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--- public:user_software:documentation:gsm.py [2016-10-11 09:08] – Document moved from engineering:software:tools:gsm.py Arno Schoenmakers
+++ public:user_software:documentation:gsm.py [2017-03-08 15:27] (current) – external edit 127.0.0.1
@@ Line 1: / Line 1: @@
 ====== gsm.py ======
-BBS needs a local sky model of the observed field. This sky model is stored in a source table created by [[public:user_software:documentation:makesourcedb]] from a text input file.
+BBS needs a local sky model of the observed field. This sky model is stored in a source table created by [[makesourcedb]] from a text input file.
 The script ''gsm.py'' can be used to extract known VLSS sources in the observed field from the GSM and store them in a text file that can directly be used as input by ''makesourcedb''. The parameters for the script need to be given at the command line. The spatial selection can be done using a cone in RA,DEC to be given in J2000.
@@ Line 6: / Line 6: @@
 The sources found will also be extracted from other catalogs (NVSS, WENSS) which are used to fit a spectral index.
-By default each source will be its own patch (see [[public:user_software:documentation:makesourcedb]]), but using the ''-p'' option it is possible to create a single patch for the sources found.
+By default each source will be its own patch (see [[makesourcedb]]), but using the ''-p'' option it is possible to create a single patch for the sources found.
 The command