HST PanCET programme: a flat optical transmission spectrum for the Hot Jupiter WASP-101b

Autor: Alexander D Rathcke, Lars A Buchhave, João M Mendonça, David K Sing, Mercedes López-Morales, Munazza K Alam, Gregory W Henry, Nikolay K Nikolov, A García Muñoz, Thomas Mikal-Evans, Hannah R Wakeford, Leonardo A Dos Santos, Vinesh Maguire Rajpaul

Publikováno v: Rathcke, A D, Buchhave, L A, Mendonça, J M, Sing, D K, López-Morales, M, Alam, M K, Henry, G W, Nikolov, N K, Muñoz, A G, Mikal-Evans, T, Wakeford, H R, Dos Santos, L A & Rajpaul, V M 2023, ' HST PanCET programme : a flat optical transmission spectrum for the Hot Jupiter WASP-101b ', Monthly Notices of the Royal Astronomical Society, vol. 522, no. 1, pp. 582-594 . https://doi.org/10.1093/mnras/stad1010

We present an optical transmission spectrum of the hot Jupiter WASP-101b. We observed three primary transits with Hubble Space Telescope (HST)/Space Telescope Imaging Spectrograph, covering a wavelength range from 0.3 to 1 $\mu$m. The observations su

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8926953daa053d62af71caba15308b73
https://doi.org/10.1093/mnras/stad1010

Dry or water world? How the water contents of inner sub-Neptunes constrain giant planet formation and the location of the water ice line

Autor: Aaron Bello-Arufe, Bertram Bitsch, Aaron David Schneider, Alexander D. Rathcke, Lars A. Buchhave, Sean N. Raymond

Publikováno v: Bitsch, B, Raymond, S N, Buchhave, L A, Bello-Arufe, A, Rathcke, A D & Schneider, A D 2021, ' Dry or water world? How the water contents of inner sub-Neptunes constrain giant planet formation and the location of the water ice line ', Astronomy and Astrophysics, vol. 649, L5 . https://doi.org/10.1051/0004-6361/202140793
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 649, pp.L5. ⟨10.1051/0004-6361/202140793⟩
Astronomy & Astrophysics
Bitsch, B, Raymond, S N, Buchhave, L A, Bello-Arufe, A, Rathcke, A D & Schneider, A D 2021, ' Dry or water world? How the water contents of inner sub-Neptunes constrain giant planet formation and the location of the water ice line ', Astronomy & Astrophysics, vol. 649, A5 . https://doi.org/10.1051/0004-6361/202140793

In the pebble accretion scenario, the pebbles that form planets drift inward from the outer disk regions, carrying water ice with them. At the water ice line, the water ice on the inward drifting pebbles evaporates and is released into the gas phase,

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::babf894e2e2d571b511ee49e82771f46
https://orbit.dtu.dk/en/publications/7efafd02-fea8-45e1-907e-6c14e47db1f3

Transmission Spectroscopy of WASP-79b from 0.6 to 5.0 μm

Autor: Gregory W. Henry, Mark S. Marley, Rahul Jayaraman, Brian Kilpatrick, Alain Lecavelier des Etangs, Joseph C. Filippazzo, David K. Sing, Jorge Sanz-Forcada, Mercedes Lopez-Morales, Kevin B. Stevenson, David Ehrenreich, Antonio García Muñoz, Nikolay Nikolov, Jonathan Fraine, Nikole K. Lewis, Hannah R. Wakeford, Kristin S. Sotzen, Panayotis Lavvas, Lars A. Buchhave, Alexander D. Rathcke, Sarah M. Hörst

Publikováno v: Sotzen, K S, Stevenson, K B, Sing, D K, Kilpatrick, B M, Wakeford, H R, Filippazzo, J C, Lewis, N K, Hörst, S M, López-Morales, M, Henry, G W, Buchhave, L A, Ehrenreich, D, Fraine, J D, García Muñoz, A, Jayaraman, R, Lavvas, P, des Etangs, A L, Marley, M S, Nikolov, N, Rathcke, A D & Sanz-Forcada, J 2020, ' Transmission Spectroscopy of WASP-79b from 0.6 to 5.0 μm ', Astrophysical Journal, vol. 159, no. 1, 5 . https://doi.org/10.3847/1538-3881/ab5442
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Instituto Nacional de Técnica Aeroespacial (INTA)
Universidad de Alicante (UA)
The Astronomical Journal
The Astronomical Journal, American Astronomical Society, 2020, 159 (1), pp.5. ⟨10.3847/1538-3881/ab5442⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname

As part of the Panchromatic Exoplanet Treasury program, we have conducted a spectroscopic study of WASP-79b, an inflated hot Jupiter orbiting an F-type star in Eridanus with a period of 3.66 days. Building on the original WASP and TRAPPIST photometry

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a84c8ec84ec4cc41402fab4ac628f98a
https://hdl.handle.net/20.500.12666/411