David W. Hogg
New York University
2005 May 9
To read this table, do the following: Find the column corresponding to the "target" chip (the chip you want to read). Look for significant amplitudes. For each "cross-talk" chip that has a significant amplitude in the column, subtract the amplitude times the cross-talk-chip image from the target-chip image. (In principle, you need to do some column and row flipping, but in practice you don't because the non-zero amplitudes are for chip pairs with identical orientations.)
chip | 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 |
---|---|---|---|---|---|---|---|---|
1 | -0.00000 | -0.00003 | +0.00001 | -0.00001 | -0.00001 | -0.00000 | -0.00000 | |
2 | +0.00137 | +0.00000 | -0.00001 | -0.00003 | +0.00001 | -0.00001 | -0.00002 | |
3 | +0.00001 | -0.00001 | +0.00002 | -0.00002 | +0.00000 | +0.00001 | -0.00001 | |
4 | -0.00000 | -0.00001 | +0.00290 | -0.00005 | -0.00001 | -0.00001 | -0.00003 | |
5 | -0.00002 | -0.00002 | +0.00001 | +0.00000 | +0.00166 | -0.00002 | -0.00000 | |
6 | -0.00001 | +0.00000 | -0.00000 | -0.00001 | +0.00003 | +0.00000 | -0.00002 | |
7 | +0.00001 | -0.00002 | -0.00003 | -0.00002 | -0.00002 | -0.00003 | +0.00083 | |
8 | +0.00000 | +0.00001 | +0.00001 | +0.00001 | +0.00000 | +0.00000 | +0.00000 |
These coefficients were found with mosaic_crosstalk and mosaic_crosstalk_analyze in the astrometry.net codebase.
Briefly, the method is as follows:
The IDL code that performs these functions is
This code depends on the skymaps.info codebase idlutils.