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cscripts/cslightcrv.par
| ... | ... | @@ -39,8 +39,8 @@ emax, r, a, 100.0,,, "Upper energy limit of events (TeV)" |
| 39 | 39 | enumbins, i, a, 0,0,100, "Number of energy bins for binned (0=unbinned for Cube analysis only)" |
| 40 | 40 | coordsys, s, a, CEL,CEL|GAL,, "Coordinate System" |
| 41 | 41 | proj, s, a, CAR,AIT|AZP|CAR|GLS|MER|MOL|SFL|SIN|STG|TAN,, "Projection method" |
| 42 | -xref, r, a, 83.63,0,360, "First coordinate of image center in degrees (RA or galactic l)" | |
| 43 | -yref, r, a, 22.01,-90,90, "Second coordinate of image center in degrees (DEC or galactic b)" | |
| 42 | +xref, r, a, 83.63,0,360, "First coordinate of image/source region center in degrees (RA or galactic l)" | |
| 43 | +yref, r, a, 22.01,-90,90, "Second coordinate of image/source region center in degrees (DEC or galactic b)" | |
| 44 | 44 | nxpix, i, a, 200,,, "Size of the X axis in pixels" |
| 45 | 45 | nypix, i, a, 200,,, "Size of the Y axis in pixels" |
| 46 | 46 | binsz, r, a, 0.02,,, "Pixel size (deg/pixel)" | ... | ... |
doc/source/users/reference_manual/cslightcrv.rst
| ... | ... | @@ -70,7 +70,7 @@ General parameters |
| 70 | 70 | File defining the time binning. |
| 71 | 71 | |
| 72 | 72 | ``method [string]`` |
| 73 | - Selects between Cube analysis (3D spatial/energy likelihood) and On/Off | |
| 73 | + Selects between CUBE analysis (3D spatial/energy likelihood) and ONOFF | |
| 74 | 74 | analysis (1D likelihood with background from Off regions). |
| 75 | 75 | |
| 76 | 76 | ``emin [real]`` | ... | ... |
doc/source/users/reference_manual/csphasecrv.rst
| ... | ... | @@ -10,14 +10,16 @@ Synopsis |
| 10 | 10 | -------- |
| 11 | 11 | |
| 12 | 12 | This script computes spectra by performing a maximum likelihood fit using |
| 13 | -:doc:`ctlike` in a series of phase bins for pulsars. The phase bins can be | |
| 13 | +:doc:`ctlike` in a series of phase bins for periodic sources. The input event | |
| 14 | +list must have a ``PHASE`` column containing the phase values, that can be | |
| 15 | +assigned using :doc:`ctphase`. The phase bins can be | |
| 14 | 16 | either specified in an ASCII file or as an interval divided into equally sized |
| 15 | 17 | phase bins. The format of the ASCII file is one row per phase bin, each |
| 16 | 18 | specifying the start of stop value of the phase bin, separated by a whitespace. |
| 17 | 19 | The phase goes from 0.0 to 1.0. |
| 18 | 20 | |
| 19 | -On output the script writes the fitting results into a FITS file. The script | |
| 20 | -also produces one XML file per phase bin that contains the fitting results for | |
| 21 | +The script writes the fit results into a FITS file. The script | |
| 22 | +also produces one XML file per phase bin that contains the best-fit model for | |
| 21 | 23 | that bin. |
| 22 | 24 | |
| 23 | 25 | |
| ... | ... | @@ -39,8 +41,14 @@ General parameters |
| 39 | 41 | ``irf [string]`` |
| 40 | 42 | Instrumental response function. |
| 41 | 43 | |
| 44 | +``(inexclusion = NONE) [file]`` | |
| 45 | + Optional FITS file containing a WCS map in the first hdu that defines sky | |
| 46 | + regions not to be used for background estimation in On/Off analysis (where | |
| 47 | + map value != 0). | |
| 48 | + | |
| 42 | 49 | ``(edisp = no) [boolean]`` |
| 43 | - Applies energy dispersion to response computation. | |
| 50 | + Applies energy dispersion to response computation (for Cube analysis only, | |
| 51 | + energy dispersion is always taken into account in On/Off analysis). | |
| 44 | 52 | |
| 45 | 53 | ``outfile [file]`` |
| 46 | 54 | Name of the XML output file. The phase interval will be automatically |
| ... | ... | @@ -55,6 +63,10 @@ General parameters |
| 55 | 63 | ``phbinfile [file]`` |
| 56 | 64 | File defining the phase binning. |
| 57 | 65 | |
| 66 | +``method [string]`` | |
| 67 | + Selects between CUBE analysis (3D spatial/energy likelihood) and ONOFF | |
| 68 | + analysis (1D likelihood with background from Off regions). | |
| 69 | + | |
| 58 | 70 | ``emin [real]`` |
| 59 | 71 | Lower energy limit of events (in TeV). |
| 60 | 72 | |
| ... | ... | @@ -85,6 +97,33 @@ General parameters |
| 85 | 97 | ``binsz [real]`` |
| 86 | 98 | Pixel size (in degrees/pixel). |
| 87 | 99 | |
| 100 | +``rad [real]`` | |
| 101 | + Radius of source region circle for On/Off analysis (deg) | |
| 102 | + | |
| 103 | +``(bkgmethod = REFLECTED) [string]`` | |
| 104 | + Method for background estimation in On/Off analysis. | |
| 105 | + ``REFLECTED:`` background evaluated in regions with the same shape as | |
| 106 | + source region reflected w.r.t. pointing direction for each observation. | |
| 107 | + | |
| 108 | +``(bkgregmin = 2) [integer]`` | |
| 109 | + Minimum number of background regions that are required for an observation in | |
| 110 | + On/Off analysis. If this number of background regions is not available the observation is | |
| 111 | + skipped. | |
| 112 | + | |
| 113 | +``(maxoffset = 4.0) [real]`` | |
| 114 | + Maximum offset in degrees of source from camera center to accept the | |
| 115 | + observation for On/Off analysis. | |
| 116 | + | |
| 117 | +``(etruemin = 0.01) [real]`` | |
| 118 | + Minimum true energy to evaluate instrumental response in On/Off analysis (TeV). | |
| 119 | + | |
| 120 | +``(etruemax = 0.01) [real]`` | |
| 121 | + Maximum true energy to evaluate instrumental response in On/Off analysis (TeV). | |
| 122 | + | |
| 123 | +``(etruebins = 30) [integer]`` | |
| 124 | + Number of bins per decade for true energy bins to evaluate instrumental | |
| 125 | + response in On/Off analysis. | |
| 126 | + | |
| 88 | 127 | ``(statistic = DEFAULT) <DEFAULT|CSTAT|WSTAT|CHI2> [string]`` |
| 89 | 128 | Optimization statistic. ``DEFAULT`` uses the default statistic for all |
| 90 | 129 | observations, which is ``CSTAT`` or the statistic specified in the |
| ... | ... | @@ -129,4 +168,5 @@ Standard parameters |
| 129 | 168 | Related tools or scripts |
| 130 | 169 | ------------------------ |
| 131 | 170 | |
| 171 | +:doc:`ctphase` | |
| 132 | 172 | :doc:`ctlike` | ... | ... |