Changes between Version 2 and Version 3 of DatabaseBasedAnalysis/calcsource

Timestamp:

09/02/18 14:49:16 (7 years ago)

Author:

tbretz

Comment:

--

DatabaseBasedAnalysis/calcsource

@@ -9 +9 @@
 == Getting the source ==
 
-The tool then requests right ascension and declination of the source observed with a given run by the following query:
+The tool then requests right ascension and declination of the source observed with a given run (Source.*) and the pointing position of the telescope (RunInfo.*) by the following query:
 
 {{{#!sql
 SELECT 
+    RunInfo.fRightAscension, 
+    RunInfo.fDeclination, 
     Source.fRightAscension, 
     Source.fDeclination, 
@@ -32 +34 @@
 == Getting events ==
 
-Then, a list of all event times and the pointing position in terms of right ascension/declination together with the corresponding event number is obtained for the given run by
+Then, a list of all event times together with the corresponding event number is obtained for the given run by
 {{{#!sql
 SELECT 
-    `Ra`, 
-    `Dec`, 
     MJD, 
     MilliSec, 
-    NanoSec, 
     EvtNumber
 FROM 
-    Events
+    Images
 WHERE 
     FileId=YYMMDDNNN
 }}}
 
-The FileId comes again from the command line argument. The table name for the '''Events''' table can be altered by `--table.events`.
+The FileId comes again from the command line argument. The table name for the '''Images''' table can be altered by `--table.events`.
 
 For source and pointing position, zenith distance and azimuth is calculated using `libnova` and the wrapper `Nova::GetHrzFromEqu`. The result is then rotated into the camera and projected on a plane which gives the x/y coordinates in the camera.