Zobrazeno 1 - 10
of 18
pro vyhledávání: '"Graham K. H. Lee"'
Autor:
Mark Hammond, Graham K. H. Lee, Raymond T. Pierrehumbert, Xianyu Tan, Shang-Min Tsai, Sarah L. Casewell, Katy L. Chubb
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Context: White dwarf - Brown dwarf short period binaries (P$_{\rm orb}$ $\lesssim$ 2 hours) are some of the most extreme irradiated atmospheric environments known. These systems offer an opportunity to explore theoretical and modelling efforts of irr
Autor:
Diana Powell, Kevin B. Stevenson, Xi Zhang, Hannah R. Wakeford, Peter Gao, Jonathan J. Fortney, Caroline V. Morley, Daniel Thorngren, Graham K. H. Lee
Publikováno v:
Nature Astronomy. 4:951-956
Aerosols are common in the atmospheres of exoplanets across a wide swath of temperatures, masses, and ages. These aerosols strongly impact observations of transmitted, reflected, and emitted light from exoplanets, obfuscating our understanding of exo
Autor:
Graham K. H. Lee
Publikováno v:
SEthics@ICSE
While ethical principles like fairness and honesty may be broad cultural or even universal virtues, many inputs into a professional software engineer's ethical code will be situational, depending on the nature of the engineer's employing institution
Autor:
Simon L. Grimm, Ryan Garland, Jean-Loup Baudino, Graham K. H. Lee, Jake Taylor, Kenneth Wood, Patrick G. J. Irwin
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Current observational data of exoplanets are providing increasing detail of their 3D atmospheric structures. As characterisation efforts expand in scope, the need to develop consistent 3D radiative-transfer methods becomes more pertinent as the compl
Autor:
John S. Brownstein, Moritz U. G. Kraemer, Bernardo Gutierrez, Rebecca Katz, Caitlin Rivers, David M. Pigott, Vukosi Marivate, Graham K. H. Lee, Jared B. Hawkins, Samuel V. Scarpino, Bo Xu
Publikováno v:
Nature Computational Science. 1:9-10
Detailed, accurate data related to a disease outbreak enable informed public health decision making. Given the variety of data types available across different regions, global data curation and standardization efforts are essential to guarantee rapid
Autor:
Laura Fortunato, Graham K. H. Lee, Helena Webb, Martin Robinson, Philippe Rocca-Serra, Ian Bush, Thibault Lestang, Susanna-Assunta Sansone, Sebastian Bacon, David J. Gavaghan, Caroline E Morton
Publikováno v:
Patterns
Patterns, Vol 2, Iss 2, Pp 100206-(2021)
Patterns, Vol 2, Iss 2, Pp 100206-(2021)
The importance of software to modern research is well understood, as is the way in which software developed for research can support or undermine important research principles of findability, accessibility, interoperability, and reusability (FAIR). W
Publikováno v:
Astronomy & Astrophysics
Sub-stellar objects exhibit photometric variability, which is believed to be caused by a number of processes, such as magnetically-driven spots or inhomogeneous cloud coverage. Recent models have shown that turbulent flows and waves, including intern
Autor:
David S. Amundsen, Pascal Tremblin, Benjamin Drummond, Ian A. Boutle, Graham K. H. Lee, Nathan J. Mayne, Stefan Lines, Christiane Helling, Max Kerslake, James Manners, Jayesh M. Goyal, David M. Acreman
To understand and compare the 3D atmospheric structure of HD 209458 b and HD 189733 b, focusing on the formation and distribution of cloud particles, as well as their feedback on the dynamics and thermal profile. We couple the 3D Met Office Unified M
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a125cc5677c5c66d6bed3297743cd449
https://hal.science/hal-01834172
https://hal.science/hal-01834172
Autor:
Jayesh M. Goyal, Christiane Helling, Dave Acreman, Stefan Lines, Graham K. H. Lee, David K. Sing, Aarynn L. Carter, Nathan J. Mayne, Ian A. Boutle, Benjamin Drummond, James Manners
We present high resolution transmission spectra, calculated directly from a 3D radiative-hydrodynamics simulation that includes kinetic cloud formation, for HD209458b. We find that the high opacity of our vertically extensive cloud deck, composed of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::14b56e56e9998b4b355cc0d2f7ebaa9f
Recent observations indicate potentially carbon-rich exoplanet atmospheres. Spectral fitting methods for brown dwarfs and exoplanets have invoked the C/O ratio as additional parameter but carbon-rich cloud formation modeling is a challenge for the mo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5d6e847a6f150463c1e1c4c70010bf55
https://hdl.handle.net/10023/15884
https://hdl.handle.net/10023/15884