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Determine Background Counts per
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Spatial Analysis
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Determine Galactic Coordinates of
5.2 Tasks of the Spatial Analysis
Determine Background Counts per Pixel
Create Smoothed Background Image
Determine Total Field of View Background Spectrum
Create Images for Source Detection
Detect Sources using Local Background
Detect Sources using Background from Smoothed Background Image
Merging of Source Tables
Detect Sources with the Maximum Likelihood Method
Merging of Source Lists after the Maximum Likelihood Detection
All Source Detection Done with one Command
Creation of a Maximum Likelihood Image
Conversion of Source Detection Lists
Multi Source Fit to Image Data
Determine Source Counts
Determine Upper Limits for Counts
Calculate Source Count Rates
Calculate Hardness Ratios
Determine Source Extent
Determine Average Off-Axis Angle of a Source
Calculation of the Point Spread Function Probability or Quantile
Creation of a Point Spread Function Model Profile
Determine Cluster Properties
Calculate Linear Intensity Profiles
Calculate Radial Intensity Profiles
Calculate Azimuthal Intensity Profiles
Calculate Intensity Contours
Calculate Counts within a Box
Calculate Counts within a Circle
Equatorial, Ecliptic and Galactic Coordinates
Create a User defined Source Table
Plot Source List Positions
Label Source List Positions
Plot Coordinate Grids
Get Coordinates by Cursor
Screen an Image by a Mask
Sources partially obscured by the PSPC Window Support Structure
Alignment of an Image to a Reference Image
Adding a Contour Image to a Reference Image
Plotting Sources on an all-sky Aitoff Grid
Create a simulated observation
If you have problems/suggestions please send mail to
rosat_svc@mpe-garching.mpg.de
