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ISOCAM Interactive Analysis User's Manual Version 5.0 - ISO - ESA

ISOCAM Interactive Analysis User's Manual Version 5.0 - ISO - ESA

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116 CHAPTER 14. IMAGE ANALYSIS AND DISPLAY<br />

CIA> xphot, raster_pds.raster, psf_dir=’/home/cia/isocia/ia/PSF/’<br />

2. Take a look at Figure 14.1. It contains the image we supplied when invoking xphot, i.e.<br />

a raster MOSAIC, and a number of buttons. The button Select Objects is highlighted, so<br />

the first action you must take is to select the sources that you wish to do photometry on.<br />

Click on Select Objects to begin the selection process. A pop-up window will appear with<br />

some information – read and dismiss. Now you can choose your sources by clicking on<br />

the image. In the example image displayed in Figure 14.1 there is clearly only one source.<br />

Click on done when you are finished making the selection.<br />

3. Now click on Photometric Method to choose the photometric method to apply to the<br />

source. In our example here we will select the first option: simple aperture photometry.<br />

4. The next step is to determine the radius over which to perform the photometry. Click<br />

on Select Radius and choose the simplest method, 1 for all. A new window will appear,<br />

displaying a region of the image centered on the source. Click on this window to indicate<br />

the desired radius. Click done when finished.<br />

5. The final step is to determine the background. Clicking on Select Background will give<br />

you a choice of methods, the simplest being 1 for all. Again, we will choose this option<br />

for our example here. Now select a region of the displayed image for determination of the<br />

background: click on the lower-left point of the region first, followed by the upper-right<br />

point.<br />

6. You can now click on the button compute to perform the photometric calculation according<br />

to the parameters that you have chosen above. The results will be printed to screen in the<br />

following order: the source/object number, its pixel coordinates, the aperture radius, the<br />

background value and the source flux. When you quit xphot (click on quit) these data<br />

will be saved to disk. To recover. . .<br />

CIA> restore,’xphot_tables_final.save’,/verb<br />

% RESTORE: Portable (XDR) SAVE/RESTORE file.<br />

% RESTORE: Save file written by mdelaney@bikini, Thu Oct 9 17:07:40 1997.<br />

% RESTORE: IDL version <strong>5.0</strong> (sunos, sparc).<br />

% RESTORE: Restored variable: ID.<br />

% RESTORE: Restored variable: X.<br />

% RESTORE: Restored variable: Y.<br />

% RESTORE: Restored variable: RAD.<br />

% RESTORE: Restored variable: BKG.<br />

% RESTORE: Restored variable: FLUX.<br />

CIA> print, flux<br />

106.678<br />

14.1.5 Other methods for photometry measurements<br />

This sections describes some other basic tools to perform photometry measurements:<br />

photom psf High level routine to perform PSF photometry. As an example, we restore the<br />

test-dataset, a raster observation of M51 and perform PSF photometry on the companion.<br />

Calling syntax:

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