Project Details
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Transmission Spectroscopy of Extrasolar Planets

Applicant Dr. Andreas Schweitzer, since 7/2021
Subject Area Astrophysics and Astronomy
Term from 2017 to 2022
Project identifier Deutsche Forschungsgemeinschaft (DFG) - Project number 362051986
 
Final Report Year 2023

Final Report Abstract

The project focuses on high-resolution spectroscopy and its applications in the context of exoplanetary atmospheres. The primary data sources are the CARMENES spectrograph at Calar Alto Observatory in Spain and the new CRIRES+ spectrograph at ESO’s VLT. Both instruments operate primarily in the nearinfrared domain, with CARMENES extending its capabilities to encompass the red portion of the visible wavelength range. To extract the extremely weak planetary signals present in the spectra of extrasolar planetary systems, the data must be carefully processed. One of the primary challenges in this process is addressing telluric contamination, which arises from the interaction between radiation emitted by celestial objects and Earth’s atmosphere. A new technique, named Template Division Telluric Modeling (TDTM), has been developed to effectively mitigate this issue. TDTM separates telluric and stellar spectral components and has been integrated into the CARMENES data reduction pipeline. With the implementation of this accurate telluric correction, significant advancements have been made possible in the field of exoplanetary atmospheric characterization. Contributions could be made to the indepth analysis of planetary atmospheres using atomic lines such as the Hydrogen-alpha (Hα) line, the Helium I triplet at 1083 nm, and the Ca IRT lines, as exemplified by studies of HAT-P-32 b, GJ 1214 b, or WASP-76 b. Additionally, contributions to numereous published studies targeting planetary and stellar spectroscopy could be achieved.

Publications

 
 

Additional Information

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