Paper
21 September 2012 The spectro-photometric calibration of the JWST NIRSpec instrument
T. Böker, S. Birkmann, G. de Marchi, P. Ferruit, G. Giardino, M. Sirianni, T. Beck
Author Affiliations +
Abstract
NIRSpec is the main near-infrared spectrograph on board the James Webb Space Telescope, offering multi-object capabilities as well as an integral field unit and a number of fixed slits for studies of individual objects. In this paper, we describe the unique challenges in calibrating this complex instrument, and the approach taken to deal with them, both in terms of operational procedures and via automated processing of NIRSpec data. We provide a high-level description of the sequence of processing steps required for NIRSpec science data, and the necessary on-ground calibration files. We focus our discussion on the case of a typical multi-object observation with the MSA, in which adjacent micro-shutters are used to sample the science object and the sky background in an alternating way. This dithering strategy is particularly well suited for faint targets, but its guiding principles also apply to other NIRSpec modes.
© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
T. Böker, S. Birkmann, G. de Marchi, P. Ferruit, G. Giardino, M. Sirianni, and T. Beck "The spectro-photometric calibration of the JWST NIRSpec instrument", Proc. SPIE 8442, Space Telescopes and Instrumentation 2012: Optical, Infrared, and Millimeter Wave, 84423F (21 September 2012); https://doi.org/10.1117/12.925369
Lens.org Logo
CITATIONS
Cited by 3 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Calibration

Sensors

Camera shutters

Space telescopes

James Webb Space Telescope

Spectral calibration

Telescopes

RELATED CONTENT

Overview of the VLT instrumentation
Proceedings of SPIE (July 09 1998)
Guide, focus/alignment system for BigBOSS
Proceedings of SPIE (September 13 2012)
Modeling of spectroscopic astronomical observations
Proceedings of SPIE (June 01 1994)
Deep fiber spectroscopy
Proceedings of SPIE (July 01 1990)

Back to Top