Zobrazeno 1 - 10
of 273
pro vyhledávání: '"Dorn, C P"'
Autor:
Soares, B. M. T. B., Adibekyan, V., Mordasini, C., Deal, M., Sousa, S. G., Delgado-Mena, E., Santos, N. C., Dorn, C.
Throughout a planetary system's formation evolution, some of the planetary material may end up falling into the host star and be engulfed by it, leading to a potential variation of the stellar composition. The present study explores how planet engulf
Externí odkaz:
http://arxiv.org/abs/2411.13455
Autor:
Naponiello, L., Bonomo, A. S., Mancini, L., Steinmeyer, M. L., Biazzo, K., Polychroni, D., Dorn, C., Turrini, D., Lanza, A. F., Sozzetti, A., Desidera, S., Damasso, M., Collins, K. A., Carleo, I., Collins, K. I., Colombo, S., D'Arpa, M. C., Dumusque, X., Gonzalez, M., Guilluy, G., Lorenzi, V., Mantovan, G., Nardiello, D., Pinamonti, M., Schwarz, R. P., Singh, V., Watkins, C. N., Zingales, T.
We examined in depth the star BD+00 444 (GJ 105.5, TOI-2443; V = 9.5 mag; d = 23.9 pc), with the aim of characterizing and confirming the planetary nature of its small companion, the planet candidate TOI-2443.01, which was discovered by TESS. We moni
Externí odkaz:
http://arxiv.org/abs/2411.09417
Autor:
Adibekyan, V., Deal, M., Dorn, C., Dittrich, I., Soares, B. M. T. B., Sousa, S. G., Santos, N. C., Bitsch, B., Mordasini, C., Barros, S. C. C., Bossini, D., Campante, T. L., Mena, E. Delgado, Demangeon, O. D. S., Figueira, P., Moedas, N., Martirosyan, Zh., Israelian, G., Hakobyan, A. A.
Publikováno v:
A&A 692, A67 (2024)
The composition of rocky planets is strongly driven by the primordial materials in the protoplanetary disk, which can be inferred from the abundances of the host star. Understanding this compositional link is crucial for characterizing exoplanets. We
Externí odkaz:
http://arxiv.org/abs/2410.17984
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:
Caballero, J. A., Gonzalez-Alvarez, E., Brady, M., Trifonov, T., Ellis, T. G., Dorn, C., Cifuentes, C., Molaverdikhani, K., Bean, J. L., Boyajian, T., Rodriguez, E., Sanz-Forcada, J., Osorio, M. R. Zapatero, Abia, C., Amado, P. J., Anugu, N., Bejar, V. J. S., Davies, C. L., Dreizler, S., Dubois, F., Ennis, J., Espinoza, N., Farrington, C. D., Lopez, A. Garcia, Gardner, T., Hatzes, A. P., Henning, Th., Herrero, E., Herrero-Cisneros, E., Kaminski, A., Kasper, D., Klement, R., Kraus, S., Labdon, A., Lanthermann, C., Bouquin, J. -B. Le, Gonzalez, M. J. Lopez, Luque, R., Mann, A. W., Marfil, E., Monnier, J. D., Montes, D., Morales, J. C., Palle, E., Pedraz, S., Quirrenbach, A., Reffert, S., Reiners, A., Ribas, I., Rodriguez-Lopez, C., Schaefer, G., Schweitzer, A., Seifahrt, A., Setterholm, B. R., Shan, Y., Shulyak, D., Solano, E., Sreenivas, K. R., Stefansson, G., Stuermer, J., Tabernero, H. M., Tal-Or, L., Brummelaar, T. ten, Vanaverbeke, S., von Braun, K., Youngblood, A., Zechmeister, M.
Publikováno v:
A&A 665, A120 (2022)
The Gl 486 system consists of a very nearby, relatively bright, weakly active M3.5 V star at just 8 pc with a warm transiting rocky planet of about 1.3 R_Terra and 3.0 M_Terra that is ideal for both transmission and emission spectroscopy and for test
Externí odkaz:
http://arxiv.org/abs/2206.09990
Autor:
Adibekyan, V., Santos, N. C., Dorn, C., Sousa, S. G., Hakobyan, A. A., Bitsch, B., Mordasini, Ch., Barros, S. C. C., Mena, E. Delgado, Demangeon, O. D. S., Faria, J. P., Figueira, P., Soares, B. M. T. B., Israelian, G.
