A high-level routine for starting the reduction of a nights-worth of acm images. Three primary steps are performed. (1) CCD processing (FBP, bias subtraction, dark subtraction). (2) image catalogs are assembled for each image found to be in a set of one or more images taken on a unique sky position (UPS = unique sky position). ( 3) Calibration material (DSS,USNO,PS1) data are gathered for or each UPS.

 


% AcmRunDate --help   

Usage: AcmRunDate 20191018  
arg1 - date of desired night to reduce (YYYYMMDD)  
Additional options: 
     -v = print verbose comments 
 --help = view a help document