Presentation + Paper
13 December 2020 Second generation spectroscopic instrumentation for the STELLA robotic observatory
Author Affiliations +
Abstract
The current STELLA Échelle spectrograph (SES), which records 390nm to 870nm in one shot at a spectral resolution of 55000, will be replaced by a suite of specialized spectrographs in three spectral bands. The UV will be covered by a newly designed H and K spectrograph covering 380nm to 470nm (SES-H and K), the visual band (470nm - 690 nm) will be covered by SES-VIS, which is a vacuum-stabilized spectrograph designed for high radial-velocity accuracy, and the NIR will be covered by the current SES spectrograph from 690nm to 1050 nm. In order to improve the UV transmission, and to accommodate three different fibre-feeds, the prime focus corrector of the telescope will be refurbished, leading to an optical system with the f/2 1200mm spherical primary, a 4-lens collimator with 2" aperture, atmospheric dispersion corrector (ADC), and two dichroic beam splitters, feeding 3 separate fibre feeds for the three bands. The newly designed H and K spectrograph will be an Échelle spectrograph, based on a R4-grating with 41.6 l/mm and 110mmx420mm, using a f/5 camera and the cross-disperser in double pass (as in TRAFICOS, MIKE, KPF), using 21 spectral orders. The spectral resolution of all three spectrographs will be comparable to the current SES's 55000.
Conference Presentation
© (2020) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Michael Weber, Manfred Woche, Klaus G. Strassmeier, Ilya Ilyin, and Arto Järvinen "Second generation spectroscopic instrumentation for the STELLA robotic observatory", Proc. SPIE 11449, Observatory Operations: Strategies, Processes, and Systems VIII, 114490J (13 December 2020); https://doi.org/10.1117/12.2562368
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KEYWORDS
Spectrographs

Observatories

Robotics

Spectroscopes

Spectral resolution

Ultraviolet radiation

Spherical lenses

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