Description: The applies a correction to the results of a query of the for various survey-specific factors, e.g., sky brightness variations, seeing variations, survey coverage variations, etc. For survey coverage variations, this could come in the form of masks built on knowledge of the survey coverage or survey depth. Basic Course: Invoke Acquire Survey Coverage Masks Alternate Course: No correction for survey effects is required. Create Cleaned Color-Magnitude Diagram WBS 02C.05.02 Data Analysis and Visualization Tools DESCRIPTION: Create Cleaned Color-Magnitude Diagram BASIC COURSE: User requests Cleaned Color-Magnitude Diagram System obtains Luminosity Function (LF) of unresolved galaxies cleans faint part of the CMD (statistically) using the LF of unresolved galaxies displays the Create Color Magnitude Result Screen which contains the URL pointer to the files and/or diagram with the CMD
Description: The applies a correction to the results of a query of the for various survey-specific factors, e.g., sky brightness variations, seeing variations, survey coverage variations, etc. For survey coverage variations, this could come in the form of masks built on knowledge of the survey coverage or survey depth. Basic Course: Invoke Acquire Survey Coverage Masks Alternate Course: No correction for survey effects is required. Create Cleaned Color-Magnitude Diagram WBS 02C.05.02 Data Analysis and Visualization Tools DESCRIPTION: Create Cleaned Color-Magnitude Diagram BASIC COURSE: User requests Cleaned Color-Magnitude Diagram System obtains Luminosity Function (LF) of unresolved galaxies cleans faint part of the CMD (statistically) using the LF of unresolved galaxies displays the Create Color Magnitude Result Screen which contains the URL pointer to the files and/or diagram with the CMD