Overview of the Frames Pipeline
Table of Contents
The order in which the modules are executed in the Frames
Pipeline is:
Start
Initialise Modules, Read Plan/Parameter Files
Foreach frame {
Read Known Objects
Foreach color {
Read Frame, and add on overlap with next frame
Correct Frame
Fix Cosmic Rays
}
Foreach color {
Find Bright Objects
}
Merge Bright_Objects
Foreach Bright_Object {
Measure Object
}
Subtract Star Wings
Foreach binning-scale {
Bin Frame
Foreach color {
Estimate and Subtract Local Sky
Find Faint Objects
}
Merge Faint Objects, adding them to object list
}
Write Corrected Frame, Mask, and Binned Image
foreach object {
Measure Object
Write parameters and atlas image
Deblend
Foreach child {
Measure Object
Write parameters and atlas image
}
}
Write remaining outputs
}
Cleanup
End
In the list below, we give representative values for several
parameters (for example, overlap region size) that are not
fixed and may change in practice; they are indicated by an italic font.
Before it can run, the Frames Pipeline requires various inputs; for
details see Correct Frame's discussion of
inputs. For each frame,
it needs:
- CCD hardware specs for each chip, including its readout noise,
gain, list of any defects, etc.
- raw frames for each color, which are a different size than corrected
frames: they lack overlap regions between frames, and hence have
a smaller number of rows (1354 vs. 1489; 10%); and they have
extra columns from the overclock region on both ends
(2128 vs. 2048).
- a bias vector appropriate for each chip.
- a flatfield vector for each chip.
- a CALIB1 structure for each frame, which includes the filter name,
sky value and slope, bias values for each amplifier, approximate flux
calibration (in the form of ``the number of DN which equal magnitude
20.0''), a model for the point-spread-function, and
the coordinate transformation to convert pixel coordinates in this
frame to great-circle coordinates (frames uses these to find the
transformation from one band to another, so which great circle
coordinates is not important).
The first item on this list must be kept up-to-date by the
Survey's Imaging Scientist (or other person who carefully
monitors the CCD camera). The second item is supplied directly
from the Data Acquisition system. All the remaining items
are
produced by the Postage-Stamp Pipeline.