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Journal of Undergraduate Research

Keywords

LBN434, clear seeing, high galactic latitudes, nebula

College

Physical and Mathematical Sciences

Department

Physics and Astronomy

Abstract

We recorded three to four images of each section of the nebula. Each group of images was identical in the data recorded; thus, after reduction, the individual images of each group could be combined directly to yield a higher intensity signal output. To reduce the data, I performed the following ~tandard CCD procedures: 1. Bad Pixel Corrections

2. Overscan Corrections

3. Zeroing and Trimming

4. Flat Fielding Corrections

Included in

Physics Commons

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