diff --git a/doc/source/users/reference_manual/csbkgmodel.rst b/doc/source/users/reference_manual/csbkgmodel.rst index e2dc787..d243486 100755 --- a/doc/source/users/reference_manual/csbkgmodel.rst +++ b/doc/source/users/reference_manual/csbkgmodel.rst @@ -18,12 +18,12 @@ For the analytical 2D Gaussian function, a bilinear multiplicative background gradient can be added using ``gradient=yes``. The spectral component can be either a power law (``PLAW``) or a nodes function (``NODES``). The number of nodes for the node function is controlled through the ``enumbins`` parameter. -Specific node energies can be specified through the ``ebinalg`` parameter. +Specific node energies can be specified through the ``ebinfile`` parameter. If ``runwise=yes``, a background model component will be added for each observation in the input observation definition XML file. The script fits the background model to the input observation(s) to preset the background model parameters -with resonable values. +with reasonable values. On output, :ref:`csbkgmodel` writes an model definition XML file that can be used for model fitting. Source model components have to be added as needed. diff --git a/doc/source/users/reference_manual/csebins.rst b/doc/source/users/reference_manual/csebins.rst index 7dd91e2..09630c8 100755 --- a/doc/source/users/reference_manual/csebins.rst +++ b/doc/source/users/reference_manual/csebins.rst @@ -9,7 +9,7 @@ Generates energy boundaries for stacked analysis. Synopsis -------- -This script generates the energy bounaries for a stacked analysis by inspecting +This script generates the energy boundaries for a stacked analysis by inspecting the variation in the effective area and the background template of the response functions. The script takes either an observation definition XML file or a specific instrument response function on input. diff --git a/doc/source/users/reference_manual/csmodelselect.rst b/doc/source/users/reference_manual/csmodelselect.rst index 842ad6f..ab46118 100755 --- a/doc/source/users/reference_manual/csmodelselect.rst +++ b/doc/source/users/reference_manual/csmodelselect.rst @@ -9,7 +9,7 @@ Selects models from a model definition XML file. Synopsis -------- -This script selects all models from a model definiton XML file that spatially +This script selects all models from a model definition XML file that spatially overlap with the Region of Interests (RoIs) of a list of observations and writes these models into a new model definition XML file. In addition to the spatial selection, the tool allows selecting only models with a photon flux and/or a diff --git a/doc/source/users/reference_manual/csobsselect.rst b/doc/source/users/reference_manual/csobsselect.rst index 348c612..e526e51 100755 --- a/doc/source/users/reference_manual/csobsselect.rst +++ b/doc/source/users/reference_manual/csobsselect.rst @@ -9,10 +9,10 @@ Selects observations from an observation definition XML file. Synopsis -------- -This script selects all observations from an observation definiton XML file that +This script selects all observations from an observation definition XML file that have pointings within a specified selection region and time interval and writes these observations into a new observation definition XML file. Possible selection -regions are a circle and a box, either in Galactic or Celestial coordinates. +regions are a circle and a box, given either in Galactic or Celestial coordinates. General parameters diff --git a/doc/source/users/reference_manual/ctfindvar.rst b/doc/source/users/reference_manual/ctfindvar.rst index d688200..940ef11 100644 --- a/doc/source/users/reference_manual/ctfindvar.rst +++ b/doc/source/users/reference_manual/ctfindvar.rst @@ -3,7 +3,7 @@ ctfindvar ========= -Search for source variability. +Searches for source variability. Synopsis @@ -13,7 +13,7 @@ This tool searches for source variability by applying the On/Off method in the time domain. The variability of sky map pixels is computed by binning the events as function of the photon arrival time and applying the On/Off method to each time bin, integrating the background over all the other time bins. Only bins -with a variabilty significance below a given threshold, defined by the hidden +with a variability significance below a given threshold, defined by the hidden ``threshold`` parameter, are included in the background estimate. Furthermore, only time bins that exceed a minimum number of events, specified by the hidden ``minoff`` parameter, are considered for the background estimate. The significance diff --git a/doc/source/users/reference_manual/ctprob.rst b/doc/source/users/reference_manual/ctprob.rst index 18491b8..67a1c79 100755 --- a/doc/source/users/reference_manual/ctprob.rst +++ b/doc/source/users/reference_manual/ctprob.rst @@ -12,7 +12,7 @@ Synopsis This tool computes for each event the probability that the event originates from a one of the components of a model. -The tool takes on input an event list or an observation definiton XML file and +The tool takes on input an event list or an observation definition XML file and appends on output to each event file columns that provide the probabilities. The column names are formed from the model name that is prefixed with ``PROB_``.