Pollacco, D., Pompei, E.
Publikováno v:
A&A 654, A104 (2021)
Context. We present precise radial-velocity measurements of five solar-type stars observed with the HARPS Echelle spectrograph mounted on the 3.6-m telescope in La Silla (ESO, Chile). With a time span of more than 10 years and a fairly dense sampling
Externí odkaz:
http://arxiv.org/abs/2108.10198
Publikováno v:
BMC Geriatrics, Vol 23, Iss 1, Pp 1-17 (2023)
Abstract During the COVID-19 pandemic and compared to other population groups, older people were at a heightened risk of developing lethal disease symptoms. Thus, many countries put in place protective measures to protect this “at-risk” populatio
Externí odkaz:
https://doaj.org/article/d13fcae126b44320a319314a12c21b84
Autor:
Teske, Johanna, Díaz, Matías R., Luque, Rafael, Močnik, Teo, Seidel, Julia V., Otegi, Jon Fernández, Feng, Fabo, Jenkins, James S., Pallè, Enric, Ségransan, Damien, Udry, Stèphane, Collins, Karen A., Eastman, Jason D., Ricker, George R., Vanderspek, Roland, Latham, David W., Seager, Sara, Winn, Joshua N., Jenkins, Jon M., Anderson, David. R., Barclay, Thomas, Bouchy, François, Burt, Jennifer A., Butler, R. Paul, Caldwell, Douglas A., Collins, Kevin I., Crane, Jeffrey D., Dorn, Caroline, Flowers, Erin, Haldemann, Jonas, Helled, Ravit, Hellier, Coel, Jensen, Eric L. N., Kane, Stephen R., Law, Nicholas, Lissauer, Jack J., Mann, Andrew W., Marmier, Maxime, Nielsen, Louise Dyregaard, Rose, Mark E., Shectman, Stephen A., Shporer, Avi, Torres, Guillermo, Wang, Sharon X., Wolfgang, Angie, Wong, Ian, Ziegler, Carl
The Transiting Exoplanet Survey Satellite mission was designed to find transiting planets around bright, nearby stars. Here we present the detection and mass measurement of a small, short-period ($\approx\,4$\,days) transiting planet around the brigh
Externí odkaz:
http://arxiv.org/abs/2007.13927
Autor:
Kane, Stephen R., Yalçınkaya, Selçuk, Osborn, Hugh P., Dalba, Paul A., Nielsen, Louise D., Vanderburg, Andrew, Močnik, Teo, Hinkel, Natalie R., Ostberg, Colby, Esmer, Ekrem Murat, Udry, Stéphane, Fetherolf, Tara, Baştürk, Özgür, Ricker, George R., Vanderspek, Roland, Latham, David W., Seager, Sara, Winn, Joshua N., Jenkins, Jon M., Allart, Romain, Bailey, Jeremy, Bean, Jacob L., Bouchy, Francois, Butler, R. Paul, Campante, Tiago L., Carter, Brad D., Daylan, Tansu, Deleuil, Magali, Diaz, Rodrigo F., Dumusque, Xavier, Ehrenreich, David, Horner, Jonathan, Howard, Andrew W., Isaacson, Howard, Jones, Hugh R. A., Kristiansen, Martti H., Lovis, Christophe, Marcy, Geoffrey W., Marmier, Maxime, O'Toole, Simon J., Pepe, Francesco, Ragozzine, Darin, Ségransan, Damien, Tinney, C. G., Turnbull, Margaret C., Wittenmyer, Robert A., Wright, Duncan J., Wright, Jason T.
Some of the most scientifically valuable transiting planets are those that were already known from radial velocity (RV) surveys. This is primarily because their orbits are well characterized and they preferentially orbit bright stars that are the tar
Externí odkaz:
http://arxiv.org/abs/2007.10995