Zobrazeno 1 - 10
of 214
pro vyhledávání: '"EVANS, A. THOMAS"'
Autor:
Tumborang, Abigail A., Spake, Jessica J., Knutson, Heather A., Mansfield, Megan Weiner, Paragas, Kimberly, Edwards, Billy, Kataria, Tiffany, Evans-Soma, Thomas M., Lewis, Nikole K., Ballester, Gilda E.
Publikováno v:
The Astronomical Journal, 168:296 (14pp), 2024 December
We present a detailed reanalysis of the atmospheric properties of WASP-19b, an ultra-hot Jupiter (1.14 M Jup, 1.41 R Jup) orbiting an active Sun-like star every 0.79 day. We reanalyze a transit and secondary eclipse of WASP-19b observed by the Hubble
Externí odkaz:
http://arxiv.org/abs/2412.03739
Autor:
Ashtari, Reza, Stevenson, Kevin B., Sing, David, Lopez-Morales, Mercedes, Alam, Munazza K., Nikolov, Nikolay K., Evans-Soma, Thomas M.
Producing optimized and accurate transmission spectra of exoplanets from telescope data has traditionally been a manual and labor-intensive procedure. Here we present the results of the first attempt to improve and standardize this procedure using ar
Externí odkaz:
http://arxiv.org/abs/2410.06804
Autor:
Piaulet-Ghorayeb, Caroline, Benneke, Bjorn, Radica, Michael, Raul, Eshan, Coulombe, Louis-Philippe, Ahrer, Eva-Maria, Kubyshkina, Daria, Howard, Ward S., Krissansen-Totton, Joshua, MacDonald, Ryan, Roy, Pierre-Alexis, Louca, Amy, Christie, Duncan, Fournier-Tondreau, Marylou, Allart, Romain, Miguel, Yamila, Schlichting, Hilke E., Welbanks, Luis, Cadieux, Charles, Dorn, Caroline, Evans-Soma, Thomas M., Fortney, Jonathan J., Pierrehumbert, Raymond, Lafreniere, David, Acuna, Lorena, Komacek, Thaddeus, Innes, Hamish, Beatty, Thomas G., Cloutier, Ryan, Doyon, Rene, Gagnebin, Anna, Gapp, Cyril, Knutson, Heather A.
With sizable volatile envelopes but smaller radii than the solar system ice giants, sub-Neptunes have been revealed as one of the most common types of planet in the galaxy. While the spectroscopic characterization of larger sub-Neptunes (2.5-4R$_\opl
Externí odkaz:
http://arxiv.org/abs/2410.03527
Autor:
Thao, Pa Chia, Mann, Andrew W., Feinstein, Adina D., Gao, Peter, Thorngren, Daniel, Rotman, Yoav, Welbanks, Luis, Brown, Alexander, Duvvuri, Girish M., France, Kevin, Longo, Isabella, Sandoval, Angeli, Schneider, P. Christian, Wilson, David J., Youngblood, Allison, Vanderburg, Andrew, Barber, Madyson G., Wood, Mackenna L., Batalha, Natasha E., Kraus, Adam L., Murray, Catriona Anne, Newton, Elisabeth R., Rizzuto, Aaron, Tofflemire, Benjamin M., Tsai, Shang-Min, Bean, Jacob L., Berta-Thompson, Zachory K., Evans-Soma, Thomas M., Froning, Cynthia S., Kempton, Eliza M. -R., Miguel, Yamila, Pineda, J. Sebastian
The characterization of young planets (< 300 Myr) is pivotal for understanding planet formation and evolution. We present the 3-5$\mu$m transmission spectrum of the 17 Myr, Jupiter-size ($R$ $\sim$10$R_{\oplus}$) planet, HIP 67522 b, observed with JW
Externí odkaz:
http://arxiv.org/abs/2409.16355
Autor:
Allen, Natalie H., Sing, David K., Espinoza, Néstor, O'Steen, Richard, Nikolov, Nikolay K., Rustamkulov, Zafar, Evans-Soma, Thomas M., Rosado, Lakeisha M. Ramos, Alam, Munazza K., López-Morales, Mercedes, Stevenson, Kevin B., Wakeford, Hannah R., May, Erin M., Brahm, Rafael, Pinto, Marcelo Tala
The Hubble Space Telescope (HST) has been our most prolific tool to study exoplanet atmospheres. As the age of JWST begins, there is a wealth of HST archival data that is useful to strengthen our inferences from JWST. Notably, HST/STIS and its 0.3-1
Externí odkaz:
http://arxiv.org/abs/2405.20361
Autor:
Benneke, Björn, Roy, Pierre-Alexis, Coulombe, Louis-Philippe, Radica, Michael, Piaulet, Caroline, Ahrer, Eva-Maria, Pierrehumbert, Raymond, Krissansen-Totton, Joshua, Schlichting, Hilke E., Hu, Renyu, Yang, Jeehyun, Christie, Duncan, Thorngren, Daniel, Young, Edward D., Pelletier, Stefan, Knutson, Heather A., Miguel, Yamila, Evans-Soma, Thomas M., Dorn, Caroline, Gagnebin, Anna, Fortney, Jonathan J., Komacek, Thaddeus, MacDonald, Ryan, Raul, Eshan, Cloutier, Ryan, Acuna, Lorena, Lafrenière, David, Cadieux, Charles, Doyon, René, Welbanks, Luis, Allart, Romain
Even though sub-Neptunes likely represent the most common outcome of planet formation, their natures remain poorly understood. In particular, planets near 1.5-2.5$\,R_\oplus$ often have bulk densities that can be explained equally well with widely di
Externí odkaz:
http://arxiv.org/abs/2403.03325
Autor:
Fortune, Mark, Gibson, Neale P., Foreman-Mackey, Daniel, Evans-Soma, Thomas M., Maguire, Cathal, Ramkumar, Swaetha
Publikováno v:
A&A 686, A89 (2024)
The use of Gaussian processes (GPs) is a common approach to account for correlated noise in exoplanet time series, particularly for transmission and emission spectroscopy. This analysis has typically been performed for each wavelength channel separat
Externí odkaz:
http://arxiv.org/abs/2402.15204
Autor:
Lamb, Jonathan Nicholas1,2 (AUTHOR), Evans, Jonathan Thomas2,3,4 (AUTHOR) j.t.evans@exeter.ac.uk, Relton, Samuel5 (AUTHOR), Whitehouse, Michael Richard2 (AUTHOR), Wilkinson, J Mark6 (AUTHOR), Pandit, Hemant7 (AUTHOR)
Publikováno v:
PLoS Medicine. 10/01/2024, Vol. 21 Issue 10, p1-14. 14p.
Post-operative periprosthetic femoral fractures in England: Patient profiles and short-term outcomes
Autor:
Aryaie, Mohammad, Evans, Jonathan Thomas, Reed, Mike, Shelton, Cliff L, Johansen, Antony, Smith, Toby O, Benn, Jonathan, Baxter, Mark, Aylin, Paul, Whitehouse, Michael R, Bottle, Alex
Publikováno v:
In Injury February 2025 56(2)
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