Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12666/210
Title: HORuS transmission spectroscopy of 55 Cnc e
Authors: Tabernero, H. M.
Allende Prieto, C.
Zapatero Osorio, M. R.
González Hernández, J. I.
Del Burgo, C.
García López, Ramón
Rebolo, R.
Abril Abril, M.
Calvo Tovar, J.
Díaz Torres, A.
Fernández Izquierdo, P.
Gómez Reñasco, M. F.
Gracia Témich, F.
Joven, E.
Peñate Castro, J.
Santana Tschudi, S.
Tenegi, F.
Viera Martín, H. D.
Keywords: Planets and satellites: atmospheres;Planets and satellites: individual: 55 Cnc e
Issue Date: 26-Aug-2020
Publisher: Oxford Academics: Blackwell Publishing
DOI: 10.1093/mnras/staa2583
Published version: https://academic.oup.com/mnras/article-abstract/498/3/4222/5897379
Citation: Monthly Notices of the Royal Astronomical Society 498(3): 4222-4229(2020)
Abstract: The High Optical Resolution Spectrograph (HORuS) is a new high-resolution echelle spectrograph available on the 10.4-m Gran Telescopio Canarias (GTC). We report on the first HORuS observations of a transit of the super-Earth planet 55 Cnc e. We investigate the presence of Na I and Hα in its transmission spectrum and explore the capabilities of HORuS for planetary transmission spectroscopy. Our methodology leads to residuals in the difference spectrum between the in-transit and out-of-transit spectra for the Na I doublet lines of (3.4 ± 0.4) × 10−4, which sets an upper limit to the detection of line absorption from the planetary atmosphere that is one order of magnitude more stringent that those reported in the literature. We demonstrate that we are able to reach the photon-noise limit in the residual spectra using HORuS to a degree that we would be able to easily detect giant planets with larger atmospheres. In addition, we modelled the structure, chemistry, and transmission spectrum of 55 Cnc e using state-of-the-art open source tools.
URI: http://hdl.handle.net/20.500.12666/210
E-ISSN: 1365-2966
ISSN: 0035-8711
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