Zobrazeno 1 - 10
of 15 744
pro vyhledávání: '"Pepper, J. A"'
Autor:
Farrar, Lloyd P
Publikováno v:
The Grove Dictionary of American Music, 2 ed., 2013.
Autor:
Ulmer-Moll, S., Lendl, M., Gill, S., Villanueva, S., Hobson, M. J., Bouchy, F., Brahm, R., Dragomir, D., Grieves, N., Mordasini, C., Anderson, D. R., Acton, J. S., Bayliss, D., Bieryla, A., Burleigh, M. R., Casewell, S. L., Chaverot, G., Eigmüller, P., Feliz, D., Gaudi, S., Gillen, E., Goad, M. R., Gupta, A. F., Günther, M. N., Henderson, B. A., Henning, T., Jenkins, J. S., Jones, M., Jordán, A., Kendall, A., Latham, D. W., Mireles, I., Moyano, M., Nadol, J., Osborn, H. P., Pepper, J., Pinto, M. T., Psaridi, A., Queloz, D., Quinn, S., Rojas, F., Sarkis, P., Schlecker, M., Tilbrook, R. H., Torres, P., Trifonov, T., Udry, S., Vines, J. I., West, R., Wheatley, P., Yao, X., Zhao, Y., Zhou, G.
Publikováno v:
A&A 666, A46 (2022)
Long-period transiting planets provide the opportunity to better understand the formation and evolution of planetary systems. Their atmospheric properties remain largely unaltered by tidal or radiative effects of the host star, and their orbital arra
Externí odkaz:
http://arxiv.org/abs/2207.03911
In the search for life in the cosmos, NASA's Transiting Exoplanet Survey Satellite (TESS) mission has already monitored about 74% of the sky for transiting extrasolar planets, including potentially habitable worlds. However, TESS only observed a frac
Externí odkaz:
http://arxiv.org/abs/2101.07898
Akademický článek
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Autor:
Kaltenegger, L., Pepper, J.
Transit observations have found the majority of exoplanets to date. Spectroscopic observations of transits and eclipses are the most commonly used tool to characterize exoplanet atmospheres and will be used in the search for life. However, an exoplan
Externí odkaz:
http://arxiv.org/abs/2010.09766
Autor:
Zasche, P., Henzl, Z., Lehmann, H., Pepper, J., Powell, B. P., Kostov, V. B., Barclay, T., Wolf, M., Kucakova, H., Uhlar, R., Masek, M., Palafouta, S., Gazeas, K., Stassun, K. G., Gaudi, B. S., Rodriguez, J. E., Stevens, D. J.
Publikováno v:
2020A&A...642A..63Z
We report the discovery of the relatively bright (V = 10.5 mag), doubly eclipsing 2+2 quadruple system CzeV1731. This is the third known system of its kind, in which the masses are determined for all four stars and both the inner and outer orbits are
Externí odkaz:
http://arxiv.org/abs/2010.07699
Autor:
Benni, P., Burdanov, A. Y., Krushinsky, V. V., Bonfanti, A., Hébrard, G., Almenara, J. M., Dalal, S., Demangeon, O. D. S., Tsantaki, M., Pepper, J., Stassun, K. G., Vanderburg, A., Belinski, A., Kashaev, F., Barkaoui, K., Kim, T., Kang, W., Antonyuk, K., Dyachenko, V. V., Rastegaev, D. A., Beskakotov, A., Mitrofanova, A. A., Pozuelos, F. J., Kuznetsov, E. D., Popov, A., Kiefer, F., Wilson, P. A., Ricker, G., Vanderspek, R., Latham, D. W., Seager, S., Jenkins, J. M., Sokov, E., Sokova, I., Marchini, A., Papini, R., Salvaggio, F., Banfi, M., Baştürk, Ö., Torun, Ş., Yalçınkaya, S., Ivanov, K., Valyavin, G., Jehin, E., Gillon, M., Pakštienė, E., Hentunen, V. -P., Shadick, S., Bretton, M., Wünsche, A., Garlitz, J., Jongen, Y., Molina, D., Girardin, E., Horta, F. Grau, Naves, R., Benkhaldoun, Z., Joner, M. D., Spencer, M., Bieryla, A., Stevens, D. J., Jensen, E. L. N., Collins, K. A., Charbonneau, D., Quintana, E. V., Mullally, S. E., Henze, C. E.
We announce the discovery of GPX-1 b, a transiting brown dwarf with a mass of $19.7\pm 1.6$ $M_{\mathrm{Jup}}$ and a radius of $1.47\pm0.10$ $R_{\mathrm{Jup}}$, the first sub-stellar object discovered by the Galactic Plane eXoplanet (GPX) survey. The
Externí odkaz:
http://arxiv.org/abs/2009.11899
Autor:
Segura, N. Castro, Knigge, C., Acosta-Pulido, J. A., Altamirano, D., del Palacio, S., Santisteban, J. V. Hernandez, Pahari, M., Rodriguez-Gil, P., Belardi, C., Buckley, D. A. H., Burleigh, M. R., Childress, M., Fender, R. P., Hewitt, D. M., James, D. J., Kuhn, R. B., Kuin, N. P. M., Pepper, J., Ponomareva, A. A., Pretorius, M. L., Rodríguez, J. E., Stassun, K. G., Williams, D. R. A., Woudt, P. A.
