SSC Home Page

IRAC: Software: Make BCD-matched photometric correction images


SPITZER HOME - SPITZER SCIENCE - INSTRUMENTS - SCIENCE USER SUPPORT - SEARCH
copy_photcorr_posns.pro was written by Mark Lacy (SSC) and is provided "as is" for testing and usage by other observers.

Aperture photometry on IRAC mosaics requires corrections to be applied based on the positions of the sources in the component BCDs. This software uses the available IRAC correction and pixel area maps to make a set of correction images which can then be mosaicked together in MOPEX. Users can then use this mosaic to look up photometric correction factors for an object at any given position in their BCD mosaic.

  • NAME: copy_photcorr_posns
  • PURPOSE: Make a set of BCD correction photometric correction images with the correct header information in for mosaicking with MOPEX
  • CALLING SEQUENCE: copy_photcorr_posns,bcdlist,photcorrimg,areaimg,OUTLIST = outlist
  • INPUTS:
  • OUTPUT: A set of photometric correction images equal in number to the BCDs, with matching header information, and, if specified, a list for input to MOPEX.
  • OPTIONAL INPUT KEYWORD:
    • OUTLIST - if specified, name of an output list of correction images for input to MOPEX
  • REQUIREMENTS: IDL v6.3 and higher

This software is not considered part of the pipeline and no installation support from the SSC should be expected. We are however very interested in your feedback in order to improve or replace the algorithm and are glad to work with you in test cases and analysis. Please send your comments to help@spitzer.caltech.edu.

Download copy_photcorr_posns.pro.


SPITZER HOME - SPITZER SCIENCE - INSTRUMENTS - SCIENCE USER SUPPORT - SEARCH

Contact Us
This file was last modified on Fri Jan 9 10:27:36 2009.
California Institute of Technology Jet Propulsion Laboratory NASA