Zobrazeno 1 - 10
of 207
pro vyhledávání: '"Bennett, Katherine A."'
Autor:
Bennett, Katherine A., Sing, David K., Stevenson, Kevin B., Wakeford, Hannah R., Rustamkulov, Zafar, Allen, Natalie H., Lothringer, Joshua D., MacDonald, Ryan J., Mayne, Nathan J., Fu, Guangwei
Which rocky exoplanets have atmospheres, and which do not? This presumably simply question is the first that must be answered in the pathway toward understanding the prevalence of nearby habitable planets. A mere 6.9 pc from Earth, the LTT 1445A syst
Externí odkaz:
http://arxiv.org/abs/2410.11054
Autor:
Kirk, James, Stevenson, Kevin B., Fu, Guangwei, Lustig-Yaeger, Jacob, Moran, Sarah E., Peacock, Sarah, Alam, Munazza K., Batalha, Natasha E., Bennett, Katherine A., Gonzalez-Quiles, Junellie, López-Morales, Mercedes, Lothringer, Joshua D., MacDonald, Ryan J., May, E. M., Mayorga, L. C., Rustamkulov, Zafar, Sing, David K., Sotzen, Kristin S., Valenti, Jeff A., Wakeford, Hannah R.
We present a JWST/NIRCam transmission spectrum from $3.9-5.0$ $\mu$m of the recently-validated sub-Earth GJ 341b ($\mathrm{R_P} = 0.92$ $\mathrm{R_{\oplus}}$, $\mathrm{T_{eq}} = 540$ K) orbiting a nearby bright M1 star ($\mathrm{d} = 10.4$ pc, $\math
Externí odkaz:
http://arxiv.org/abs/2401.06043
Autor:
May, E. M., MacDonald, Ryan J., Bennett, Katherine A., Moran, Sarah E., Wakeford, Hannah R., Peacock, Sarah, Lustig-Yaeger, Jacob, Highland, Alicia N., Stevenson, Kevin B., Sing, David K., Mayorga, L. C., Batalha, Natasha E., Kirk, James, Lopez-Morales, Mercedes, Valenti, Jeff A., Alam, Munazza K., Alderson, Lili, Fu, Guangwei, Gonzalez-Quiles, Junellie, Lothringer, Joshua D., Rustamkulov, Zafar, Sotzen, Kristin S.
Publikováno v:
ApJL (2023): 959, L9
The search for rocky planet atmospheres with JWST has focused on planets transiting M dwarfs. Such planets have favorable planet-to-star size ratios, enhancing the amplitude of atmospheric features. Since the expected signal strength of atmospheric f
Externí odkaz:
http://arxiv.org/abs/2310.10711
Autor:
Bennett, Katherine A., Redfield, Seth, Oklopčić, Antonija, Carleo, Ilaria, Ninan, Joe P., Endl, Michael
Hot Jupiters orbiting extremely close to their host star may experience atmospheric escape due to the large amounts of high-energy radiation they receive. Understanding the conditions under which this occurs is critical, as atmospheric escape is beli
Externí odkaz:
http://arxiv.org/abs/2305.02465
Autor:
Moran, Sarah E., Stevenson, Kevin B., Sing, David K., MacDonald, Ryan J., Kirk, James, Lustig-Yaeger, Jacob, Peacock, Sarah, Mayorga, L. C., Bennett, Katherine A., López-Morales, Mercedes, May, E. M., Rustamkulov, Zafar, Valenti, Jeff A., Redai, Jéa I. Adams, Alam, Munazza K., Batalha, Natasha E., Fu, Guangwei, Gonzalez-Quiles, Junellie, Highland, Alicia N., Kruse, Ethan, Lothringer, Joshua D., Ceballos, Kevin N. Ortiz, Sotzen, Kristin S., Wakeford, Hannah R.
Planets orbiting M-dwarf stars are prime targets in the search for rocky exoplanet atmospheres. The small size of M dwarfs renders their planets exceptional targets for transmission spectroscopy, facilitating atmospheric characterization. However, it
Externí odkaz:
http://arxiv.org/abs/2305.00868
Autor:
Barretina-Ginesta, Pilar, Bennett, Katherine, Berek, Jonathan, Berger, Regina, Bjørge, Line, Boere, Ingrid, Brennan, Donal, Bruchim, Ilan, Chang, Ting-Chang, Chavez Blanco, Adriana, Chen, Xiaojun, Colombo, Nicoletta, Crosbie, Emma, Denys, Hannelore, Duska, Linda, Fruehauf, Filip, Gomez Garcia, Eva Maria, van Gorp, Toon, Grimm, Christoph, Guitmann, Gustavo, Han, Kathy, Hanker, Lars, Harano, Kenichi, Hasegawa, Kosei, Herrington, C Simon, Ip, Philip, Joly, Florence, Khaw, Pearly, Kohn, Elise, Kristeleit, Rebecca, Kroep, Judith, Leary, Alexandra, Lee, Jung-Yun, Lheureux, Stephanie, Liu, Jihong, Mackay, Helen, Mahner, Sven, Mariani, Andrea, McAlpine, Jessica, Mikami, Yoshiki, Mirza, Mansoor Raza, Mukhopadhyay, Asima, Nagao, Shoji, Ng, Joseph, Nogueira-Rodrigues, Angelica, Novák, Zoltán, O'Donnell, Jennifer, Osborne, Sherill, Perez-Fidalgo, J. Alejandro, Romeo Marin, Margarita, Roy Chowdhury, Rahul, Sadozye, Azmat, Safra, Tamar, Scott, Claire, Sehouli, Jalid, Slomovitz, Brian, Tan, David, Taylor, Alexandra, Valabrega, Giorgio, Veneziani, Ana, Verhoeven, Karen, Vetter, Marcus, Wampfler, Julian, Westin, Shannon, Wimberger, Pauline, Zola, Paolo, Creutzberg, Carien L *, *, Kim, Jae-Weon *, Eminowicz, Gemma, Allanson, Emma, Eberst, Lauriane, Kim, Se Ik, Nout, Remi A, Park, Jeong-Yeol, Lorusso, Domenica, Mileshkin, Linda, Ottevanger, Petronella B, Brand, Alison, Mezzanzanica, Delia, Oza, Amit, Gebski, Val, Pothuri, Bhavana, Batley, Tania †, Gordon, Carol †, Mitra, Tina †, White, Helen †, Howitt, Brooke, Matias-Guiu, Xavier, Ray-Coquard, Isabelle, Gaffney, David, Small, William, Jr, Miller, Austin, Concin, Nicole, Powell, Matthew A, Stuart, Gavin, Bookman, Michael A
Publikováno v:
In The Lancet Oncology September 2024 25(9):e420-e431
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Publikováno v:
In Renewable and Sustainable Energy Reviews May 2022 160