Optical ray tracing of echelle spectrographs applied to the wavelength solution for precise radial velocities

We present moes, a ray tracing software package that computes the path of rays through echelle spectrographs. Our algorithm is based on sequential direct tracing with Seidel aberration corrections applied at the detector plane. As a test case, we model the CARMENES VIS spectrograph. After subtractin...

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Hauptverfasser: Tala, Marcelo (VerfasserIn) , Kaminski, Adrian (VerfasserIn) , Quirrenbach, Andreas (VerfasserIn) , Zechmeister, Mathias (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: April 2024
In: Journal of astronomical telescopes, instruments, and systems
Year: 2024, Jahrgang: 10, Heft: 2, Pages: 1-22
ISSN:2329-4221
DOI:10.1117/1.JATIS.10.2.028001
Online-Zugang:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1117/1.JATIS.10.2.028001
Verlag, lizenzpflichtig, Volltext: https://www.spiedigitallibrary.org/journals/Journal-of-Astronomical-Telescopes-Instruments-and-Systems/volume-10/issue-2/028001/Optical-ray-tracing-of-echelle-spectrographs-applied-to-the-wavelength/10.1117/1.JATIS.10.2.028001.full
Volltext
Verfasserangaben:Marcelo Tala Pinto, Adrian Kaminski, Andreas Quirrenbach, and Mathias Zechmeister
Beschreibung
Zusammenfassung:We present moes, a ray tracing software package that computes the path of rays through echelle spectrographs. Our algorithm is based on sequential direct tracing with Seidel aberration corrections applied at the detector plane. As a test case, we model the CARMENES VIS spectrograph. After subtracting the best model from the data, the residuals yield an rms of 0.024 pix, setting a new standard for the precision of the wavelength solution of state-of-the-art radial velocity (RV) instruments. By including the influence of the changes of the environment in ray propagation, we are able to predict instrumental RV systematics at the 1 m/s level.
Beschreibung:Veröffentlicht: 01. April 2024
Gesehen am 05.09.2025
Beschreibung:Online Resource
ISSN:2329-4221
DOI:10.1117/1.JATIS.10.2.028001