High-resolution Emission Spectroscopy of the Ultrahot Jupiter KELT-9b: Little Variation in Day- and Nightside Emission Line Contrasts

0571488 - ASÚ 2024 RIV US eng J - Článek v odborném periodiku
Ridden-Harper, A. - de Mooij, E.J.W. - Jayawardhana, R. - Gibson, N. - Karjalainen, Raine - Karjalainen, Marie
High-resolution Emission Spectroscopy of the Ultrahot Jupiter KELT-9b: Little Variation in Day- and Nightside Emission Line Contrasts.
Astronomical Journal. Roč. 165, č. 5 (2023), č. článku 211. ISSN 0004-6256. E-ISSN 1538-3881
Grant CEP: GA MŠMT(CZ) LTT20015
Grant ostatní: ESA(XE) ESA-PRODEX PEA4000127913
Institucionální podpora: RVO:67985815
Klíčová slova: exoplanet atmospheres * planetary atmospheres * extrasolar gaseous giant planets
Obor OECD: Astronomy (including astrophysics,space science)
Impakt faktor: 5.3, rok: 2022
Způsob publikování: Open access

The transmission spectrum of the ultrahot Jupiter KELT-9b (T (eq) similar to 4000 K) exhibits absorption by several metal species. We searched for atomic and molecular lines in its emission spectrum by observing partial phase curves with the Calar Alto high-Resolution search for M dwarfs with Exoearths with Near-infrared and optical Echelle Spectrographs (R similar to 80,000-95,000). We find evidence for emission by Si i in the atmosphere of KELT-9b for the first time. Additionally we find evidence for emission by Mg i and Ca ii, which were previously detected in transmission, and confirmed earlier detections of Fe i emission. Conversely, we find no evidence for dayside emission from Al i, Ca i, Cr i, FeH, Fe ii, K i, Li i, Mg ii, Na i, OH, Ti i, TiO, V i, V ii, VO, and Y i. By employing likelihood mapping, we find indications of there being little variation in emission line contrast between the day- and nightsides-suggesting that KELT-9b may harbor iron emission on its nightside. Our results demonstrate that high-resolution ground-based emission spectroscopy can provide valuable insights into exoplanet atmospheres.
Trvalý link: https://hdl.handle.net/11104/0342983