Detection of Na in the atmosphere of the hot Jupiter HAT-P-55b
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arXiv
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| Autori principali: | , , , , , , , , |
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| Natura: | Preprint |
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2024
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| _version_ | 1866917704197210112 |
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| author | Kang, Huiyi Chen, Guo Jiang, Chengzi Palle, Enric Murgas, Felipe Parviainen, Hannu Ma, Yuehua Fukui, Akihiko Narita, Norio |
| author_facet | Kang, Huiyi Chen, Guo Jiang, Chengzi Palle, Enric Murgas, Felipe Parviainen, Hannu Ma, Yuehua Fukui, Akihiko Narita, Norio |
| contents | The spectral signatures of optical absorbers, when combined with those of infrared molecules, play a critical role in constraining the cloud properties of exoplanet atmospheres. We aim to use optical transmission spectroscopy to confirm the tentative color signature previously observed by multiband photometry in the atmosphere of hot Jupiter HAT-P-55b. We observed a transit of HAT-P-55b with the OSIRIS spectrograph on the Gran Telescopio Canarias (GTC). We created two sets of spectroscopic light curves using the conventional band-integrated method and the newly proposed pixel-based method to derive the transmission spectrum. We performed Bayesian spectral retrieval analyses on the transmission spectrum to interpret the observed atmospheric properties. The transmission spectra derived from the two methods are consistent, both spectrally resolving the tentative color signature observed by MuSCAT2. The retrievals on the combined OSIRIS and MuSCAT2 transmission spectrum yield the detection of Na at 5.5$σ$ and the tentative detection of MgH at 3.4$σ$. The current optical-only wavelength coverage cannot constrain the absolute abundances of the atmospheric species. Space-based observations covering the molecular infrared bands or ground-based high-resolution spectroscopy are needed to further constrain the atmospheric properties of HAT-P-55b. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2404_13849 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Detection of Na in the atmosphere of the hot Jupiter HAT-P-55b Kang, Huiyi Chen, Guo Jiang, Chengzi Palle, Enric Murgas, Felipe Parviainen, Hannu Ma, Yuehua Fukui, Akihiko Narita, Norio Earth and Planetary Astrophysics The spectral signatures of optical absorbers, when combined with those of infrared molecules, play a critical role in constraining the cloud properties of exoplanet atmospheres. We aim to use optical transmission spectroscopy to confirm the tentative color signature previously observed by multiband photometry in the atmosphere of hot Jupiter HAT-P-55b. We observed a transit of HAT-P-55b with the OSIRIS spectrograph on the Gran Telescopio Canarias (GTC). We created two sets of spectroscopic light curves using the conventional band-integrated method and the newly proposed pixel-based method to derive the transmission spectrum. We performed Bayesian spectral retrieval analyses on the transmission spectrum to interpret the observed atmospheric properties. The transmission spectra derived from the two methods are consistent, both spectrally resolving the tentative color signature observed by MuSCAT2. The retrievals on the combined OSIRIS and MuSCAT2 transmission spectrum yield the detection of Na at 5.5$σ$ and the tentative detection of MgH at 3.4$σ$. The current optical-only wavelength coverage cannot constrain the absolute abundances of the atmospheric species. Space-based observations covering the molecular infrared bands or ground-based high-resolution spectroscopy are needed to further constrain the atmospheric properties of HAT-P-55b. |
| title | Detection of Na in the atmosphere of the hot Jupiter HAT-P-55b |
| topic | Earth and Planetary Astrophysics |
| url | https://arxiv.org/abs/2404.13849 |