Zobrazeno 1 - 10
of 282
pro vyhledávání: '"Fowler, Martin"'
Autor:
Noguer, Federico R., Corley, Suber, Pearson, Kyle A., Zellem, Robert T., Simon, Molly N., Burt, Jennifer A., Huckabee, Isabela, August, Prune C., Mansfield, Megan Weiner, Dalba, Paul A., Smith, Peter C. B., Banks, Timothy, Bell, Ira, Daniel, Dominique, Dawson, Lindsay, De Mula, Jesús, Deldem, Marc, Deligeorgopoulos, Dimitrios, Di Sisto, Romina P., Dymock, Roger, Evans, Phil, Follero, Giulio, Fowler, Martin J. F., Fernández-Lajús, Eduardo, Hamrick, Alex, Iannascoli, Nicoletta, Kovacs, Andre O., Kulh, Denis Henrique, Lopresti, Claudio, Marino, Antonio, Martin, Bryan E., Matassa, Paolo Arcangelo, Napoleão, Tasso Augusto, Nastasi, Alessandro, Norris, Anthony, Odasso, Alessandro, Paschalis, Nikolaos I., Pintr, Pavel, Postiglione, Jake, Randolph, Justus, Regembal, François, Rousselot, Lionel, da Silva, Sergio José Gonçalves, Smith, Andrew, Tomacelli, Andrea
We present an updated ephemeris and physical parameters for the exoplanet WASP-77 A b. In this effort, we combine 64 ground- and space-based transit observations, 6 space-based eclipse observations, and 32 radial velocity observations to produce the
Externí odkaz:
http://arxiv.org/abs/2405.19615
Autor:
Smith, Peter, Line, Michael, Bean, Jacob, Brogi, Matteo, August, Prune, Welbanks, Luis, Desert, Jean-Michel, Lunine, Jonathan, Sanchez, Jorge, Mansfield, Megan, Pino, Lorenzo, Rauscher, Emily, Kempton, Eliza, Zalesky, Joseph, Fowler, Martin
Ground-based, high-resolution and space-based, low-resolution spectroscopy are the two main avenues through which transiting exoplanet atmospheres are studied. Both methods provide unique strengths and shortcomings, and combining the two can be a pow
Externí odkaz:
http://arxiv.org/abs/2312.13069
Autor:
Nediyedath, Avinash S., Fowler, Martin J., Norris, A., Maidur, Shivaraj R., Pearson, Kyle A., Dixon, S., Lewin, P., Kovacs, Andre O., Odasso, A., Davis, K., Primm, M., Das, P., Martin, Bryan E., Lalla, D.
Publikováno v:
JAAVSO Volume 51 number 2 (2023)
NASA Citizen Scientists have used Exoplanet Transit Interpretation Code (EXOTIC) to reduce 40 sets of time-series images of WASP-12 taken by privately owned telescopes and a 6-inch telescope operated by the Center for Astrophysics | Harvard & Smithso
Externí odkaz:
http://arxiv.org/abs/2306.17473
Autor:
Pearson, Kyle A., Beichman, Chas, Fulton, Benjamin J., Esposito, Thomas M., Zellem, Robert T., Ciardi, David R., Rolfness, Jonah, Engelke, John, Fatahi, Tamim, Zimmerman-Brachman, Rachel, Avsar, Arin, Bhalerao, Varun, Boyce, Pat, Bretton, Marc, Burnett, Alexandra D., Burt, Jennifer, Fowler, Martin, Gallego, Daniel, Gomez, Edward, Guillet, Bruno, Hilburn, Jerry, Jongen, Yves, Kataria, Tiffany, Kokori, Anastasia, Kumar, Harsh, Kuossari, Petri, Lekkas, Georgios, Marchini, Alessandro, Meneghelli, Nicola, Ngeow, Chow-Choong, Primm, Michael, Samantaray, Subham, Shimizu, Masao, Silvis, George, Sienkiewicz, Frank, Swain, Vishwajeet, Tan, Joshua, Tock, Kalee, Wagner, Kevin, Wünsche, Anaël
The transiting planet HD80606b undergoes a 1000-fold increase in insolation during its 111-day orbit due to it being highly eccentric (e=0.93). The planet's effective temperature increases from 400K to over 1400K in a few hours as it makes a rapid pa
Externí odkaz:
http://arxiv.org/abs/2208.14520
Autor:
Yeung, Paige, Perian, Quinn, Robertson, Peyton, Fitzgerald, Michael, Fowler, Martin, Sienkiewicz, Frank, Tock, Kalée
Based on the light an exoplanet blocks from its host star as it passes in front of it during a transit, the mid-transit time can be determined. Periodic variations in mid-transit times can indicate another planet's gravitational influence. We investi
Externí odkaz:
http://arxiv.org/abs/2207.01559
Autor:
Adebayo, Oyeboade, Bhatnagar, Srijak, Webb, Jamie, Campbell, Calvin, Fowler, Martin, MacAdam, Natasha M., Macdonald, Adam, Li, Carmen, Hubert, Casey R.J.
Publikováno v:
In Marine Pollution Bulletin November 2024 208
Autor:
Kokori, Anastasia, Tsiaras, Angelos, Edwards, Billy, Rocchetto, Marco, Tinetti, Giovanna, Wünsche, Anaël, Paschalis, Nikolaos, Agnihotri, Vikrant Kumar, Bachschmidt, Matthieu, Bretton, Marc, Caines, Hamish, Caló, Mauro, Casali, Roland, Crow, Martin, Dawes, Simon, Deldem, Marc, Deligeorgopoulos, Dimitrios, Dymock, Roger, Evans, Phil, Falco, Carmelo, Ferratfiat, Stephane, Fowler, Martin, Futcher, Stephen, Guerra, Pere, Hurter, Francois, Jones, Adrian, Kang, Wonseok, Kim, Taewoo, Lee, Richard, Lopresti, Claudio, Marino, Antonio, Mallonn, Matthias, Mortari, Fabio, Morvan, Mario, Mugnai, Lorenzo V., Nastasi, Alessandro, Perroud, Valère, Pereira, Cédric, Phillips, Mark, Pintr, Pavel, Raetz, Manfred, Regembal, Francois, Savage, John, Sedita, Danilo, Sioulas, Nick, Strikis, Iakovos, Thurston, Geoffrey, Tomacelli, Andrea, Tomatis, Alberto
The Ariel mission will observe spectroscopically around 1000 exoplanets to further characterise their atmospheres. For the mission to be as efficient as possible, a good knowledge of the planets' ephemerides is needed before its launch in 2028. While
Externí odkaz:
http://arxiv.org/abs/2012.07478