He I λ 10 830 Å in the transmission spectrum of HD209458 b

The error is an approximation obtained from the average transmission spectrum provided by Allart et al. (2018). Program H18-3.5-022, P.I: S. Czesla. After one year from the observation date, the reduced spectra can be downloaded from the Calar Alto archive, http://caha.sdc.cab.inta-csic.es/calto/ ht...

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Detalhes bibliográficos
Autores: Alonso Floriano, F. J., Snellen, Ignas, Czesla, S., Bauer, F. F., Salz, M., Lampón, M., Lara, L. M., Nagel, E., López Puertas, M., Nortmann, L., Sánchez López, A., Sanz-Forcada, Jorge, Caballero, J. A., Reiners, A., Ribas, I., Quirrenbach, A., Amado, P. J., Aceituno, J., Anglada Escudé, G., Béjar, V. J. S., Brinkmöller, M., Hatzes, Artie, Henning, T., Kaminski, A., Kürster, M., Labarga, F., Montes, D., Pallé, E., Schmitt, J. H. M. M., Zapatero Osorio, María Rosa
Formato: artículo
Estado:Versión publicada
Fecha de publicación:2019
País:España
Recursos:Instituto Nacional de Técnica Aeroespacial (INTA)
Repositorio:DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
OAI Identifier:oai:digital.inta.es:20.500.12666/363
Acesso em linha:https://www.aanda.org/articles/aa/full_html/2019/09/aa35979-19/aa35979-19.html
http://hdl.handle.net/20.500.12666/363
Access Level:acceso abierto
Palavra-chave:Planets and satellites: atmospheres
Planets and satellites: individual: HD 209458b
Techniques: spectroscopic
Infrared: planetary systems
Descrição
Resumo:The error is an approximation obtained from the average transmission spectrum provided by Allart et al. (2018). Program H18-3.5-022, P.I: S. Czesla. After one year from the observation date, the reduced spectra can be downloaded from the Calar Alto archive, http://caha.sdc.cab.inta-csic.es/calto/ https://www.nist.gov/pml/atomic-spectra-database

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