V341 Ara was recently recognised as one of the closest (d ~ 150 pc) and brightest (V~ 10) nova-like cataclysmic variables. This unique system is surrounded by a bright emission nebula, likely to be the remnant of a recent nova eruption. Embedded with
Externí odkaz:
http://arxiv.org/abs/2008.07462
Autor:
Taggart, D., Ratnatunga, Westaby, S., Cook, J., Wallis, C., Wos, S., Jasinski, M., Deja, M., Widenka, K., Blach, A., Gocol, R., Hudziak, D., Zurek, P., Bachowski, R., Mrozek, R., Kargul, T., Domarardzki, W., Frackiewicz, J., Zamvar, V., Ezakadan, D., Buxton, B., Seevanayagam, S., Matalanis, G., Rosalion, A., Negri, J., Moten, S., Atkinson, V., Newcomb, A., Polidano, P., Pana, R., Gerbo, S., O'Keefe, P., von Oppell, U., Mehta, D., Azzu, A., Szafranek, A., Kulatilake, E., Evans, J., Martin, N., Banner, D., Trivedi, U., Forsyth, A., Hyde, J., Cohen, A., Lewis, M., Gardner, E., MacKenzie, A., Cooter, N., Joyce, E., Parker, J., Champney, F., Clark, S., Dark, J., Tocewicz, K., Pillay, T., Rowling, S., Adams-Hall, J., Bochenek, A., Cisowski, M., Bolkowski, M., Morawski, W., Guc, M., Krejca, M., Wilczynski, M., Duralek, A., Gerber, W., Skarysz, J., Shrestha, R., Swiech, W., Szmagala, X., Krzych, L., Pawlak, A., Kepa, K., Hasan, R., Keenan, D., Prendergast, B., Odom, N., McLaughlin, K., Cummings-Fosong, G., Mathew, C., Iles-Smith, H., Oomen, A., Desai, J., El-Gamel, A., John, L., Wendler, O., Andrews, M., Rance, K., Williams, R., Hogervorst, V., Gregory, J., Jessup, J., Knighton, A., Hoare, A., Ritchie, A., Choong, C., Nair, S., Sudarshan, C., Jenkins, D., Large, S., Barman, M., Dhital, K., Routledge, T., Rosengard, B., Munday, H., Rintoul, K., Jarrett, E., Lao-Sirieix, S., Wilkinson, A., Garner, L., Osmond, J., Holcombe, H., Cale, A., Griffin, S., Dickson, J., Spyt, T., Gershlick, A., Hickey, M., Sosnowski, A., Peek, G., Szostek, J., Hadjinikalaou, L., Logtens, E., Oakley, M., Leji, S., Gaer, J., Amrani, M., Dreyfus, G., Bahrami, T., de Robertis, F., Baig, K., Asimakopoulos, G., Vohra, H., Pai, V., Tadjkarimi, S., Soleimani, G., Stavri, G., Bull, H., Collappen, H., Sadowksi, J., Kapelak, B., Gaweda, B., Rudzinski, P., Stolinski, J., Konstanty-Kalandyk, J., Moraes, F., Moraes, C., Wanderley, J., Pepper, J., De Souza, A., Petrou, M., Trimlett, R., Morgan, T., Gavino, J., Wang, S.F., Chandrasekaran, V., Kanagasaby, R., Sarsam, M., Ryan, H., Billings, L., Ruddick, L., Achampong, A., Forster, E., Mohama, E., McDonnell, P., Pawlaczyk, R., Siondalski, P., Rogowski, J., Roszak, K., Jarmoszewicz, K., Jagielak, D., Gafka, S., Mannam, G., Naguboyin, Sajja, L. Rao, Dandu, B., Peddireddy, J., Adepu, A., Briffa, N., Braidley, P., Cooper, G., Allen, K., Sangha, G., Bridge, C., McMellon, H., Shaw, P., Casabona, R., Dato, G. Actis, Bardi, G., Del Ponte, S., Forsennati, F., Parisi, F., Punta, G., Flocco, R., Sansone, F., Zingarelli, E., Demartino, A., Dihmis, W., Kuduvali, M., Prince, C., Rogers, H., McQuade, L., Duran-Rosas, A., Anisimowicz, L., Bokszanski, M., Pawliszak, W., Kolakowski, J., Lau, G., Ogorzeja, W., Gumanska, I., Kulinski, P., Podesser, B., Trescher, K., Bernecker, O., Holzinger, C., Binder, K., Schor, I., Bergmann, P., Kassal, H., Dunkel, E., Motovova, B., Trehan, N., Meharwal, Z., Malhotra, R., Goel, M., Kumer, B., Bazaz, S., Bake, N., Singh, A., Mishka, Y., Gupta, R., Basumatary, S., Zembala, M., Szafron, B., Pacholewicz, J., Krason, M., Farmas, Wojarski, Zych, Szymanik, I., Kolwca, M., Mazur, W., Kurowicki, A., Zurek, S., Stacel, T., Jaworska, I., Gaudino, Mario, Audisio, Katia, Rahouma, Mohamed, Robinson, N. Bryce, Soletti, Giovanni J., Cancelli, Gianmarco, Masterson Creber, Ruth M., Gray, Alastair, Lees, Belinda, Gerry, Stephen, Benedetto, Umberto, Flather, Marcus, Taggart, David P.
Publikováno v:
In The Journal of Thoracic and Cardiovascular Surgery August 2023 166(2):532-539
Autor:
Shultz, M. E., Johnston, C., Labadie-Bartz, J., Petit, V., David-Uraz, A., Kochukhov, O., Wade, G. A., Pepper, J., Stassun, K. G., Rodriguez, J. E., Lund, M. B., James, D. J.
HD 62658 (B9p V) is a little-studied chemically peculiar star. Light curves obtained by the Kilodegree Extremely Little Telescope (KELT) and Transiting Exoplanet Survey Satellite (TESS) show clear eclipses with a period of about 4.75 d, as well as ou
Externí odkaz:
http://arxiv.org/abs/1910.02928