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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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234 CHAPTER 20. ADVANCED DATA CALIBRATION<br />

3. method=‘tcor’<br />

method: Deglitch tcor. This method attempts to attempts to avoid the problems that<br />

arise from instability by initially transforming the cube into a zero-mean cube and<br />

then deglitching. The algorithm is:<br />

(a) Compute the zero-mean, D, of the input .CUBE, cube in:<br />

D = √ 2<br />

6<br />

cube in(∗, ∗,i) − √ 1<br />

6<br />

cube in(∗, ∗,i− 1) + cube in(∗, ∗,i+1))<br />

(b) Compute S t, theNsigma clipping of D<br />

(c) For each IMAGE of cube in:<br />

i. Compute I, whereI = IMAGE − median(IMAGE,5)<br />

ii. Compute S p, theNsigma clipping of I<br />

iii. A glitch has occurred if abs(D(∗, ∗,f)) >S t and abs(I) >S p<br />

iv. Replace glitched pixels cube out(i, j, k) bycube out(i, j, k − 1)<br />

Some criticisms of the tcor have been made – under certain conditions it will eradicate<br />

your data. As with all deglitching techniques it should be used with care.<br />

routine called: deglitch tcor<br />

PDS side effects: Glitches removed from IMAGEs in .CUBE, i.e. .CUBE is modified.<br />

Glitched pixels also flagged in .MASK.<br />

reference: online help.<br />

4. method=‘mm’<br />

method: Deglitch MM (Multiresolution Median Transform). The Multiresolution Median<br />

Transform works on the principle that in temporal space glitches are small scale<br />

structures and source signal will always be large scale structure. Consequently, this<br />

method may fail for glitches of very long duration. In general though, it is very<br />

robust and handles non-stabilized data well. It is especially good for observations<br />

where many IMAGEs are accrued. This method is the default.<br />

routine called: mr1d deglitch<br />

PDS side effects: Glitches removed from IMAGEs in .CUBE, i.e. .CUBE is modified.<br />

Glitched pixels also flagged in .MASK.<br />

reference: <strong><strong>ISO</strong>CAM</strong> Handbook, Chapter Data processing methods, Section Deglitching<br />

using the Multiresolution Median Transform (MMT).<br />

5. method=‘sky’<br />

method: sky cube deglitching. Faders and dippers can be rejected from rasters with<br />

redundant observation. Flags .MASK of a PDS. The input data (cube and image)<br />

should be flat-fielded. The algorithm is:<br />

(a) The mosaic is created and back-projected into the image again.<br />

(b) The image is rebinned into a cube<br />

(c) Standard deglitching is performed on the difference between the original and the<br />

back-projected cube.<br />

routine called: deglitch sky<br />

PDS side effects: Glitched pixels are flagged in .MASK. A new .RASTER is created.

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