Poster + Paper
29 August 2022 Final pipeline design of the MICADO spectroscopic mode
Wolfgang Kausch, Nadeen B. Sabha, Norbert Przybilla
Author Affiliations +
Conference Poster
Abstract
The Multi-AO Imaging Camera for Deep Observations (MICADO1) will be one of the first generation instruments for the Extremely Large Telescope (ELT) currently being built by the European Southern Observatory (ESO) at Cerro Armazones in the Chilean Atacama desert comprising several observing modes for a wide range of astrophysical applications. Its spectroscopic mode is an echelle design aiming for point and compact sources with a medium resolving power (R ≈ 20, 000) covering the entire I to K bands in two setups. The goal of the respective pipeline is to fully calibrate the raw data, i.e. to deliver science data products fully compliant with the Phase 3 requirements of the ESO Science Data Archive Facility. This includes the removal of the instrument signature, geometrical distortion correction, wavelength calibration and conversion to physical units (flux calibration). In addition, a comprehensive set of quality control parameters is foreseen for monitoring the instrument health and the data quality control.
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Wolfgang Kausch, Nadeen B. Sabha, and Norbert Przybilla "Final pipeline design of the MICADO spectroscopic mode", Proc. SPIE 12189, Software and Cyberinfrastructure for Astronomy VII, 121891L (29 August 2022); https://doi.org/10.1117/12.2630021
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KEYWORDS
Calibration

Spectroscopy

Algorithm development

Imaging spectroscopy

Spectral resolution

Spectroscopes

Point spread functions

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