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Copy file name to clipboardexpand all lines: README.md
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De-blended SPIRE Photometry algorithm
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DESPHOT
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DESPHOT, described in the papers above, has been used to find the flux for objects in a prior catalogue. In the first ([Roseboom et al. 2010](http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1009.1658)) and second iteration of the algorithm ([Roseboom et al. 2012](http://adsabs.harvard.edu/abs/2012MNRAS.419.2758R))(XID), 24 micron and radio sources were used as prior positions. For the final iteration (DESPHOT) [Wang et al. 2014](http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1312.0552) used the 250 micron sources detected with Starfinder as prior positions.
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***Shell scripts***
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HermesAstroSetup.csh: Old shell script to setup IDL environment
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HermesXIDSetup.csh: Lingyu's specific shel script for her version of XIDcode
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scat_xid_batch.csh
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test_scat_xid_batch.csh
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-HermesAstroSetup.csh: Old shell script to setup IDL environment
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-HermesXIDSetup.csh: Lingyu's specific shel script for her version of XIDcode
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-scat_xid_batch.csh
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-test_scat_xid_batch.csh
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***IDL code***
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lstdrv_readmaps.pro:
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lstdrv_readscat.pro: uses a two-pass strategy to do list-driven sources extraction, also finds new sources in the residual maps.
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-lstdrv_readmaps.pro:
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-lstdrv_readscat.pro: uses a two-pass strategy to do list-driven sources extraction, also finds new sources in the residual maps.
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