High-resolution spectroscopy
High-resolution spectroscopy (HRS) allows resolving the spectrum of an exoplanetary atmosphere into individual lines and using the Doppler shift of the planet spectrum to disentangle it from other sources, such as telluric contamination and the host star spectrum. The method excels at identifying ch...
| Main Authors: | , |
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| Other Authors: | |
| Format: | Book section |
| Language: | English |
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IOP Publishing
2021
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| _version_ | 1797106989520650240 |
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| author | Brogi, M Birkby, J |
| author2 | Madhusudhan, N |
| author_facet | Madhusudhan, N Brogi, M Birkby, J |
| author_sort | Brogi, M |
| collection | OXFORD |
| description | High-resolution spectroscopy (HRS) allows resolving the spectrum of an exoplanetary atmosphere into individual lines and using the Doppler shift of the planet spectrum to disentangle it from other sources, such as telluric contamination and the host star spectrum. The method excels at identifying chemical species with numerous spectral lines and can be used for transmission, day/night-side emission, and reflected light spectroscopy. This chapter discusses the state of the art and important questions and goals for HRS, the opportunities it offers and the challenges it faces. |
| first_indexed | 2024-03-07T07:10:16Z |
| format | Book section |
| id | oxford-uuid:17e8a1f9-670e-4531-a097-ba7b8274fc09 |
| institution | University of Oxford |
| language | English |
| last_indexed | 2024-03-07T07:10:16Z |
| publishDate | 2021 |
| publisher | IOP Publishing |
| record_format | dspace |
| spelling | oxford-uuid:17e8a1f9-670e-4531-a097-ba7b8274fc092022-06-16T11:25:05ZHigh-resolution spectroscopyBook sectionhttp://purl.org/coar/resource_type/c_1843uuid:17e8a1f9-670e-4531-a097-ba7b8274fc09EnglishSymplectic ElementsIOP Publishing2021Brogi, MBirkby, JMadhusudhan, NHigh-resolution spectroscopy (HRS) allows resolving the spectrum of an exoplanetary atmosphere into individual lines and using the Doppler shift of the planet spectrum to disentangle it from other sources, such as telluric contamination and the host star spectrum. The method excels at identifying chemical species with numerous spectral lines and can be used for transmission, day/night-side emission, and reflected light spectroscopy. This chapter discusses the state of the art and important questions and goals for HRS, the opportunities it offers and the challenges it faces. |
| spellingShingle | Brogi, M Birkby, J High-resolution spectroscopy |
| title | High-resolution spectroscopy |
| title_full | High-resolution spectroscopy |
| title_fullStr | High-resolution spectroscopy |
| title_full_unstemmed | High-resolution spectroscopy |
| title_short | High-resolution spectroscopy |
| title_sort | high resolution spectroscopy |
| work_keys_str_mv | AT brogim highresolutionspectroscopy AT birkbyj highresolutionspectroscopy |