...
P5_v13_0_diff ( = P5_v13_0_diff::FRONT + P5_v13_0_diff::BACK ) |
P5_v13_0_diff::BACK |
P5_v13_0_diff::FRONT |
P5_v13_0_source ( = P5_v13_0_source::FRONT + P5_v13_0_source::BACK ) |
P5_v13_0_source::BACK |
P5_v13_0_source::FRONT |
P5_v13_0_trans ( = P5_v13_0_trans::FRONT + P5_v13_0_trans::BACK ) |
P5_v13_0_trans::BACK |
P5_v13_0_trans::FRONT |
PASS4 ( = PASS4::FRONT + PASS4::BACK ) |
PASS4::BACK |
PASS4::FRONT |
PASS4_v2 ( = PASS4_v2::FRONT + PASS4_v2::BACK ) |
PASS4_v2::BACK |
PASS4_v2::FRONT |
PASS5_v0 ( = PASS5_v0::FRONT + PASS5_v0::BACK ) |
PASS5_v0::BACK |
PASS5_v0::FRONT |
PASS5_v0_DIFFUSE ( = PASS5_v0_DIFFUSE::FRONT + PASS5_v0_DIFFUSE::BACK ) |
PASS5_v0_DIFFUSE::BACK |
PASS5_v0_DIFFUSE::FRONT |
PASS5_v0_TRANSIENT ( = PASS5_v0_TRANSIENT::FRONT + PASS5_v0_TRANSIENT::BACK ) |
PASS5_v0_TRANSIENT::BACK |
PASS5_v0_TRANSIENT::FRONT |
Older IRFs (DC2, DC1, et al.) are still available and can be viewed by doing
| Code Block |
|---|
gtirfs chatter=3
|
From Eric W.: "The ScienceTools tarball distributed by the GSSC is in beta test now. We have also prepared a second tarball with the GSSC version of the ModelEditor. The latter has not been touched for many months, so I expect it will get some tweaking over the next few weeks. The GSSC-distributed tarball is now supported on 32- and 64-bit Linux, and OS X 10.4 on Intel- and PowerPC-based Macs."
Source Catalog
Met last week. The multi-band method that Jean and Ludovic have implemented for MRfilter have made it (currently) the best-performing source detection algorithm. The same approach will likely improve the performance of PGWave as well. UW pointfind (which inspired the mult-band approach) is not far behind and has a performance advantage in the vicinity of bright sources. Toby described the new command-line interface for pointfit. We also discussed the current state of using the Big Run backgrounds to make resampled (Pass 5) backgrounds for gtobssim simulations.