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Comment: Migration of unmigrated content due to installation of a new plugin

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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.