Poster + Paper
18 July 2024 Stacks, maps, and all that CHαS: refined image processing methods to map the nearby universe with the Circumgalactic H-alpha Spectrograph
Author Affiliations +
Conference Poster
Abstract
The Circumgalactic H-alpha Spectrograph (CHαS) is a ground-based, narrowband optical integral field spectrograph designed to observe ultra-faint extended emission from ionized gas in the nearby universe. Commissioned for use as a facility instrument at MDM observatory, we are currently surveying nearby galaxies to produce deep H-alpha images and velocity maps, complemented with observations in other wavelengths. We present our work developing a robust analysis pipeline for CHαS, providing a toolkit to process images with densely-packed, spatially-resolved spectra. The pipeline includes techniques for astrometric refinement, wavelength mapping and distortion calibration of arrayed spectral images, as well as manipulations in Fourier space. With these, we are able to optimize our image registration and stacking procedures, sky background removal and spectral cube extraction for the tightly packed microlens array images. We highlight results using 5-10h deep image stacks and demonstrate results from cross-correlation with imaging and spectral data from other astronomical surveys.
(2024) Published by SPIE. Downloading of the abstract is permitted for personal use only.
Ignacio Cevallos-Aleman, David Schiminovich, Meghna Sitaram, Nicole Melso, Barbara Cruvinel Santiago, Nazende I. Kerkeser, Gianni Popko, and Mia Yiannias "Stacks, maps, and all that CHαS: refined image processing methods to map the nearby universe with the Circumgalactic H-alpha Spectrograph", Proc. SPIE 13096, Ground-based and Airborne Instrumentation for Astronomy X, 1309643 (18 July 2024); https://doi.org/10.1117/12.3019501
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KEYWORDS
Fourier transforms

Microlens array

Spectrographs

Galactic astronomy

Image processing

Bandpass filters

Microlens

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