Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Lindsey Wiser"'
Autor:
Everett Schlawin, Sagnick Mukherjee, Kazumasa Ohno, Taylor J. Bell, Thomas G. Beatty, Thomas P. Greene, Michael Line, Ryan C. Challener, Vivien Parmentier, Jonathan J. Fortney, Emily Rauscher, Lindsey Wiser, Luis Welbanks, Matthew Murphy, Isaac Edelman, Natasha Batalha, Sarah E. Moran, Nishil Mehta, Marcia Rieke
Publikováno v:
The Astronomical Journal, Vol 168, Iss 3, p 104 (2024)
WASP-69 b is a hot, inflated, Saturn-mass planet (0.26 M _Jup ) with a zero-albedo equilibrium temperature of 963 K. Here, we report the JWST 2–12 μ m emission spectrum of the planet consisting of two eclipses observed with NIRCam grism time serie
Externí odkaz:
https://doaj.org/article/e69769acde3d47b0a037dfde7ec88e60
Autor:
Lindsey Wiser, Timiebi Aganaba
Publikováno v:
Acta Astronautica. 203:537-543
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::cb9b29249a119347e726bf23c60c1fcb
https://doi.org/10.1016/j.actaastro.2022.11.023
https://doi.org/10.1016/j.actaastro.2022.11.023
Exoplanet CoRoT-1 b is intriguing because we predict it to be a transitional planet between hot Jupiters (equilibrium temperatures ~ 1500 K) and ultra-hot Jupiters (equilibrium temperatures > 2000 K). In 2012, observations of CoRoT-1 b included one p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d9799bcae7dfb35bb4497e083c16fcdd
http://arxiv.org/abs/2206.03517
http://arxiv.org/abs/2206.03517
Autor:
Megan Mansfield, Lindsey Wiser, Kevin B. Stevenson, Peter Smith, Michael R. Line, Jacob L. Bean, Jonathan J. Fortney, Vivien Parmentier, Eliza M.-R. Kempton, Jacob Arcangeli, Jean-Michel Désert, Brian Kilpatrick, Laura Kreidberg, Matej Malik
Publikováno v:
The Astronomical Journal, 163(6):261. IOP Publishing Ltd.
Secondary eclipse observations of hot Jupiters can reveal both their compositions and thermal structures. Previous observations have shown a diversity of hot Jupiter eclipse spectra, including absorption features, emission features, and featureless b
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a75db2079bcac1c23b03d1d729db39a4
https://dare.uva.nl/personal/pure/en/publications/confirmation-of-water-absorption-in-the-thermal-emission-spectrum-of-the-hot-jupiter-wasp77ab-with-hstwfc3(b1b2c18a-ab84-40d9-9399-64400ba7dc99).html
https://dare.uva.nl/personal/pure/en/publications/confirmation-of-water-absorption-in-the-thermal-emission-spectrum-of-the-hot-jupiter-wasp77ab-with-hstwfc3(b1b2c18a-ab84-40d9-9399-64400ba7dc99).html
Autor:
Michael R. Line, Jean-Michel Desert, Jonathan J. Fortney, Megan Mansfield, Vivien Parmentier, Mark R. Swain, Ehsan Gharib-Nezhad, David K. Sing, Lindsey Wiser, Mercedes Lopez-Morales, Gael M. Roudier, Jacob L. Bean, Eliza M.-R. Kempton, Claire Baxter
Publikováno v:
Nature Astronomy, vol 5, iss 12
Nature Astronomy, 5, 1224-1232. Nature Publishing Group
Nature Astronomy, 5, 1224-1232. Nature Publishing Group
The emergent spectra of close-in, giant exoplanets ("hot Jupiters") are expected to be distinct from those of self-luminous objects with similar effective temperatures because hot Jupiters are primarily heated from above by their host stars rather th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f69d5e019474e826fe085326e2234245