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pro vyhledávání: '"Skemer, Andrew J. I."'
Autor:
Mukherjee, Sagnick, Fortney, Jonathan J., Batalha, Natasha E., Karalidi, Theodora, Marley, Mark S., Visscher, Channon, Miles, Brittany E., Skemer, Andrew J. I.
Evidence of disequilibrium chemistry due to vertical mixing in the atmospheres of many T and Y-dwarfs has been inferred due to enhanced mixing ratios of CO and reduced NH$_3$. Atmospheric models of planets and brown dwarfs typically parameterize this
Externí odkaz:
http://arxiv.org/abs/2208.14317
Autor:
Doelman, David S., Stone, Jordan M., Briesemeister, Zackery W., Skemer, Andrew J. I., Barman, Travis, Brock, Laci S., Hinz, Philip M., Bohn, Alexander, Kenworthy, Matthew, Haffert, Sebastiaan Y., Snik, Frans, Ertel, Steve, Leisenring, Jarron M., Woodward, Charles E., Skrutskie, Michael F.
Understanding the physical processes sculpting the appearance of young gas-giant planets is complicated by degeneracies confounding effective temperature, surface gravity, cloudiness, and chemistry. To enable more detailed studies, spectroscopic obse
Externí odkaz:
http://arxiv.org/abs/2203.08165
Autor:
Carter, Aarynn L., Hinkley, Sasha, Bonavita, Mariangela, Phillips, Mark W., Girard, Julien H., Perrin, Marshall, Pueyo, Laurent, Vigan, Arthur, Gagné, Jonathan, Skemer, Andrew J. I.
The James Webb Space Telescope (JWST), currently scheduled to launch in 2021, will dramatically advance our understanding of exoplanetary systems with its ability to directly image and characterise planetary-mass companions at wide separations throug
Externí odkaz:
http://arxiv.org/abs/2011.07075
Autor:
Miles, Brittany E., Skemer, Andrew J. I., Morley, Caroline V., Marley, Mark S., Fortney, Jonathan J., Allers, Katelyn N., Faherty, Jacqueline K., Geballe, Thomas R., Visscher, Channon, Schneider, Adam C., Lupu, Roxana, Freedman, Richard S., Bjoraker, Gordon L.
Cold brown dwarfs are excellent analogs of widely separated, gas giant exoplanets, and provide insight into the potential atmospheric chemistry and physics we may encounter in objects discovered by future direct imaging surveys. We present a low reso
Externí odkaz:
http://arxiv.org/abs/2004.10770
Autor:
Skemer, Andrew J. I., Close, Laird M., Greene, Thomas P., Hinz, Philip M., Hoffmann, William F., Males, Jared R.
Core-accretion planet formation begins in protoplanetary disks with the growth of small, ISM dust grains into larger particles. The progress of grain growth, which can be quantified using 10 micron silicate spectroscopy, has broad implications for th
Externí odkaz:
http://arxiv.org/abs/1107.3161
Akademický článek
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Autor:
Shaklan, Stuart B., Ruane, Garreth J., Carter, Aarynn L., Skemer, Andrew J. I., Danielski, Camilla, Leisenring, Jarron, Wang, Jason J., Van Gorkom, Kyle, York, Brian, Adams, Jea, Biller, Beth, Girard, Julien H., Hinkley, Sasha, Nickson, Bryony, Perrin, Marshall, Pueyo, Laurent
Publikováno v:
Proceedings of SPIE; September 2021, Vol. 11823 Issue: 1 p118230H-118230H-17, 11704788p
Autor:
Carter, Aarynn L., Skemer, Andrew J. I., Danielski, Camilla, Leisenring, Jarron, Wang, Jason J., Van Gorkom, Kyle, York, Brian, Adams, Jea, Biller, Beth, Girard, Julien H., Hinkley, Sasha, Nickson, Bryony, Perrin, Marshall, Pueyo, Laurent
Publikováno v:
Proceedings of SPIE; 6/4/2021, Vol. 11823, p118230H-118230H-17, 1p