Because of their common origin, it was assumed that the composition of planet building blocks should, to a first order, correlate with stellar atmospheric composition, especially for refractory elements. In fact, information on the relative abundance
Externí odkaz:
http://arxiv.org/abs/2112.14512
Autor:
Silva, T. Azevedo, Demangeon, O. D. S., Barros, S. C. C., Armstrong, D. J., Otegi, J. F., Bossini, D., Mena, E. Delgado, Sousa, S. G., Adibekyan, V., Nielsen, L. D., Dorn, C., Lillo-Box, J., Santos, N. C., Hoyer, S., Stassun, K. G., Almenara, J. M., Bayliss, D., Barrado, D., Boisse, I., Brown, D. J. A., Díaz, R. F., Dumusque, X., Figueira, P., Hadjigeorghiou, A., Hojjatpanah, S., Mousis, O., Osborn, A., Santerne, A., Strøm, P. A., Udry, S., Wheatley, P. J.
Publikováno v:
A&A 657, A68 (2022)
Most of the currently known planets are small worlds with radii between that of the Earth and that of Neptune. The characterization of planets in this regime shows a large diversity in compositions and system architectures, with distributions hinting
Externí odkaz:
http://arxiv.org/abs/2111.08764
Autor:
Osborn, Ares, Armstrong, David J., Cale, Bryson, Brahm, Rafael, Wittenmyer, Robert A., Dai, Fei, Crossfield, Ian J. M., Bryant, Edward M., Adibekyan, Vardan, Cloutier, Ryan, Collins, Karen A., Mena, E. Delgado, Fridlund, Malcolm, Hellier, Coel, Howell, Steve B., King, George W., Lillo-Box, Jorge, Otegi, Jon, Sousa, S., Stassun, Keivan G., Matthews, Elisabeth C., Ziegler, Carl, Ricker, George, Vanderspek, Roland, Latham, David W., Seager, S., Winn, Joshua N., Jenkins, Jon M., Acton, Jack S., Addison, Brett C., Anderson, David R., Ballard, Sarah, Barrado, David, Barros, Susana C. C., Batalha, Natalie, Bayliss, Daniel, Barclay, Thomas, Benneke, Björn, Berberian Jr., John, Bouchy, Francois, Bowler, Brendan P., Briceño, César, Burke, Christopher J., Burleigh, Matthew R., Casewell, Sarah L., Ciardi, David, Collins, Kevin I., Cooke, Benjamin F., Demangeon, Olivier D. S., Díaz, Rodrigo F., Dorn, C., Dragomir, Diana, Dressing, Courtney, Dumusque, Xavier, Espinoza, Néstor, Figueira, P., Fulton, Benjamin, Furlan, E., Gaidos, E., Geneser, C., Gill, Samuel, Goad, Michael R., Gonzales, Erica J., Gorjian, Varoujan, Günther, Maximilian N., Helled, Ravit, Henderson, Beth A., Henning, Thomas, Hogan, Aleisha, Hojjatpanah, Saeed, Horner, Jonathan, Howard, Andrew W., Hoyer, Sergio, Huber, Dan, Isaacson, Howard, Jenkins, James S., Jensen, Eric L. N., Jordán, Andrés, Kane, Stephen R., Kidwell Jr., Richard C., Kielkopf, John, Law, Nicholas, Lendl, Monika, Lund, M., Matson, Rachel A., Mann, Andrew W., McCormac, James, Mengel, Matthew W., Morales, Farisa Y., Nielsen, Louise D., Okumura, Jack, Osborn, Hugh P., Petigura, Erik A., Plavchan, Peter, Pollacco, Don, Quintana, Elisa V., Raynard, Liam, Robertson, Paul, Rose, Mark E., Roy, Arpita, Reefe, Michael, Santerne, Alexandre, Santos, Nuno C., Sarkis, Paula, Schlieder, J., Schwarz, Richard P., Scott, Nicholas J., Shporer, Avi, Smith, A. M. S., Stibbard, C., Stockdale, Chris, Strøm, Paul A., Twicken, Joseph D., Tan, Thiam-Guan, Tanner, A., Teske, J., Tilbrook, Rosanna H., Tinney, C. G., Udry, Stephane, Villaseñor, Jesus Noel, Vines, Jose I., Wang, Sharon X., Weiss, Lauren M., West, Richard G., Wheatley, Peter J., Wright, Duncan J., Zhang, Hui, Zohrabi, F.
