Submission Type
Event
Expected Graduation Date
2015
Location
Atrium, Center for Natural Sciences, Illinois Wesleyan University
Start Date
4-20-2013 9:00 AM
End Date
4-20-2013 10:00 AM
Disciplines
Physics
Abstract
The study of very distant “dusty” galaxies whose visible light is obscured by cosmic dust is a developing field in astronomy. To discover such galaxies, images of the sky are made with telescopes sensitive to millimeter-wavelength light. Because these images are inherently low in signal-to-noise, special image processing techniques are needed to reliably identify galaxies in them. Usually, a software “filter” is applied to a sky image in order to better distinguish galaxies from noise. We have developed a novel filter that, in principle, performs better than the standard filter used in the astronomical community. Our study, which involved testing this new filter, is presented here. This is a continuation of an improvement over work previously presented in 2010.
Included in
Tests of a Novel Technique for Finding Galaxies in Millimeter Wavelength Maps
Atrium, Center for Natural Sciences, Illinois Wesleyan University
The study of very distant “dusty” galaxies whose visible light is obscured by cosmic dust is a developing field in astronomy. To discover such galaxies, images of the sky are made with telescopes sensitive to millimeter-wavelength light. Because these images are inherently low in signal-to-noise, special image processing techniques are needed to reliably identify galaxies in them. Usually, a software “filter” is applied to a sky image in order to better distinguish galaxies from noise. We have developed a novel filter that, in principle, performs better than the standard filter used in the astronomical community. Our study, which involved testing this new filter, is presented here. This is a continuation of an improvement over work previously presented in 2010.