Presentation + Paper
26 August 2022 Spectrograph design for the Asgard/BIFROST spectro-interferometric instrument for the VLTI
Author Affiliations +
Abstract
The BIFROST instrument will be the first VLTI instrument optimised for high spectral resolution up to R=25,000 and operate between 1.05 and 1.7 μm. A key component of the instrument will be the spectrograph, where we require a high throughput over a broad bandwidth. In this contribution, we discuss the four planned spectral modes (R=50, R=1000, R=5000, and R=25,000), the key spectral windows that we need to cover, and the technology choices that we have considered. We present our plan to use Volume Phase Holographic Gratings (VPHGs) to achieve a high efficiency > 85%. We present our preliminary optical design and our strategies for wavelength calibration.
Conference Presentation
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Sorabh Chhabra, Michele Frangiamore, Stefan Kraus, Andrea Bianco, Francisco Garzon, John Monnier, and Daniel Mortimer "Spectrograph design for the Asgard/BIFROST spectro-interferometric instrument for the VLTI", Proc. SPIE 12183, Optical and Infrared Interferometry and Imaging VIII, 121830M (26 August 2022); https://doi.org/10.1117/12.2628805
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KEYWORDS
Spectrographs

Binary data

Diffraction gratings

Calibration

Prisms

Sensors

Spectral resolution

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