Please work through the documentation and add your comments on the bottom of this page, or email comments to email@example.com. Thank you.
The Photometry Pipeline (PP) is a Python software package for automated photometric analysis of imaging data from small to medium-sized observatories. It uses Source Extractor and SCAMP to register and photometrically calibrate images based on catalogs that are available online; photometry is measured using Source Extractor aperture photometry. PP has been designed for asteroid observations, but can be used with any kind of imaging data
- A CyVerse account. (Register for an CyVerse account here - user.cyverse.org)
- Mandatory arguments
- Input - One or more image files
The following test data are provided for testing HISAT2 in here - /iplant/home/shared/iplantcollaborative/example_data/uncompress_files_with_gunzipphotometry_pipeline: