Journal
ASTRONOMICAL JOURNAL
Volume 144, Issue 2, Pages -Publisher
IOP PUBLISHING LTD
DOI: 10.1088/0004-6256/144/2/68
Keywords
galaxies: fundamental parameters; galaxies: statistics; infrared: galaxies; surveys; techniques: image processing
Categories
Funding
- NASA
- NASA Postdoctoral Program at the Jet Propulsion Laboratory
- National Aeronautics and Space Administration
- Direct For Mathematical & Physical Scien
- Division Of Astronomical Sciences [909159] Funding Source: National Science Foundation
Ask authors/readers for more resources
After eight months of continuous observations, the Wide-field Infrared Survey Explorer (WISE) mapped the entire sky at 3.4 mu m, 4.6 mu m, 12 mu m, and 22 mu m. We have begun a dedicated WISE High Resolution Galaxy Atlas project to fully characterize large, nearby galaxies and produce a legacy image atlas and source catalog. Here we summarize the deconvolution techniques used to significantly improve the spatial resolution of WISE imaging, specifically designed to study the internal anatomy of nearby galaxies. As a case study, we present results for the galaxy NGC 1566, comparing the WISE enhanced-resolution image processing to that of Spitzer, Galaxy Evolution Explorer, and ground-based imaging. This is the first paper in a two-part series; results for a larger sample of nearby galaxies are presented in the second paper.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available