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pro vyhledávání: '"Maguire, Cathal"'
Recent advancements in ultra-stable ground-based high-resolution spectrographs have propelled ground-based astronomy to the forefront of exoplanet detection and characterisation. Retrieving accurate atmospheric parameters depends on accurate modellin
Externí odkaz:
http://arxiv.org/abs/2410.19588
Autor:
Maguire, Cathal, Gibson, Neale P., Nugroho, Stevanus K., Fortune, Mark, Ramkumar, Swaetha, Gandhi, Siddharth, de Mooij, Ernst
Publikováno v:
A&A 687, A49 (2024)
Direct atmospheric retrievals of exoplanets at high-resolution have recently allowed for a more detailed characterisation of their chemistry and dynamics from the ground. By monitoring the longitudinal distribution of species, as well as the varying
Externí odkaz:
http://arxiv.org/abs/2404.10463
Autor:
Fortune, Mark, Gibson, Neale P., Foreman-Mackey, Daniel, Evans-Soma, Thomas M., Maguire, Cathal, Ramkumar, Swaetha
Publikováno v:
A&A 686, A89 (2024)
The use of Gaussian processes (GPs) is a common approach to account for correlated noise in exoplanet time series, particularly for transmission and emission spectroscopy. This analysis has typically been performed for each wavelength channel separat
Externí odkaz:
http://arxiv.org/abs/2402.15204
The characterization of exoplanet atmospheres has proven to be successful using high-resolution spectroscopy. Phase curve observations of hot/ultra-hot Jupiters can reveal their compositions and thermal structures, thereby allowing the detection of m
Externí odkaz:
http://arxiv.org/abs/2308.07157
Autor:
Gandhi, Siddharth, Kesseli, Aurora, Zhang, Yapeng, Louca, Amy, Snellen, Ignas, Brogi, Matteo, Miguel, Yamila, Casasayas-Barris, Núria, Pelletier, Stefan, Landman, Rico, Maguire, Cathal, Gibson, Neale P.
Publikováno v:
The Astronomical Journal, Volume 165, 242 (2023)
Ground-based high-resolution spectroscopy (HRS) has detected numerous chemical species and atmospheric dynamics in exoplanets, most notably ultra-hot Jupiters (UHJs). However, quantitative estimates on abundances have been challenging but are essenti
Externí odkaz:
http://arxiv.org/abs/2305.17228
Autor:
Maguire, Cathal, Gibson, Neale P., Nugroho, Stevanus K., Ramkumar, Swaetha, Fortune, Mark, Merritt, Stephanie R., de Mooij, Ernst
Recent progress in high-resolution transmission spectroscopy has offered new avenues in which to characterise the atmospheres of transiting exoplanets. High-resolution cross-correlation spectroscopy allows for the unambiguous detection of molecules/a
Externí odkaz:
http://arxiv.org/abs/2211.09621
High-resolution Doppler-resolved spectroscopy has presented new opportunities for studying the atmospheres of exoplanets. While the 'classical' cross-correlation approach has proven to be efficient at finding atmospheric species, it is unable to perf
Externí odkaz:
http://arxiv.org/abs/2201.04025
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Akademický článek
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Publikováno v:
Monthly Notices of the Royal Astronomical Society; 5/30/2022, Vol. 512 Issue 3, p4618-4638, 21p