LSSTApplications
16.0-1-gce273f5+18,16.0-10-gc1446dd+17,16.0-12-g569485f+1,16.0-12-g6065a46,16.0-13-g5e87145+1,16.0-13-g80874fd,16.0-13-gb122224+8,16.0-13-gd9b1b71+17,16.0-14-g08f9460,16.0-15-g77ef378+3,16.0-16-gf910c00+1,16.0-17-g0bdc215+10,16.0-17-g6a7bfb3b+17,16.0-2-g0febb12+14,16.0-2-g839ba83+55,16.0-2-g9d5294e+43,16.0-2-gc6e0ed0+1,16.0-21-g8fa7d5a4,16.0-3-g404ea43+10,16.0-3-gbc759ec+15,16.0-3-gcfd6c53+41,16.0-4-g03cf288+32,16.0-4-g13a27c5+18,16.0-4-g5f3a788+13,16.0-4-g8a0f11a+39,16.0-4-ga3eb747+3,16.0-5-g1991253+17,16.0-5-g1e9226d+1,16.0-5-g865efd9+18,16.0-5-gb3f8a4b+49,16.0-5-gd0f1235+7,16.0-51-gb4b4a8566,16.0-6-gf9cb114+19,16.0-7-g6043bfc+5,16.0-7-ga8e1655+13,16.0-7-gde5bd64,16.0-8-g4dec96c+30,16.0-8-gfd407c0+3,16.0-9-g2f60796,master-g5768c874b9+2,w.2018.41
LSSTDataManagementBasePackage
|
The goal of the multi-band coadd measurement procedure is to consistently detect and measure sources across coadds constructed in multiple filter bands in a consistent and reasonable manner i.e.
measure the same sources, with consistent centroids and shapes, across all the photometric bands. This is useful, for example:
Consider how this workflow contrasts with a simpler approach in which detection and measurement is carried out in each band independently.
Our strategy for is broken up into a number of simple steps:
["HSC-I", "HSC-R", "HSC-Z", "HSC-Y", "HSC-G",]
in the case of HSC). Every source must have a centroid, shape, and CModel fit in every band, even if the object was not detected in the canonical band. We now provide a complete run through multiband processing using the ci_hsc package. We will process the HSC-I & -R band coadds generated from HSC engineering test data provided in the ci_hsc package. To begin, assuming that the lsst stack has been already set up, we must set up the obs_subaru and ci_hsc packages. This defines the environment variable $CI_HSC_DIR
which points at the location of the package on disc. The raw HSC exposures live in the $CI_HSC_DIR/raw
directory. Note that all the scons build commands are cumulative i.e. to build the coadd in step 4, scons checks to see if the targets of step 3 exist. If not, it first builds step 3 etc. Stepwise, we can process the data in ci_hsc as follows:
$CI_HSC_RAW
to produce calibrated exposures. Having done this, we can run forced photometry on the coadds and individual visits using the master catalog generated by step 8.