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APERTURE-Do simple minded aperture photometry on a series of frames

Description:
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.

Parameters:
OUTPUT
The name of the file where the answers will be written.
IMAGE
The name of the file with the frame to be analysed.
OPT
The option parameter. Type H for help.
LOW
The low data value for 2-D plots.
HIGH
The high data value for 2-D plots.
RADIUS
The radius of the circle to be used for the integration.
OK
Say "yes" when you are happy with the apearture.

Source comments:
 A P E R T U R E

 Description
 -----------
 Do simple minded aperture photometry on a series of frames

 Scope of program
 ----------------
 - 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
 ----------
 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
 --------
 OK

 Method
 ------
 - 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
 --------
 Jim Lewis RGO (jrl@ast.cam.ac.uk)


next up previous 79
Next: ARC-Interactive manual arc line identification
Up: Applications in detail
Previous: ALASOUT-Output a spectrum in ALAS (Abs. Line Analysis System) format

FIGARO A general data reduction system
Starlink User Note 86
Keith Shortridge, Horst Meyerdierks,
Malcolm Currie, Martin Clayton, Jon Lockley,
Anne Charles, Clive Davenhall,
Mark Taylor, Tim Ash, Tim Wilkins, Dave Axon,
John Palmer, Anthony Holloway and
Vito Graffagnino
2004 February 17
E-mail:ussc@star.rl.ac.uk

Copyright © 2009 Science and Technology Facilities Council