Paper
13 September 2012 The slitmask alignment tool: robust, efficient, and astronomer-friendly software for aligning multi-object slitmasks
Author Affiliations +
Abstract
Multi-object spectroscopy via custom slitmasks is a key capability on three instruments at the W. M. Keck Observatory. Before observers can acquire spectra they must complete a complex procedure to align each slit with its corresponding science target. We developed the Slitmask Alignment Tool (SAT), to replace a complex, inefficient, and error-prone slitmask alignment process that often resulted in lost sky time for novice and experienced observers alike. The SAT accomplishes rapid initial mask alignment, prevents field misidentification, accurately predicts alignment box image locations, corrects for flexure-induced image displacement, verifies the instrument and exposure configuration, and accommodates both rectangular and trapezoidal alignment box shapes. The SAT is designed to lead observers through the alignment process and coordinate image acquisition with instrument and telescope moves to improve efficiencies. By simplifying the process to just a few mouse clicks, the SAT enables even novice observers to achieve robust, efficient, and accurate alignment of slitmasks on all three Keck instruments supporting multislit spectroscopy, saving substantial observing time.
© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Marc Kassis, Gregory D. Wirth, Andrew C. Phillips, and Charles C. Steidel "The slitmask alignment tool: robust, efficient, and astronomer-friendly software for aligning multi-object slitmasks", Proc. SPIE 8448, Observatory Operations: Strategies, Processes, and Systems IV, 844807 (13 September 2012); https://doi.org/10.1117/12.926693
Lens.org Logo
CITATIONS
Cited by 1 scholarly publication.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Stars

Telescopes

Image processing

Spectrographs

Astronomical imaging

Image acquisition

Sensors

Back to Top