Zobrazeno 1 - 10
of 143
pro vyhledávání: '"Colon, K."'
Autor:
Carleo, I., Malavolta, L., Desidera, S., Nardiello, D., Wang, S., Turrini, D., Lanza, A. F., Baratella, M., Marzari, F., Benatti, S., Biazzo, K., Bieryla, A., Brahm, R., Bonavita, M., Collins, K. A., Hellier, C., Locci, D., Hobson, M. J., Maggio, A., Mantovan, G., Pinamonti, S. Messina M., Rodriguez, J. E., Sozzetti, A., Stassun, K., Wang, X. Y., Ziegler, C., Damasso, M., Giacobbe, P., Murgas, F., Parviainen, H., Andreuzzi, G., Barkaoui, K., Berlind, P., Bignamini, A., Borsa, F., Briceño, C., Brogi, M., Cabona, L., Calkins, M. L., Capuzzo-Dolcetta, R., Cecconi, M., Colon, K. D., Cosentino, R., Dragomir, D., Esquerdo, G. A., Henning, T., Ghedina, A., Goeke, R. F., Gratton, R., Horta, F. Grau, Gupta, A. F., Jenkins, J. M., Jordán, A., Knapic, C., Latham, D. W., Mireles, I., Law, N., Lorenzi, V., Lund, M. B., Maldonado, J., Mann, A. W., Molinari, E., Pallé, E., Paegert, M., Pedani, M., Quinn, S. N., Scandariato, G., Seager, S., Winn, J. N., Wohler, B., Zingales, T.
Context. Different theories have been developed to explain the origins and properties of close-in giant planets, but none of them alone can explain all of the properties of the warm Jupiters (WJs, Porb = 10 - 200 days). One of the most intriguing cha
Externí odkaz:
http://arxiv.org/abs/2311.11903
Hot planets around cool stars -- two short-period mini-Neptunes transiting the late K-dwarf TOI-1260
Autor:
Georgieva, I. Y., Persson, C. M., Barragán, O., Nowak, G., Fridlund, M., Locci, D., Palle, E., Luque, R., Carleo, I., Gandolfi, D., Kane, S. R., Korth, J., Stassun, K. G., Livingston, J., Matthews, E. C., Collins, K. A., Howell, S. B., Serrano, L. M., Albrecht, S., Bieryla, A., Brasseur, C. E., Ciardi, D., Cochran, W. D., Colon, K. D., Crossfield, I. J. M., Csizmadia, Sz., Deeg, H. J., Esposito, M., Furlan, E., Gan, T., Goffo, E., Gonzales, E., Grziwa, S., Guenther, E. . W., Guerra, P., Hirano, T., Jenkins, J. M., Jensen, E. L. N., Kabáth, P., Knudstrup, E., Lam, K. W. F., Latham, D. W., Levine, A. M., Matson, R. A., McDermott, S., Osborne, H. L. M., Paegert, M., Quinn, S. N ., Redfield, S., Ricker, G. R., Schlieder, J. E., Scott, N. J., Seager, S., Smith, A. M. S., Tenenbaum, P., Twicken, J. D., Vanderspek, R., Van Eylen, V., Winn, J. N.
We present the discovery and characterization of two sub-Neptunes in close orbits, as well as a tentative outer planet of a similar size, orbiting TOI-1260 - a low metallicity K6V dwarf star. Photometry from TESS yields radii of $R_{\rm b} = 2.33 \pm
Externí odkaz:
http://arxiv.org/abs/2104.05653
Autor:
Luque, R., Serrano, L. M., Molaverdikhani, K., Nixon, M. C., Livingston, J. H., Guenther, E. W., Pallé, E., Madhusudhan, N., Nowak, G., Korth, J., Cochran, W. D., Hirano, T., Chaturvedi, P., Goffo, E., Albrecht, S., Barragán, O., Briceño, C, Cabrera, J., Charbonneau, D., Cloutier, R., Collins, K. A., Collins, K. I., Colón, K. D., Crossfield, I. J. M., Csizmadia, Sz., Dai, F., Deeg, H. J., Esposito, M., Fridlund, M., Gandolfi, D., Georgieva, I., Glidden, A., Goeke, R. F., Grziwa, S., Hatzes, A. P., Henze, C. E., Howell, S. B., Irwin, J., Jenkins, J. M., Jensen, E. L. N., Kábath, P., Kidwell Jr., R. C., Kielkopf, J. F., Knudstrup, E., Lam, K. W. F., Latham, D. W., Lissauer, J. J., Mann, A. W., Matthews, E. C., Mireles, I., Narita, N., Paegert, M., Persson, C. M., Redfield, S., Ricker, G. R., Rodler, F., Schlieder, J. E., Scott, N. J., Seager, S., Šubjak, J., Tan, T. G., Ting, E. B., Vanderspek, R., Van Eylen, V., Winn, J. N., Ziegler, C.
