Poster + Paper
29 August 2022 The BlueMUSE calibration unit: phase-A studies
Author Affiliations +
Conference Poster
Abstract
BlueMUSE is a novel instrument under development for the ESO VLT, that builds on the legacy of MUSE, however with a blue wavelength range, a larger field-of-view (FoV), and higher spectral resolution. Driven by high-profile and unique science cases, the requirements present new challenges to the development of the instrument, although the fundamental layout will be based on the successful modular structure of the classical MUSE. In order to achieve the expected mean spectral resolution of R=3600 and radial velocity measurement accuracy of better than 1 km/s, as well as spectrophotometric performance, BlueMUSE must be equipped with a calibration unit to perform accurate wavelength, flat-field, and geometrical calibration. Lessons learned from MUSE show that the variation of the line-spread-function (LSF) across the FoV as a consequence of the field-splitter and image slicer layout requires a methodology to accurately measure the LSF as a function of x and y. Moreover, classical spectral line lamps that have been used traditionally for wavelength calibration present the problem of a scarce emission line coverage in the blue. BlueMUSE has entered pre-Phase-A in 2022. We report first results from conceptual design studies to address these challenges, in particular concepts of Fabry-Perot based tunable frequency combs, and as an alternative approach novel concepts with laser frequency combs or micro-ring resonator based combs in the blue.
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Martin M. Roth, Peter M. Weilbacher, Andreas Kelz, Kalaga Madhav, Eloy Hernandez, Johan Richard, Rémy Giroud, and Roland Bacon "The BlueMUSE calibration unit: phase-A studies", Proc. SPIE 12184, Ground-based and Airborne Instrumentation for Astronomy IX, 121845S (29 August 2022); https://doi.org/10.1117/12.2629630
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KEYWORDS
Calibration

Fabry–Perot interferometers

Lamps

Frequency combs

Spectrographs

Telescopes

Velocity measurements

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