Up: IPP at the ROE
IPP Data Reduction Stages
This page is a work in project. Please add if you know more or better.
In order of processing:
- Raw (14 or 15 bits per pixel? In either case, 2 bytes required.)
- Straight from the telescope
- Chip
- Images:
- detrended (5 bytes per pixel: 2 signal, 2 weight, 1 mask. Compresses to 44%)
- flattened
- debiased
- detrended (5 bytes per pixel: 2 signal, 2 weight, 1 mask. Compresses to 44%)
- Products:
- PSF measurement
- point source catalogues
- Tools used
- Images:
- Camera
- Images
- Nothing new
- Products
- astrometry for entire focal plane
- some position-dependent masks
- Tools used
- Images
- ( Fake )
- Images
- detrended
- Tools used
- Images
- Warp
- Images
- Warped to predefined skycells (i.e. images in sky coordinates)
- Products
- Remeasured PSF
- Tools used
- Images
- Stack
- Images
- Combination of warps (images in sky coordinates) convolved to a common PSF
- Products
- Nothing new
- Tools used
- Images
- Diff
- Images
- Difference between two frames or a frame and a stack, all in sky coordinates (a.k.a warps)
- Tools used
- Images
- Magic
- Stripes added to hide high-proper motion objects (satellites and other things which shouldn't be masked)
- Tools used
- Addstar Stage
- ?
- Tools used
Last modified
16 years ago
Last modified on Nov 12, 2009, 10:52:33 AM
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