| | 1 | I tried for about a week to figure out the right format file for the CTIO 4m Blanco MOSAIC2 that would support both full-FPA processing and individual amp- or chip-based processing. In the end I just gave up and treated each reduced amplifier as an FPA in the configuration files. This was easy and simple, but a guide with examples on how the configurations are supposed to be set up for various different detectors would be quite helpful to be able to self-consistently use the IPP for a full processing of images. But for now the first goal is just to see if we can get subtractions from already-processed ESSENCE images and do object detection, lightcurves, and classification. |
| | 2 | |
| | 3 | On our IIC cluster here at Harvard, I ran |
| | 4 | |
| | 5 | ppSub /gpfs1/Panstarrs/smsn/data/v9.0/W/workspace/sm061227/2/wdd8.061227_0404.033_2.sw.fits \ |
| | 6 | /gpfs1/Panstarrs/smsn/data/v9.0/W/workspace/wtempl_05/2/wdd8.041114_0358.078_2.sw.fits \ |
| | 7 | -inweight /gpfs1/Panstarrs/smsn/data/v9.0/W/workspace/sm061227/2/wdd8.061227_0404.033_2.sw.noise.fits.gz \ |
| | 8 | -refweight /gpfs1/Panstarrs/smsn/data/v9.0/W/workspace/wtempl_05/2/wdd8.041114_0358.078_2.sw.noise.fits.gz \ |
| | 9 | Wsub |
| | 10 | |
| | 11 | ESSENCE and the IPP use a slightly different convention for masking so I didn't use the ESSENCE masks. However, the weight images do have very high variances set for the masked-out regions so it's OK for now not to have the mask. I ran with a very simple, and theoretically inadequate, convolution kernel size. Here's the "ppSub.config" I used. This was with Paul Price's ipp-2.2b ppSub modifications. |
| | 12 | |
| | 13 | ### Recipe file for ppSub |
| | 14 | |
| | 15 | KERNEL.TYPE STR ISIS # Kernel type to use (POIS|ISIS|SPAM|FRIES) |
| | 16 | KERNEL.SIZE S32 5 # Kernel half-size (pixels) |
| | 17 | SPATIAL.ORDER S32 0 # Spatial polynomial order |
| | 18 | STAMP.SPACING F32 200 # Typical spacing between stamps (pixels) |
| | 19 | STAMP.FOOTPRINT S32 5 # Size of stamps (pixels) |
| | 20 | STAMP.THRESHOLD F32 0 # Flux threshold for stamps (ADU) |
| | 21 | ITER S32 10 # Number of rejection iterations |
| | 22 | REJ F32 1.5 # Rejection level (std dev) |
| | 23 | MASK.BAD STR BLANK,BAD,SAT # Mask value for bad pixels |
| | 24 | MASK.BLANK STR BLANK # Mask value to give blank pixels |
| | 25 | @ISIS.WIDTHS F32 3 6 # Gaussian widths for ISIS kernels |
| | 26 | @ISIS.ORDERS S32 2 2 # Polynomial orders for ISIS kernels |
| | 27 | SPAM.BINNING S32 2 # Binning in outer region for SPAM kernels |
| | 28 | INNER S32 5 # Inner half-size for SPAM and FRIES kernels |
| | 29 | RINGS.ORDER S32 1 # Polynomial order for RING kernels |
| | 30 | |
| | 31 | REGION.SIZE F32 NAN # Size of region over which to solve for one variable convolution; 0 or NAN means one regio |
