Mass, Mu and Mv -- IU Algo
In regard to Dave Underwoods post on Jan. 12th, 2012, I plot the Mu vs Mv and several related mass plots.
IST numbering
Updated on Thu, 2012-03-01 14:16. Originally created by margetis on 2012-03-01 13:44.Reference
Talk time : 13:30, Duration : 00:20
HFT Software
Updated on Thu, 2012-03-01 12:44. Originally created by margetis on 2012-03-01 12:44.510-4867333, at 18:30 (GMT), duration : 00:00
HFT Software
Updated on Tue, 2012-03-20 12:25. Originally created by margetis on 2012-03-01 12:44.510-4867333, at 18:30 (GMT), duration : 00:00
510-4867333
Items for this Friday's meeting are:
1) Hao Qiu has prepared an informal presentation on his
analysis of the single-thinned chip survey with the new
CMM machine, optical probe. I asked him to present it to
the group. We also had the chance at LBL to discuss a bit
about the geometry structures in detail were I promised to
provide some details on previous SVT work and details/examples
on structures we use.
2) Jonathan made some progress (timing) and managed to fix some bugs
in reconstruction with new geometry.
Other Items:
a) Flemming provided some prelim drawings of the beam pipe. They are good
to be used for modeling.
b) I talked to H.W. about big chunks of mass still missing from modeling. Some of
his feedback is posted on the action-items of Geometry-review page:
http://drupal.star.bnl.gov/STAR/event/2012/03/09/hft-software/round-table-discussion-action-items-defined-20
c) I talked to H.M. (with J.T and M.L) about a plan for SSD ladder survey at LBL.
Ladder(s) are stuck in customs on their way to LBL, not for long I hope.
We all have an understanding about what need to be done.
d) I had a discussion with Xin on the Offline structures/needs. There is
a multitude of structures we need to touch or build from scratch and
associated issues like:
1) StEvent Hit containers -> move away from RnD to PXL, IST etc
with proper structure, e.g. instead of layer, ladder, pixel have sector,
ladder, pixel for PXL etc. The same for StMcEvent containers
2) Hit info on Tracks. make sure it is done properly, e.g. possible # hits
3) Is current MuDst info sufficient? We have made proposal to modify
and update the info (+Evaluation, minimc info). Need to finalize/implement.
We both agreed/emphasized the use of Dcageometry info in HF reconstruction
as well as Kalman fitters (minimum work is needed to fully deploy this).
4) Slow/Fast simulators: Move final scheme/products in place of current
short-cut one.
This is the road map more or less, also by looking at the overall execution flow
of software.
e) There are two reviews coming up we need to keep in mind:
i) One review for software/procedure that connects metrology to geometry
structures in the Db. This is going to happen in about a month from now.
By then we need to have the test-sector CMM data taken (this is a
pre-requisite for the review).
ii) Track Alignment structures/procedures in place (prototype run etc). This
will happen sometime in the Fall.
Time | Talk | Presenter |
---|---|---|
13:30 | Beam pipe etc pics ( 00:10 ) 4 files | |
13:40 | Single sensor CMM measurements ( 00:20 ) 0 files | Hao |
14:00 | item 2. : bfc timing ( 00:20 ) 0 files | |
14:20 | item d. : offline structures ( 00:20 ) 1 file |
HFT Software
Updated on Thu, 2012-03-01 14:01. Originally created by margetis on 2012-03-01 12:44.510-4867333, at 18:30 (GMT), duration : 00:00
Agenda for Internal Review of Y2013-base geometry
Place: BNL/EVO, Date: March 9, 2012
Reviewers: Eric Anderssen, Howard Wieman (rerp. by Leo Greiner), Yuri Fisyak , Jason Webb, Xin Dong, +"Management" (not Flemming since he is an author)
Presentations/ Content
- Overview 10' Spiros
* context but also what is this geometry for
* This is not only about what the review is
but also what we want from the product
- comparisons of SW model and Flemmings implementation
20' Flemming
- Geant modeling and comparison with SW model
20-30' Jonathan
- Comments after walkthrough of code (issues, clarity etc)
10-15' Jason (?)
- Numbering schemes - 10' Spiros (?) Mostly restate what
was agreed upon
- BFC-tests with simple tracks. Timing/Issues
10-15' Jonathan
- Round table discussion. Action items defined.
Time | Talk | Presenter |
---|---|---|
13:30 | IST numbering ( 00:20 ) 1 file | |
13:30 | Minutes ( 00:20 ) 1 file | |
13:50 | prototype patch Acceptance/Efficiency for D0s ( 00:20 ) 2 files | jonathan |
HFT Y2013 Geometry Review
Updated on Mon, 2012-03-05 17:50. Originally created by margetis on 2012-03-01 12:44.BNL/EVO, at 18:30 (GMT), duration : 00:00
You have BOOKED a meeting in EVO (http://evo.caltech.edu).
Title: HFT Y2013 Geometry Review -
PLACE: BNL, Rm 1-189 from 1.30-3.30 Fri 3/9/2012
Description: STAR-HFT detector internal review
Community: STAR
Password: geometry
Meeting Access Information:
- Meeting URL
http://evo.caltech.edu/evoNext/koala.jnlp?meeting=MaMDMt2I22D2Du9e98DI9a
- Password: geometry
- Phone Bridge
ID: 487 6317
Password: 1193
Eastern Standard Time (-0500)
Start 2012-03-09 13:30
End 2012-03-09 18:00
Time | Talk | Presenter |
---|---|---|
13:30 | Overview 10' ( 00:20 ) 1 file | Spiros |
13:40 | Comparisons of SW model and Flemmings implementation ~15' ( 00:20 ) 1 file | Flemming |
13:50 | Geant modeling and comparison with SW model 20-30' ( 00:20 ) 3 files | Jonathan |
13:55 | Comments after walkthrough of code [in advance] (issues, clarity etc) 10-15' ( 00:20 ) 1 file | Jason |
14:00 | HFT-Numbering scheme/doc - 10' ( 00:20 ) 2 files | Spiros |
14:15 | BFC-tests with simple tracks. Timing/Issues 10-15' ( 00:20 ) 3 files | Jonathan |
14:35 | Action items/Summary ( 00:20 ) 0 files | All |
IST prototype stave testing
Updated on Thu, 2012-03-01 12:49. Originally created by nieuwhzs on 2012-03-01 12:17.Speaker : Dr. Gerrit J. van Nieuwenhuizen II ( Massachusetts Institute of Technology )
Talk time : 13:45, Duration : 00:20
gas flow study, 6A
We have switched to high gas flow around 2 pm on Tuesday, Feb 29. The purpose was to increase removal of the oxygen drifting in to detector due to diffusion.
Run 9 NPE Analysis in p+p collisions at 200 GeV
Dataset & cuts
Run 9 p+p 200 GeV 105M vpdMB events after selection.
First reco FGT track in pp200, 2012, gas mix 10-90, Feb 26
run 13057059, taken just before beam dump (no CNI background).
2nd check of Run12
These plots include the data from the first check (i.e.
new cluster file for st_physics_13050045_raw_2010002 -
new format, dead strip masking enabled, dead strip jumping enabled
first 300 evts
new radio plots for st_physics_13050045_raw_2010002
The difference with the previous plots is:
-used seeded cluster algo