Zobrazeno 1 - 10
of 951
pro vyhledávání: '"Zamyatina A"'
Autor:
Kirk, James, Ahrer, Eva-Maria, Claringbold, Alastair B., Zamyatina, Maria, Fisher, Chloe, McCormack, Mason, Panwar, Vatsal, Powell, Diana, Taylor, Jake, Thorngren, Daniel P., Christie, Duncan A., Esparza-Borges, Emma, Tsai, Shang-Min, Alderson, Lili, Booth, Richard A., Fairman, Charlotte, López-Morales, Mercedes, Mayne, N. J., Meech, Annabella, Molliere, Paul, Owen, James E., Penzlin, Anna B. T., Sergeev, Denis E., Valentine, Daniel, Wakeford, Hannah R., Wheatley, Peter J.
We present a transmission spectrum of the misaligned hot Jupiter WASP-15b from 2.8--5.2 microns observed with JWST's NIRSpec/G395H grating. Our high signal to noise data, which has negligible red noise, reveals significant absorption by H$_2$O ($4.2\
Externí odkaz:
http://arxiv.org/abs/2410.08116
Autor:
Espinoza, Néstor, Steinrueck, Maria E., Kirk, James, MacDonald, Ryan J., Savel, Arjun B., Arnold, Kenneth, Kempton, Eliza M. -R., Murphy, Matthew M., Carone, Ludmila, Zamyatina, Maria, Lewis, David A., Samra, Dominic, Kiefer, Sven, Rauscher, Emily, Christie, Duncan, Mayne, Nathan, Helling, Christiane, Rustamkulov, Zafar, Parmentier, Vivien, May, Erin M., Carter, Aarynn L., Zhang, Xi, López-Morales, Mercedes, Allen, Natalie, Blecic, Jasmina, Decin, Leen, Mancini, Luigi, Molaverdikhani, Karan, Rackham, Benjamin V., Palle, Enric, Tsai, Shang-Min, Ahrer, Eva-Maria, Bean, Jacob L., Crossfield, Ian J. M., Haegele, David, Hébrard, Eric, Kreidberg, Laura, Powell, Diana, Schneider, Aaron D., Welbanks, Luis, Wheatley, Peter, Brahm, Rafael, Crouzet, Nicolas
Transmission spectroscopy has been a workhorse technique over the past two decades to constrain the physical and chemical properties of exoplanet atmospheres. One of its classical key assumptions is that the portion of the atmosphere it probes -- the
Externí odkaz:
http://arxiv.org/abs/2407.10294
Autor:
Kirk, James, Ahrer, Eva-Maria, Penzlin, Anna B. T., Owen, James E., Booth, Richard A., Alderson, Lili, Christie, Duncan A., Claringbold, Alastair B., Esparza-Borges, Emma, Fisher, Chloe E., López-Morales, Mercedes, Mayne, N. J., McCormack, Mason, Meech, Annabella, Panwar, Vatsal, Powell, Diana, Taylor, Jake, Sergeev, Denis E., Valentine, Daniel, Wakeford, Hannah R., Wheatley, Peter J., Zamyatina, Maria
A primary objective of exoplanet atmosphere characterisation is to learn about planet formation and evolution, however, this is challenged by degeneracies. To determine whether differences in atmospheric composition can be reliably traced to differen
Externí odkaz:
http://arxiv.org/abs/2407.03198
Autor:
Penzlin, Anna B. T., Booth, Richard A., Kirk, James, Owen, James E., Ahrer, Eva-Maria, Christie, Duncan A., Claringbold, Alastair B., Esparza-Borges, Emma, López-Morales, M., Mayne, N. J., McCormack, Mason, Meech, Annabella, Panwar, Vatsal, Powell, Diana, Sergeev, Denis E., Taylor, Jake, Wheatley, Peter J., Zamyatina, Maria
Hot Jupiters present a unique opportunity for measuring how planet formation history shapes present-day atmospheric composition. However, due to the myriad pathways influencing composition, a well-constructed sample of planets is needed to determine
Externí odkaz:
http://arxiv.org/abs/2407.03199
Autor:
Christie, D. A., Mayne, N. J., Zamyatina, M., Baskett, H., Evans-Soma, T. M., Wood, N., Kohary, K.
