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

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

20.9. DEALING WITH DEAD PIXELS 251<br />

20.8.1 PDS history<br />

In general, operations performed on a PDS are recorded in .HISTORY. It lists routines and<br />

calibration methods applied to the PDS:<br />

CIA> print, staring_pds.history<br />

date=26-May-1998 17:21:49 node=bikini user=mdelaney<br />

procedure=darklibrary V 1.0 algorithm=Find best CCGLWDARK_97031713382678 END<br />

date=26-May-1998 17:19:22 node=bikini user=mdelaney<br />

procedure=spdtoscd V 2.0 algorithm=default<br />

(7) cisp03001209.fits (7) $cia_vers/test <br />

(2) 19 (2) 119 END<br />

date=26-May-1998 17:21:54 node=bikini user=mdelaney<br />

procedure=flat_library V 1.1 algorithm=Find best CCGLWOFLT_98041510080669 END<br />

date=26-May-1998 17:21:55 node=bikini user=mdelaney<br />

procedure=flat_library V 1.1 algorithm=Find best CCGLWDFLT_98031519384439 END<br />

date=26-May-1998 17:21:40 node=bikini user=mdelaney<br />

procedure=get_sscdstruct V 2.1 algorithm=default<br />

CSSC030012090001_98052617205667 END<br />

date=13-Jul-1998 10:53:06 node=bikini user=mdelaney<br />

procedure=corr_dark V 3.9 algorithm=cube = (cube/gain/tint)-dark model END<br />

etc...<br />

If you use CIA routines to convert your PDS to a FITS file, the text in .HISTORY is saved<br />

in the FITS header (see Chapter 18).<br />

20.9 Dealing with dead pixels<br />

Usually, the only dead pixels you need worry about are the four of the SW detector and column<br />

24 of the LW detector. However, if you have very heavily glitched or unstable data, then<br />

after calibration a pixel may be masked all the way through a set of IMAGEs from a STATE.<br />

When reduced to an EXPOSURE, such pixels will be effectively dead in that EXPOSURE.<br />

Their corresponding value in .NPIX will be zero, in other words they will have a zero weight.<br />

raster scan ignores all dead pixels – if EXPOSUREs do not overlap where a dead pixel occurs,<br />

then a blank spot will appear in the MOSAIC.<br />

Note the following when you are dealing with data from the LW detector: after calibration,<br />

but before building the raster MOSAIC, calib struct automatically smooths column 24 in the<br />

.IMAGE and .CUBE. However, the weight of every pixel, i.e. the values in .NPIX, in column 24<br />

will always remain as zero. Therefore column 24 will appear as a dead column in the MOSAIC.<br />

However, it will no longer be column 24, but column (.NX RASTER-8).<br />

Dead pixels appearing in the raster MOSAIC are optionally smoothed by calib raster:<br />

1. /dead<br />

method: Where dead pixels appear in the raster MOSAIC, i.e. where .NPIXRASTER<br />

is zero, a median smoothing method is applied. Only the dead pixels are smoothed<br />

into their neighbors – no other pixels are affected.<br />

called routine: im smooth<br />

PDS side effects: Dead pixels in .RASTER are smoothed.

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

Saved successfully!

Ooh no, something went wrong!