We present the bright (V$_{mag} = 9.12$), multi-planet system TOI-431, characterised with photometry and radial velocities. We estimate the stellar rotation period to be $30.5 \pm 0.7$ days using archival photometry and radial velocities. TOI-431b is
Externí odkaz:
http://arxiv.org/abs/2108.02310
Autor:
Otegi, J. F., Bouchy, F., Helled, R., Armstrong, D. J., Stalport, M., Stassun, K. G., Delgado-Mena, E., Santos, N. C., Collins, K., Gandhi, S., Dorn, C., Brogi, M., Fridlund, M., Osborn, H. P., Hoyer, S., Udry, S., Hojjatpanah, S., Nielsen, L. D., Dumusque, X., Adibekyan, V., Conti, D., Schwarz, R., Wang, G., Figueira, P., Lillo-Box, J., Díaz, R. F., Hadjigeorghiou, A., Bayliss, D., Strøm, P. A., Sousa, S. G., Barrado, D., Osborn, A., Barros, S. S. C., Brown, D. J. A., Eastman, J. D., Ciardi, D. R., Vanderburg, A., Goeke, R. F., Guerrero, N. M., Boyd, P. T., Caldwell, D. A., Henze, C. E., McLean, B., Ricker, G., Vanderspek, R., Latham, D. W., Seager, S., Winn, J., Jenkins, J. M.
Publikováno v:
A&A 653, A105 (2021)
The Transiting Exoplanet Survey Satellite (\textit{TESS}) mission was designed to perform an all-sky search of planets around bright and nearby stars. Here we report the discovery of two sub-Neptunes orbiting around the TOI 1062 (TIC 299799658), a V=
Externí odkaz:
http://arxiv.org/abs/2105.01945
Autor:
Cointepas, M., Almenara, J. M., Bonfils, X., Bouchy, F., Astudillo-Defru, N., Murgas, F., Otegi, J. F., Wyttenbach, A., Anderson, D. R., Artigau, E., Martins, B. L. Canto, Charbonneau, D., Collins, K. A., Collins, K. I., Correia, J-J., Curaba, S., Delboulbe, A., Delfosse, X., Diaz, R. F., Dorn, C., Doyon, R., Feautrier, P., Figueira, P., Forveille, T., Gaisne, G., Gan, T., Gluck, L., Helled, R., Hellier, C., Jocou, L., Kern, P., Lafrasse, S., Law, N., Leao, I. C., Lovis, C., Magnard, Y., Mann, A. W., Maurel, D., de Medeiros, J. R., Melo, C., Moulin, T., Pepe, F., Rabou, P., Rochat, S., Rodriguez, D. R., Roux, A., Santos, N. C., Segransan, D., Stadler, E., Ting, E. B., Twicken, J. D., Udry, S., Waalkes, W. C., West, R. G., Wunsche, A., Ziegler, C., Ricker, G., Vanderspek, R., Latham, D. W., Seager, S., Winn, J., Jenkins, J. M.
Publikováno v:
A&A 650, A145 (2021)
We present the confirmation of a new sub-Neptune close to the transition between super-Earths and sub-Neptunes transiting the M2 dwarf TOI- 269 (TIC 220479565, V = 14.4 mag, J = 10.9 mag, Rstar = 0.40 Rsun, Mstar = 0.39 Msun, d = 57 pc). The exoplane
Externí odkaz:
http://arxiv.org/abs/2104.14782