New deep ugr imaging was obtained on the Wyoming Infrared Observatory 2.3 meter telescope for NGC4102 and UGC07608, two galaxies in the Extended Disk Galaxy Exploration Science survey. These data are coupled with deep GALEX ultraviolet and Spitzer, WISE and Herschel infrared imaging to study the radial variations in the spectral energy distributions. Results from the CIGALE SED modeling software are presented, including trends in the galaxy star formation histories.
Identifer | oai:union.ndltd.org:ETSU/oai:dc.etsu.edu:asrf-1340 |
Date | 12 April 2019 |
Creators | Cox, Isaiah S, Anderson, Kristin R, Bran, Loius M, Drake, Carolyn L, Lee, Nathan J, Pilawa, Jacob D, Slane, Frederick A, Soto, Susana, Jensen, Emily I, Sutter, Jessica S, Turner, Jordan A, Kobulnicky, Henry A, Dale, Daniel A |
Publisher | Digital Commons @ East Tennessee State University |
Source Sets | East Tennessee State University |
Detected Language | English |
Type | text |
Source | Appalachian Student Research Forum |
Page generated in 0.0018 seconds