The following command:

 nex;dcut CAVE x 0.0 2.0 2.0 0.05 0.05

as used to produce TPC Y-Z cross section.

Looks to me THE TPC electronic card are missing in UPGR13.

CuCu Spectra Pi- Spectra

Attached are extensive mapping files for the BSMD and BPRS. These maps were generated for 2008-03-04 10:30:54, which is the beginning of run 9064017.

 This is zoom in on the eta=1 gap between BTOW & ETOW.

I : Selection of good wafers

Goal : 

The attached lists have the towers with status == 1 and gain == 0 and gain_status == 0. There are 130 from 2006 and 143 from 2005.

The two attached .pdf files show the results of a preliminary set of endcap cuts including the SMD.

Intro

I’ve been struggling to keep our MIT database mirror synchronized with the BNL master, and I wanted to write about some steps we (STAR) might take to do a better job of keeping our slaves synchronized. The problem that I’m worried about is the situation where, according the the Heartbeat Page, a slave is up-to-date with robinson, but in reality the slave somehow become silently corrupted.

Initial Checksums

It turns out that this problem is actually pretty common. I found what seems to be a slick set of utilities called Maatkit that will calculate checksums of every table in a DB and look for differences between replicated DBs. I ran mk-table-checksum on the following servers

• robinson.star.bnl.gov:3306
• db01.star.bnl.gov:3316
• db02.star.bnl.gov:3316
• db03.star.bnl.gov:3316
• rhig.physics.yale.edu:3316
• star1.lns.mit.edu:3316

and attached the output below as initial_checksum.txt. None of the slaves in that list are fully in sync with robinson according to those checksums. db02 and db03 come much closer than the others; in db02’s case only Calibrations_tracker.{schema,ssdHitError} are different from robinson. I verified for a few cases that differences actually do exist in the tables when the checksums don’t match.

Resynchronization and Results

Maatkit also provides a utility (mk-table-sync) which will determine and optionally execute the SQL commands needed to re-sync one server against another. I used this utility to re-sync star1 against robinson — it takes quite a while. I then ran mk-table-checksum and mk-checksum-filter again, and attached the output as checksum_after_sync_filtered.txt. Unfortunately, robinson and star1 still don’t have perfect agreement according to the checksums. I’m not sure what tables like Nodes, NodeRelation, and tableCatalog do, but I noticed the following “physics” tables still did not have matching checksums:

• Calibrations_ftpc.ftpcGasOut
• Calibrations_rich.trigDetSums
• Calibrations_svt.svtPedestals
• RunLog_onl.beamInfo
• RunLog_onl.biFitParams
• RunLog_onl.starMagOnl
• RunLog_onl.zdcFitParams

Now comes a weird part: I tried a SELECT * FROM biFitParams on star1 and on robinson, and in that case there was no difference in the output. I’m not sure how the checksums could still be different in that case. I also tried diff’ing the starMagOnl tables; the only difference I found was one server reported some currents as “-0.0000000000” and the other one reported “0.0000000000” (no leading minus sign).

Summary

So, I realize the results aren’t 100% conclusive, but I still believe that these maatkit scripts would be a valuable addition to STAR’s QA toolkit. They definitely helped me correct a variety of real problems with our MIT database mirror.

It’s straightforward to take the output of mk-table-checksum and mk-checksum-filter and programmatically put it on a webpage; in fact, Mike Betancourt wrote up a little sed script to do just that. I think we should try scheduling ~daily checksum calculations and posting any discrepancies to the Heartbeat webpage automatically.

M-C pileup simulation 

1. Prepare 2 .fzd files, use the same geometry
   1. phys.fzd ( hard process simulation you want to study).

Mission statement:  PPV finds only Z-vertex (as of June 2008)

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