Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Odden, Caroline"'
Autor:
Bryant, Edward M., Bayliss, Daniel, Santerne, Alexandre, Wheatley, Peter J., Nascimbeni, Valerio, Ducrot, Elsa, Burdanov, Artem, Acton, Jack S., Alves, Douglas R., Anderson, David R., Armstrong, David J., Awiphan, Supachai, Cooke, Benjamin F., Burleigh, Matthew R., Casewell, Sarah L., Delrez, Laetitia, Demory, Brice-Olivier, Eigmüller, Philipp, Fukui, Akihiko, Gan, Tianjun, Gill, Samuel, Gillon, Michael, Goad, Michael R., Tan, Thiam-Guan, Günther, Maximilian N., Hardee, Bronwen, Henderson, Beth A., Jehin, Emmanuel, Jenkins, James S., Kosiarek, Molly, Lendl, Monika, Moyano, Maximiliano, Murray, Catriona A., Narita, Norio, Niraula, Prajwal, Odden, Caroline E., Palle, Enric, Parviainen, Hannu, Pedersen, Peter P., Pozuelos, Francisco J., Rackham, Benjamin V., Sebastian, Daniel, Stockdale, Chris, Tilbrook, Rosanna H., Thompson, Samantha J., Triaud, Amaury H. M. J., Udry, Stéphane, Vines, Jose I., West, Richard G., de Wit, Julien
HIP 41378 f is a temperate $9.2\pm0.1 R_{\oplus}$ planet with period of 542.08 days and an extremely low density of $0.09\pm0.02$ g cm$^{-3}$. It transits the bright star HIP 41378 (V=8.93), making it an exciting target for atmospheric characterizati
Externí odkaz:
http://arxiv.org/abs/2104.03159
Autor:
Collins, Karen A., Collins, Kevin I., Pepper, Joshua, Labadie-Bartz, Jonathan, Stassun, Keivan, Gaudi, B. Scott, Bayliss, Daniel, Bento, Joao, Colón, Knicole D., Feliz, Dax, James, David, Johnson, Marshall C., Kuhn, Rudolf B., Lund, Michael B., Penny, Matthew T., Rodriguez, Joseph E., Siverd, Robert J., Stevens, Daniel J., Yao, Xinyu, Zhou, George, Akshay, Mundra, Aldi, Giulio F., Ashcraft, Cliff, Awiphan, Supachai, Baştürk, Özgür, Baker, David, Beatty, Thomas G., Benni, Paul, Berlind, Perry, Berriman, G. Bruce, Berta-Thompson, Zach, Bieryla, Allyson, Bozza, Valerio, Novati, Sebastiano Calchi, Calkins, Michael L., Cann, Jenna M., Ciardi, David R., Clark, Ian R., Cochran, William D., Cohen, David H., Conti, Dennis, Crepp, Justin R., Curtis, Ivan A., D'Ago, Giuseppe, Diazeguigure, Kenny A., Dressing, Courtney D., Dubois, Franky, Ellingson, Erica, Ellis, Tyler G., Esquerdo, Gilbert A., Evans, Phil, Friedli, Alison, Fukui, Akihiko, Fulton, Benjamin J., Gonzales, Erica J., Good, John C., Gregorio, Joao, Gumusayak, Tolga, Hancock, Daniel A., Harada, Caleb K., Hart, Rhodes, Hintz, Eric G., Jang-Condell, Hannah, Jeffery, Elizabeth J., Jensen, Eric L. N., Jofré, Emiliano, Joner, Michael D., Kar, Aman, Kasper, David H., Keten, Burak, Kielkopf, John F., Komonjinda, Siramas, Kotnik, Cliff, Latham, David W., Leuquire, Jacob, Lewis, Tiffany R., Logie, Ludwig, Lowther, Simon J., MacQueen, Phillip J., Martin, Trevor J., Mawet, Dimitri, McLeod, Kim K., Murawski, Gabriel, Narita, Norio, Nordhausen, Jim, Oberst, Thomas E., Odden, Caroline, Panka, Peter A., Petrucci, Romina, Plavchan, Peter, Quinn, Samuel N., Rau, Steve, Reed, Phillip A., Relles, Howard, Renaud, Joe P., Scarpetta, Gaetano, Sorber, Rebecca L., Spencer, Alex D., Spencer, Michelle, Stephens, Denise C., Stockdale, Chris, Tan, Thiam-Guan, Trueblood, Mark, Trueblood, Patricia, Vanaverbeke, Siegfried, Villanueva Jr., Steven, Warner, Elizabeth M., West, Mary Lou, Yalçınkaya, Selçuk, Yeigh, Rex, Zambelli, Roberto
The Kilodegree Extremely Little Telescope (KELT) project has been conducting a photometric survey for transiting planets orbiting bright stars for over ten years. The KELT images have a pixel scale of ~23"/pixel---very similar to that of NASA's Trans
Externí odkaz:
http://arxiv.org/abs/1803.01869