Poster + Paper
13 December 2020 Verification observations of the Manfred Hirt Planet Spectrograph
Hanna Kellermann, Liang Wang, Vanessa Fahrenschon, Jana Steuer, Fei Zhao, Frank Grupp, Michael Schmidt, Christoph Ries, Claus Goessel, Wolfgang Mitsch, Ulrich Hopp, Ralf Bender
Author Affiliations +
Conference Poster
Abstract
The Manfred Hirt Planet Spectrograph - formerly operated under the name FOCES - started its regular scientific observation program in fall 2019 at the 2m telescope of the Wendelstein Observatory, operated by the University Observatory of the LMU Munich. We present the first radial velocity stability measurements of an astronomical target, the 51 Pegasi b exoplanet system, utilizing our Astro Frequency Comb (ACF) for wavelength calibration. For computing RV shifts from orderwisely extracted Echelle spectra we have developed a new software pipeline. In this proceeding we will introduce the most important features of our pipeline: wavelength calibration with simultaneously recorded spectra of the AFC, generation of spectral templates, and an optional fit or cross- correlation function (CCF) for the calculation of the relative RV signals. Finally, the performance of the pipeline real data is demonstrated.
© (2020) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Hanna Kellermann, Liang Wang, Vanessa Fahrenschon, Jana Steuer, Fei Zhao, Frank Grupp, Michael Schmidt, Christoph Ries, Claus Goessel, Wolfgang Mitsch, Ulrich Hopp, and Ralf Bender "Verification observations of the Manfred Hirt Planet Spectrograph", Proc. SPIE 11447, Ground-based and Airborne Instrumentation for Astronomy VIII, 114474K (13 December 2020); https://doi.org/10.1117/12.2562495
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KEYWORDS
Planets

Spectrographs

Observatories

Velocity measurements

Aluminium phosphide

Astronomy

Calibration

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