Domenico Tiziani / ctools

Commit 6c570e24591ba308b3c317bde7554049663c37c2

Authored by Jürgen Knödlseder
1 parent 63480218

Update reference manual.

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Showing 7 changed files with 27 additions and 19 deletions
doc/source/reference_manual/cscaldb.rst
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1 -.. _cscaldb: cscaldb ======= Dumps available instrument response functions. Synopsis -------- This scripts dumps all instrument response functions that are available in the calidation database into a log file. General parameters ------------------ None Standard parameters ------------------- ``(chatter = 2) [integer]`` Verbosity of the executable: chatter = 0: no information will be logged chatter = 1: only errors will be logged chatter = 2: errors and actions will be logged chatter = 3: report about the task execution chatter = 4: detailed report about the task execution ``(clobber = yes) [boolean]`` Specifies whether an existing output counts cube should be overwritten. ``(debug = no) [boolean]`` Enables debug mode. In debug mode the executable will dump any log file output to the console. ``(mode = ql) [string]`` Mode of automatic parameters (default is "ql", i.e. "query and learn"). Related tools ------------- None  
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  2 +.. _cscaldb: cscaldb ======= Dumps all available instrument response functions into log fil. Synopsis -------- This scripts dumps all instrument response functions that are available in the calibration database into the log file. If you want the information on the screen, add the ``debug=yes`` parameter. General parameters ------------------ None Standard parameters ------------------- ``(chatter = 2) [integer]`` Verbosity of the executable: chatter = 0: no information will be logged chatter = 1: only errors will be logged chatter = 2: errors and actions will be logged chatter = 3: report about the task execution chatter = 4: detailed report about the task execution ``(clobber = yes) [boolean]`` Specifies whether an existing output counts cube should be overwritten. ``(debug = no) [boolean]`` Enables debug mode. In debug mode the executable will dump any log file output to the console. ``(mode = ql) [string]`` Mode of automatic parameters (default is "ql", i.e. "query and learn"). Related tools ------------- None
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doc/source/reference_manual/cslightcrv.rst
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@@ -9,7 +9,16 @@ Computes a lightcurve for a given source. @@ -9,7 +9,16 @@ Computes a lightcurve for a given source.
9 Synopsis 9 Synopsis
10 -------- 10 --------
11 11
12 -Computes a lightcurve for a given source. 12 +Computes a lightcurve by performing a maximum likekihood fit in a series of
  13 +time bins. The time bins can be either specified in an ASCII file, as an
  14 +interval divided into equally sized time bins, or can be taken from the Good
  15 +Time Intervals of the observation(s). The format of the ASCII file is one
  16 +row per time bin, each specifying the start of stop value of the bin, separated
  17 +by a whitespace. The times are given in Modified Julian Days (MJD).
  18 +cslightcrv writes the fitted model parameters and their statistical errors
  19 +in a FITS file. In addition, it computes for each time bin the statistical
  20 +significance of the detection, expressed by the Test Statistics, and the
  21 +upper flux limit.
13 22
14 23
15 General parameters 24 General parameters
doc/source/reference_manual/cspull.rst
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@@ -9,11 +9,11 @@ Generates pull distribution for all model parameters. @@ -9,11 +9,11 @@ Generates pull distribution for all model parameters.
9 Synopsis 9 Synopsis
10 -------- 10 --------
11 11
12 -Generates pull distributions for all parameters in a model.  
13 -The pull is defined by the fitted value minus the simulated true value,  
14 -devided by the statistical uncertainty.  
15 -For unbiased parameter estimates, the pull distribution should follow a  
16 -Gaussian centred on 0 and a sigma parameter of 1. 12 +Generates pull distributions for all parameters in a model. The pull is
  13 +defined by the fitted value minus the simulated true value, devided by
  14 +the statistical uncertainty. For unbiased parameter estimates, the pull
  15 +distribution should follow a Gaussian centred on 0 and a sigma parameter
  16 +of 1.
17 17
18 18
19 General parameters 19 General parameters
doc/source/reference_manual/cssens.rst
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@@ -11,10 +11,10 @@ Synopsis @@ -11,10 +11,10 @@ Synopsis
11 11
12 Computes the CTA sensitivity for a number of energy bins using :doc:`ctlike`. 12 Computes the CTA sensitivity for a number of energy bins using :doc:`ctlike`.
13 Crab spectra are fitted in narrow energy bins to simulated data, and the 13 Crab spectra are fitted in narrow energy bins to simulated data, and the
14 -flux level is determined that leads to a particular significance.  
15 -The significance is estimated using the Test Statistic value.  
16 -The simplified assumption is made that the significance (in Gaussian  
17 -sigma) is the square root of the Test Statistic. 14 +flux level is determined that leads to a particular significance. The
  15 +significance is estimated using the Test Statistic value. The simplified
  16 +assumption is made that the significance (in Gaussian sigma) is the square
  17 +root of the Test Statistic.
18 18
19 19
20 General parameters 20 General parameters
doc/source/reference_manual/cstsdist.rst
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@@ -9,8 +9,8 @@ Generates the TS distribution for a particular model. @@ -9,8 +9,8 @@ Generates the TS distribution for a particular model.
9 Synopsis 9 Synopsis
10 -------- 10 --------
11 11
12 -Generates the Test Statistics (TS) distribution for a particular model based on  
13 -Monte-Carlo simulations. 12 +Generates the Test Statistics (TS) distribution for a particular model
  13 +based on Monte-Carlo simulations.
14 14
15 15
16 General parameters 16 General parameters
doc/source/reference_manual/ctbin.rst
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@@ -10,9 +10,8 @@ Synopsis @@ -10,9 +10,8 @@ Synopsis
10 -------- 10 --------
11 11
12 This tool computes the counts cube for use in a binned maximum likelihood 12 This tool computes the counts cube for use in a binned maximum likelihood
13 -analysis.  
14 -The counts cubes are 3-dimensional data cubes spanned by Right Ascension or  
15 -Galactic longitude, Declination or Galactic latitude, and energy. 13 +analysis. The counts cubes are 3-dimensional data cubes spanned by Right
  14 +Ascension or Galactic longitude, Declination or Galactic latitude, and energy.
16 The energy binning may be either linear, logarithmic, or custom defined. 15 The energy binning may be either linear, logarithmic, or custom defined.
17 If an observation definition XML file containing several observations is 16 If an observation definition XML file containing several observations is
18 provided on input, the tool will stack all data into a single counts cube. 17 provided on input, the tool will stack all data into a single counts cube.
doc/source/reference_manual/ctmodel.rst
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@@ -9,9 +9,9 @@ Computes model counts cube. @@ -9,9 +9,9 @@ Computes model counts cube.
9 Synopsis 9 Synopsis
10 -------- 10 --------
11 11
12 -This tool computes a model counts cube based on an XML model.  
13 -The counts cube is a 3-dimensional data cube spanned by Right Ascension or  
14 -Galactic longitude, Declination or Galactic latitude, and energy. 12 +This tool computes a model counts cube based on an XML model. The counts
  13 +cube is a 3-dimensional data cube spanned by Right Ascension or Galactic
  14 +longitude, Declination or Galactic latitude, and energy.
15 15
16 16
17 General parameters 17 General parameters