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Previous: Fitting an Optical Image
Here we will fit the Gaussian model to a GIS2 simulation of an elliptical
Gaussian source (e.g., this is a sanity check since we should get back
the same parameters that went into the simulation, namely 1' by 2'). This
example also includes a mask to only include the central 18' of the GIS
FOV.
ximgfit> data tutorial/g2_g1x2min_100ks.img.gz
ximgfit> psf tutorial/g2_psf_sim_1Ms.img.gz
ximgfit> mask tutorial/gis_mask_18min.img.gz 1
ximgfit> model Gaussian
ximgfit> new 3 100
ximgfit> new 4 50
ximgfit> new 5 130
ximgfit> stat C
ximgfit> show
Data file: test/test_g2_g1x2min_100ks.img.gz, size = 256 X 256
PSF: test/test_g2_1Ms.img.gz, size = 256 X 256
Mask file: gis_mask_18min.img.gz, size = 256 X 256
Padding = none
Rebinning = none
Plate scale = 14.753989 arcsec/pixel
Model: Gaussian
Par Mod Name Value ( units) Description
1 1 xc 0 ( arcsec) X offset from image center
2 1 yc 0 ( arcsec) Y offset from image center
3 1 norm 100 ( comp) Normalization
4 1 sigmax 50 ( arcsec) Sigma in the X direction
5 1 sigmay 130 ( arcsec) Sigma in the Y direction
6 1 theta 0 ( degrees) Rotation angle
C = -69510.24, with 16286 degrees of freedom (16292 data bins)
ximgfit> fit
-70937.52 -4 0.3171 1.977 121.3 54.86 116.4 0.01173
-71043.90 -5 0.3677 2.327 128.7 55.84 114.7 0.02735
-71044.48 -6 0.3633 2.397 129.3 55.92 114.5 0.04423
-71044.55 -7 0.3621 2.402 129.3 55.92 114.5 0.06094
-71044.61 -8 0.362 2.402 129.3 55.92 114.5 0.07736
-71044.67 -9 0.362 2.402 129.3 55.92 114.5 0.09349
-71044.74 -10 0.362 2.402 129.3 55.92 114.5 0.1093
-71044.79 -11 0.362 2.401 129.3 55.92 114.5 0.1249
-71044.85 -12 0.3621 2.401 129.3 55.91 114.5 0.1402
-71044.90 -13 0.3621 2.401 129.3 55.91 114.5 0.1553
Last change in fit statistic = 0.0546
Although C is coming out negative (probably due to the fact that the
term is dropped in the fitting procedure, see Cash 1979), note that a proper
minimum is reached. The results of ``view data'', ``view model'', ``view
psf'', and ``view psf'' are shown in Figure 2 (after running
fit 100 to reach a slightly better minimum in the C statistic). These images
are shown with view set to display logarithmically (set view log). The
effect of the 18' mask is evident in the model image.
Figure:
Result of ``view data'' (top left), ``view psf'' (top right),
``view model'' (bottom left),
and ``view resid'' (bottom right) within XIMGFIT. All images are displayed logarithmically.
 |
To get the error on a parameter, use either the ``error'' command or the
``step'' command (to manual search for an error range when the expect range
of the parameter is already known):
ximgfit> step 5 115 120 5
Fit Statisitc Delta Fit Stat. Mod Param
-71046.26 0.16 115.00
-71044.61 1.81 116.00
-71041.19 5.22 117.00
-71036.03 10.39 118.00
-71029.13 17.29 119.00
-71020.52 25.90 120.00
This example implies that there is some systematic error in the difference
between the best-fit
and the inputted
of 120'',
probably due to the slight change in the GIS PSF with off-axis angle.
Next: Fit to a ROSAT
Up: Quick-start Tutorial
Previous: Fitting an Optical Image
Andrew Ptak
2001-10-11