General circulation models are a useful tool in understanding the three dimensional structure of hot Jupiter and sub-Neptune atmospheres; however, understanding the validity of the results from these simulations requires an understanding the artifici
Externí odkaz:
http://arxiv.org/abs/2406.02231
Autor:
Zamyatina, Maria, Christie, Duncan A., Hébrard, Eric, Mayne, Nathan J., Radica, Michael, Taylor, Jake, Baskett, Harry, Moore, Ben, Lils, Craig, Sergeev, Denis, Ahrer, Eva-Maria, Manners, James, Kohary, Krisztian, Feinstein, Adina D.
Transport-induced quenching in hot Jupiter atmospheres is a process that determines the boundary between the part of the atmosphere at chemical equilibrium and the part of the atmosphere at thermochemical (but not photothermochemical) disequilibrium.
Externí odkaz:
http://arxiv.org/abs/2402.14535
Autor:
Radica, Michael, Welbanks, Luis, Espinoza, Néstor, Taylor, Jake, Coulombe, Louis-Philippe, Feinstein, Adina D., Goyal, Jayesh, Scarsdale, Nicholas, Albert, Loic, Baghel, Priyanka, Bean, Jacob L., Blecic, Jasmina, Lafrenière, David, MacDonald, Ryan J., Zamyatina, Maria, Allart, Romain, Artigau, Étienne, Batalha, Natasha E., Cook, Neil James, Cowan, Nicolas B., Dang, Lisa, Doyon, René, Fournier-Tondreau, Marylou, Johnstone, Doug, Line, Michael R., Moran, Sarah E., Mukherjee, Sagnick, Pelletier, Stefan, Roy, Pierre-Alexis, Talens, Geert Jan, Filippazzo, Joseph, Pontoppidan, Klaus, Volk, Kevin
The future is now - after its long-awaited launch in December 2021, JWST began science operations in July 2022 and is already revolutionizing exoplanet astronomy. The Early Release Observations (ERO) program was designed to provide the first images a
Externí odkaz:
http://arxiv.org/abs/2305.17001
Autor:
Taylor, Jake, Radica, Michael, Welbanks, Luis, MacDonald, Ryan J., Blecic, Jasmina, Zamyatina, Maria, Roth, Alexander, Bean, Jacob L., Parmentier, Vivien, Coulombe, Louis-Philippe, Feinstein, Adina D., Espinoza, Néstor, Benneke, Björn, Lafrenière, David, Doyon, René, Ahrer, Eva-Maria
The newly operational JWST offers the potential to study the atmospheres of distant worlds with precision that has not been achieved before. One of the first exoplanets observed by JWST in the summer of 2022 was WASP-96 b, a hot-Saturn orbiting a G8
Externí odkaz:
http://arxiv.org/abs/2305.16887
Autor:
Zamyatina, Maria, Hébrard, Éric, Drummond, Benjamin, Mayne, Nathan J., Manners, James, Christie, Duncan A., Tremblin, Pascal, Sing, David K., Kohary, Krisztian
Transport-induced quenching, i.e., the homogenisation of chemical abundances by atmospheric advection, is thought to occur in the atmospheres of hot gas giant exoplanets. While some numerical modelling of this process exists, the three-dimensional na
Externí odkaz:
http://arxiv.org/abs/2211.09071
Autor:
Christie, Duncan A., Lee, Elspeth K. H., Innes, Hamish, Noti, Pascal A., Charnay, Benjamin, Fauchez, Thomas J., Mayne, Nathan J., Deitrick, Russell, Ding, Feng, Greco, Jennifer J., Hammond, Mark, Malsky, Isaac, Mandell, Avi, Rauscher, Emily, Roman, Michael T., Sergeev, Denis E., Sohl, Linda, Steinrueck, Maria E., Turbet, Martin, Wolf, Eric T., Zamyatina, Maria, Carone, Ludmila
With an increased focus on the observing and modelling of mini-Neptunes, there comes a need to better understand the tools we use to model their atmospheres. In this paper, we present the protocol for the CAMEMBERT (Comparing Atmospheric Models of Ex
Externí odkaz:
http://arxiv.org/abs/2211.04048