Radial velocity accuracy prediction of the GREGOR at night spectrograph based on simulated spectra

Michael Weber; Klaus G. Strassmeier; Manfred Woche; Ilya Ilyin; Arto Järvinen

doi:10.1117/12.2311715

10 July 2018 Radial velocity accuracy prediction of the GREGOR at night spectrograph based on simulated spectra

Michael Weber, Klaus G. Strassmeier, Manfred Woche, Ilya Ilyin, Arto Järvinen

Author Affiliations +

Proceedings Volume 10705, Modeling, Systems Engineering, and Project Management for Astronomy VIII; 107051E (2018) https://doi.org/10.1117/12.2311715
Event: SPIE Astronomical Telescopes + Instrumentation, 2018, Austin, Texas, United States

Abstract

The Gregor At Night Spectrograph (GANS) is a new instrument currently being built for the GREGOR solar telescope at Iza~na observatory on Tenerife. Its primary science case will be the follow up of planetary candidates detected by upcoming surveys focussing on bright targets (TESS, PLATO2). Therefore it will be optimised for precise radial velocity determination and long term stability. We have developed a ZEMAX based software package to create simulated spectra, which are reduced using standard IRAF tasks. We used a solar model spectrum to determine the influence of S/N ratio, wavelength coverage, pixel sampling and telluric lines on the extracted radial velocities. Furthermore we derived the effect of an asymmetric spectrograph illumination on the measured radial velocity.

Citation Download Citation

Michael Weber, Klaus G. Strassmeier, Manfred Woche, Ilya Ilyin, and Arto Järvinen "Radial velocity accuracy prediction of the GREGOR at night spectrograph based on simulated spectra", Proc. SPIE 10705, Modeling, Systems Engineering, and Project Management for Astronomy VIII, 107051E (10 July 2018); https://doi.org/10.1117/12.2311715

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