Publikováno v:
A&A 645, A41 (2021)
We report the discovery and characterization of two transiting planets around the bright M1 V star LP 961-53 (TOI-776, J = 8.5 mag, M = 0.54+-0.03 Msun) detected during Sector 10 observations of the Transiting Exoplanet Survey Satellite (TESS). Combi
Externí odkaz:
http://arxiv.org/abs/2009.08338
Autor:
Airapetian, V. S., Adibekyan, V., Ansdell, M., Alexander, D., Bastian, T., Saikia, S. Boro, Brun, A. S., Cohen, O., Cuntz, M., Danchi, W., Davenport, J., DeNolfo, J., DeVore, R., Dong, C. F., Drake, J. J., France, K., Fraschetti, F., Herbst, K., Garcia-Sage, K., Gillon, M., Glocer, A., Grenfell, J. L., Gronoff, G., Gopalswamy, N., Guedel, M., Hartnett, H., Harutyunyan, H., Hinkel, N. R., Jensen, A. G., Jin, M., Johnstone, C., Kalas, P., Kane, S. R., Kay, C., Kitiashvili, I. N., Kochukhov, O., Kondrashov, D., Lazio, J., Leake, J., Li, G., Linsky, J., Lueftinger, T., Lynch, B., Lyra, W., Mandell, A. M., Mandt, K. E., Maehara, H., Miesch, M. S., Mickaelian, A. M., Mouchou, S., Notsu, Y., Ofman, L., Oman, L. D., Osten, R. A., Oran, R., Petre, R., Ramirez, R. M., Rau, G., Redfield, S., Réville, V., Rugheimer, S., Scheucher, M., Schlieder, J. E., Shibata, K., Schnittman, J. D., Soderblom, David, Strugarek, A., Turner, J. D., Usmanov, A., Der Holst, Van, Vidotto, A., Vourlidas, A., Way, M. J., Wolk, Zank, G. P., R., P. Zarka, Kopparapu, Babakhanova, S., Pevtsov, A. A., Lee, Y., Henning, W., Colón, K. D., Wolf, E. T.
The field of exoplanetary science is making rapid progress both in statistical studies of exoplanet properties as well as in individual characterization. As space missions provide an emerging picture of formation and evolution of exoplanetary systems
Externí odkaz:
http://arxiv.org/abs/1903.06853
Autor:
Bouma, L. G., Winn, J. N., Baxter, C., Bhatti, W., Dai, F., Daylan, T., Désert, J. -M., Hill, M. L., Kane, S. R., Stassun, K. G., Villasenor, J., Ricker, G. R., Vanderspek, R., Latham, D. W., Seager, S., Jenkins, J. M., Berta-Thompson, Z., Colón, K., Fausnaugh, M., Glidden, Ana, Guerrero, N., Rodriguez, J. E., Twicken, J. D., Wohler, B.
Publikováno v:
2019, AJ, 157, 217
The Transiting Exoplanet Survey Satellite (TESS) recently observed 18 transits of the hot Jupiter WASP-4b. The sequence of transits occurred 81.6 $\pm$ 11.7 seconds earlier than had been predicted, based on data stretching back to 2007. This is unlik
Externí odkaz:
http://arxiv.org/abs/1903.02573
Autor:
Kedziora-Chudczer, L., Zhou, G., Bailey, J., Bayliss, D. D. R., Tinney, C. G., Osip, D., Colon, K. D., Shporer, A., Dragomir, D.
We present new eclipse observations for one of the hottest "hot Jupiters" WASP-18b, for which previously published data from HST WFC3 and Spitzer have led to radically conflicting conclusions about the composition of this planet's atmosphere. We meas
Externí odkaz:
http://arxiv.org/abs/1812.10623
Autor:
Mallonn, M., von Essen, C., Herrero, E., Alexoudi, X., Granzer, T., Sosa, M., Strassmeier, K. G., Bakos, G., Bayliss, D., Brahm, R., Bretton, M., Campos, F., Carone, L., Colón, K. D., Dale, H. A., Dragomir, D., Espinoza, N., Evans, P., Garcia, F., Gu, S. -H., Guerra, P., Jongen, Y., Jordán, A., Kang, W., Keles, E., Kim, T., Lendl, M., Molina, D., Salisbury, M., Scaggiante, F., Shporer, A., Siverd, R., Sokov, E., Sokova, I., Wünsche, A.
Publikováno v:
A&A 622, A81 (2019)
Transit events of extrasolar planets offer a wealth of information for planetary characterization. However, for many known targets, the uncertainty of their predicted transit windows prohibits an accurate scheduling of follow-up observations. In this
Externí odkaz:
http://arxiv.org/abs/1812.05882
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
Autor:
Temple, L. Y., Hellier, C., Albrow, M. D., Anderson, D. R., Bayliss, D., Beatty, T. G., Bieryla, A., Brown, D. J. A., Cargile, P. A., Cameron, A. Collier, Collins, K. A., Colón, K. D., Curtis, I. A., D'Ago, G., Delrez, L., Eastman, J., Gaudi, B. S., Gillon, M., Gregorio, J., James, D., Jehin, E., Joner, M. D., Kielkopf, J. F., Kuhn, R. B., Labadie-Bartz, J., Latham, D. W., Lendl, M., Lund, M. B., Malpas, A. L., Maxted, P. F. L., Myers, G., Oberst, T. E., Pepe, F., Pepper, J., Pollacco, D., Queloz, D., Rodriguez, J. E., Ségransan, D., Siverd, R. J., Smalley, B., Stassun, K. G., Stevens, D. J., Stockdale, C., Tan, T. G., Triaud, A. H. M. J., Udry, S., Villanueva Jr, S., West, R. G., Zhou, G.
We report the joint WASP/KELT discovery of WASP-167b/KELT-13b, a transiting hot Jupiter with a 2.02-d orbit around a $V$ = 10.5, F1V star with [Fe/H] = 0.1 $\pm$ 0.1. The 1.5 R$_{\rm Jup}$ planet was confirmed by Doppler tomography of the stellar lin
Externí odkaz:
http://arxiv.org/abs/1704.07771
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