23.04.2015 Views

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

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

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

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

176 CHAPTER 15. CIA DATA STRUCTURE HIGH-LEVEL ARCHITECTURE<br />

CIA> cds_display, ’CCGLWDARK_96052312123000’<br />

All the parameters from the CAL-G FITS file are graphically displayed – see Figure 15.1.<br />

Clicking on the appropriate button will display plots of voltage and temperature statistics.<br />

Clicking on IMAGE M-Image will display a window containing the data image alongside its<br />

error image and allow you to scroll through all the images in the CDS. You can also load an<br />

additional CDS from disk by clicking on CDS+.<br />

15.4 Auxiliary calibration data<br />

Along with CDSs, there are additional calibration data contained in the CIA distribution. These<br />

are described in the following subsections.<br />

15.4.1 Theoretical PSFs<br />

CIA is distributed with a limited number of theoretical PSFs for use by xphot. A full set<br />

of 210 theoretical PSFs for all possible optical CONFIGURATIONS of CAM, along with the<br />

observed PSFs described in Section 15.4.2, can be found in the subdirectory psf at the official<br />

CIA ftp site. In order for CIA routines to find these PSFs they should be placed in the directory<br />

$cia vers/data/cds/. The PSFs same may be shared between all CIA versions at your site by<br />

using soft links.<br />

The theoretical PSFs are derived from the theoretical camera model – the model includes<br />

the transmission profile of a particular filter by assuming a flat spectral shape of the source.<br />

Note that no stray-light features have been considered. Though originally generated for use by<br />

xphot many observers have found them invaluable for advanced analyses such as jitter correction<br />

(Section 22.1) and source simulation.<br />

The theoretical PSFs are stored as IDL save sets and with filenames of the following format:<br />

Fixed filters e.g. psf lw5 6p0as.save<br />

psf filter pfov.save<br />

CVF filters e.g. psf 9p5mic 3p0as.save<br />

psf wavelength-in-microns pfov.save<br />

Extracting a PSF can be easily done with the aid of make psf name. Just give this routine<br />

a PDS and it return the correct filename for the appropriate PSF library:<br />

CIA> restore, make_psf_name(raster_pds), /verb<br />

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

% RESTORE: Save file written by aussel@challenger, Sat Nov 29 23:24:43 1997.<br />

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

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

.<br />

If you don’t have a PDS then you can supply the necessary parameters directly:<br />

CIA> restore, make_psf_name({aot:’raster’, wavelength:’6.75’, pfov:3.0, $<br />

CIA> fltrwhl:’lw2’}, ack=ack), /verb

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!