Science Tools Working Group
We probably won't have 'll skip having a meeting this week; the time slot will be used for a session on source identification convened by the Catalog group.
Since Mondaylast Thursday, the current version of the Science Tools v9r5p2 v9r5p1. Here are the differences from v9r5p1v9r5. The most important change is including the pgwave package, which is used in the Catalog pipeline.changes relate to IRFs; see below.
If you weren't one of the 46 people in the C&A meeting on Monday, you might want to check out Toby and Matthew's presentations yesterday on spectral analysis PointLike.
Data products: No newsData products: Examples of all of the LAT Science Data Products have been evaluated by the ingest system at the GSSC and the higher-level (post-L1 pipeline) products have been found to be wanting in various ways, mostly owing to omissions of some header keywords and lack of checksum and/or datasum calculations. These will be addressed to allow associated requirements to be signed off at the ISOC and the GSSC.
Databases and related utilities
No news
Likelihood analysis
No newsJim's implementation of calculation of TS for diffuse sources in pyLikelihood, mentioned last week, is in v9r5p1
GRB tools
No news
Pulsar tools
Masa and James have started coding expect to start coding this week to allow multiple binary timing models in the pulsar tools.
...
User interface and infrastructure (& utilities)
Jim added a kludge to the irfs package to allow the old HANDOFF response functions to still be recognized. This was needed because the Catalog group in particular is still working with the obssim2 (SC2) data set, but otherwise these response functions are only of historical interest, and in fact soon will be donated to the Smithsonian Air and Space Museum.
Johann made minor changes to several packages to make them able to compile on 64-bit computers; the need for these changes was discovered by Eric W. in porting the Science Tools to the hmake system at the GSSC.
Source Catalog
See Jim's note to irflist regarding the updates to IRF-related packages in v9r5p1. Riccardo's presentation in the C&A meeting yesterday provides a synopsis.
Here are the IRF sets that gtirfs reports are available in v9r5p1:
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 simulationsMet last week for a discussion about source identification/counterpart assignment. The meeting was nearly foiled by EVO problems; the cross-group strategies are available for comment - now's the time.