Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Adam J. R. W. Smith"'
Autor:
Nicholas Susemiehl, Avi M. Mandell, Geronimo L. Villanueva, Giuliano Liuzzi, Michael Moore, Tyler Baines, Michael D. Himes, Adam J. R. W. Smith
Publikováno v:
The Astronomical Journal, Vol 166, Iss 3, p 86 (2023)
Techniques to retrieve the atmospheric properties of exoplanets via direct observation of their reflected light have often been limited in scope owing to computational constraints imposed by the forward-model calculations. We have developed a new set
Externí odkaz:
https://doaj.org/article/2be0dc3990004438bd04b45ac174fa73
Autor:
Channon Visscher, Didier Saumon, Christopher Seay, Adam J. R. W. Smith, Caroline V. Morley, Richard S. Freedman, Jonathan J. Fortney, D. J. Teal, Roxana E. Lupu, Ruoyan Wang, Mark S. Marley
Publikováno v:
The Astrophysical Journal, 920(2)
We present a new generation of substellar atmosphere and evolution models, appropriate for application to studies of L, T, and Y-type brown dwarfs and self-luminous extrasolar planets. The atmosphere models describe the expected temperature-pressure
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dc019009e726f1285f8e0ef371d84263
http://arxiv.org/abs/2107.07434
http://arxiv.org/abs/2107.07434
Autor:
Nicholas D. Susemiehl, Michael W. McElwain, Adam J. R. W. Smith, Tyler Baines, Tyler D. Groff, Hari B. Subedi, Christopher C. Stark, Neil T. Zimmerman, Avi Mandell, Mark S. Marley, Aki Roberge, Bernard J. Rauscher, Natasha E. Batalha, Roser Juanola-Parramon
Publikováno v:
Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave.
The exoplanet atmosphere characterization goals of future UV/Optical/Infrared flagship space missions will drive challenging design requirements for instrument wavefront controls, spatial and spectral sampling, spectral bandwidth, and detector perfor
In anticipation of future flagship missions focused on the goal of achieving direct imaging of rocky exoplanets, we have developed a database of models to help the community examine the potential spectral characteristics of a broad range of rocky pla
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1e73fb38dca7c0ccc23a13989cf85778
Publikováno v:
The Astronomical Journal. 162:30
Simulations of exoplanet albedo profiles are key to planning and interpreting future direct imaging observations. In this paper we demonstrate the use of the Planetary Spectrum Generator to produce simulations of reflected light exoplanet spectra. We
Autor:
Mark S. Marley, Jonathan J. Fortney, Tyler D. Robinson, Roxana Lupu, Adam J. R. W. Smith, Y. Katherina Feng, Nikole K. Lewis
Publikováno v:
The Astronomical Journal. 159:36
The characterization of rocky, Earth-like planets is an important goal for future large ground- and space-based telescopes. In support of developing an efficient observational strategy, we have applied Bayesian statistical inference to interpret the
Autor:
Mark S. Marley, Jonathan J. Fortney, Natasha E. Batalha, Nikole K. Lewis, Adam J. R. W. Smith, Bruce Macintosh
Atmospheric characterization of directly imaged planets has thus far been limited to ground-based observations of young, self-luminous, Jovian planets. Near-term space- and ground- based facilities like \emph{WFIRST} and ELTs will be able to directly
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d986f09b5c8e94420817c91b3371295f
http://arxiv.org/abs/1807.08453
http://arxiv.org/abs/1807.08453
Autor:
Adam J. R. W. Smith, Y. Katherina Feng, Jonathan J. Fortney, Tyler D. Robinson, Mark S. Marley, Roxana E. Lupu, Nikole K. Lewis
Publikováno v:
Astronomical Journal; Feb2020, Vol. 159 Issue 2, p1-1, 1p
Autor:
Natasha E. Batalha, Adam J. R. W. Smith, Nikole K. Lewis, Mark S. Marley, Jonathan J. Fortney, Bruce Macintosh
Publikováno v:
Astronomical Journal; Oct2018, Vol. 156 Issue 4, p1-1, 1p