A P E R T U R E
Description
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Do simple minded aperture photometry on a series of frames
Scope of program
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- Handles 2-D images only.
- Data array converted to FLOAT.
- Magic values supported.
- Error arrays not supported
- Quality arrays not supported.
- Batch execution not supported.
Parameters
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OUTPUT Name of output ASCII file for results. The output info goes in
the following order: (1) Either 'O' or 'S' for "object" or
"sky"; (2) a sequence number; (3) the x,y coords of the
cursor, (4) the radius of the aperture; (5) the total
flux in pixels which are with a radial distance less than
or equal to the aperture radius. No correction is made for
partial pixels; (6) the total number of pixels included.
(character)(prompted for)
IMAGE Name of individual images in case you're not using a
list file. (character)(prompted for)
RADIUS Radius for integration. (real)(prompted for)
LOW Data value for lowest level in 2-d plot (real)(prompted for)
HIGH Data value for highest level in 2-d plot (real)(prompted for)
Keywords
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OK
Method
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- The image name is read and that image is plotted on the current
plot device.
- The user is presented with a menu which allows him/her/it to specify
object and sky regions, change the colour levels, change the radius
of the aperture, show cuts or quit.
- Integrations are a simple sum of the values of the pixels within the
aperture radius.
Author/s
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Jim Lewis RGO (jrl@ast.cam.ac.uk)
FIGARO A general data reduction system