OSIRIS Calibration Scan Analysis | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
BackgroundThe OSIRIS Data Reduction Pipeline (DRP) converts raw 2-d images into 3-d datacubes via rectification matrices (recmats). Recmats are created by combining 30 (broadband) or 62 (narrowband) calibration scans that illuminate a single column of lenslets. Occasionally, a set of scans is "bad" due to uneven illumination or a misaligned slitmask stage. We analyze these raw scans and show the results below. Good scans have a constant value or vary continuously across the illuminated lenslets. Click on a link for your filter and scale combination to see recent scans. ContentsLinks
OSIRIS Calibration ScansCALSCANS - Scan Analysis
| ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
Last modified: 06/02/2013 07:06 Send questions or comments to:OSIRIS Support |