Attic

Retired Simulation Pages kept here.

Action Items

Immediate action items:

  •  Y2008 tag
    • find out about the status of the FTPC (can't locate the relevant e-mail now)
    • find out about the status of PMD in 2008 (open/closed)
    • ask Akio about possible updates of the FMS code, get the final version
    • based on Dave's records, add a small amount of material to the beampipe
    • review the tech drawings from Bill and Will and others and start coding the support structure
    • extract information from TOF people about the likely configuration
    • when ready, produce the material profile plots for Y2008 in slices in Z
  • TUP tags
    • work with Jim Thomas, Gerrit and primarily Spiros on the definition of geometry for the next TUP wave
    • coordinate with Spiros, Jim and Yuri a possible repass of the trecent TUP MC data without the IST
  • Older tags
    • check the more recent correction to the SVT code (carbon instead of Be used in the water channels)
    • provide code for the correction for 3 layers of mylar on the beampipe as referred to above in Y2008
    • check with Dave about the dimensions of the water channels (likely incorrect in GEANT)
    • determine which years we will choose to retrofit with improved SVT (ask STAR members)
  • MTD
    • Establish a new UPGRXX tag for the MTD simulation
    • supervise and help Lijuan in extending the filed map
    • provide facility for reading a separate map in starsim and root4star (with Yuri)
  • Misc
    • collect feedback on possible simulation plans for the fall'07
    • revisit the codes for event pre-selection ("hooks")
    • revisit the event mixing scripts
  • Development
    • create a schema to store MC run catalog data with a view to automate job definition (Michael has promised help)

 

Beampipe support geometry and other news

Documentation for the beampipe support geometry description development

After the completion of the 2007 run, the SVT and the SSD were removed from the STAR detector along with there utility lines. The support structure for the beampipe remained, however.

The following drawings describe the structure of the beampipe support as it exists in the late 2007 and probably throughout 2008

Further corrections to the SVT geometry model
 
In the course of recent discussion of the beampipe support and shield material, Dave Lynn has found that even though according to the plans, the material of the cooling water channels in the SVT was specified as Be, in reality carbon composite material was used for that purpose. Below, there are materil vs pseudorapidity plots for the "old" and "new" codes
 
 
 
It can be seen that the difference is of the order of 0.4% rad. length on top of the existing (roughly) 6%. This is enough grounds for cutting a new version of the geometry and will shall create a geometry tag Y2007A which will reflect such change.
 

Datasets

Here we present information about our datasets.

2005

Description
Dataset name
Statistics, thousands
Status
Moved to HPSS
Comment
Herwig 6.507, Y2004Y
rcf1259
225
Finished
Yes
  7Gev<Pt<9Gev
Herwig 6.507, Y2004Y
rcf1258
248
Finished
Yes
  5Gev<Pt<7Gev
Herwig 6.507, Y2004Y
rcf1257
367
Finished
Yes
  4Gev<Pt<5Gev
Herwig 6.507, Y2004Y
rcf1256
424
Finished
Yes
  3Gev<Pt<4Gev
Herwig 6.507, Y2004Y
rcf1255
407
Finished
Yes
  2Gev<Pt<3Gev
Herwig 6.507, Y2004Y
rcf1254
225
Finished
Yes
  35Gev<Pt<100Gev
Herwig 6.507, Y2004Y
rcf1253
263
Finished
Yes
  25Gev<Pt<35Gev
Herwig 6.507, Y2004Y
rcf1252
263
Finished
Yes
  15Gev<Pt<25Gev
Herwig 6.507, Y2004Y
rcf1251
225
Finished
Yes
  11Gev<Pt<15Gev
Herwig 6.507, Y2004Y
rcf1250
300
Finished
Yes
  9Gev<Pt<11Gev
Hijing 1.382 AuAu 200 GeV minbias, 0< b < 20fm
rcf1249
24
Finished
Yes
Tracking,new SVT geo, diamond: 60, +-30cm, Y2005D
Herwig 6.507, Y2004Y
rcf1248
15
Finished
Yes
35Gev<Pt<45Gev
Herwig 6.507, Y2004Y
rcf1247
25
Finished
Yes
25Gev<Pt<35Gev
Herwig 6.507, Y2004Y
rcf1246
50
Finished
Yes
15Gev<Pt<25Gev
Herwig 6.507, Y2004Y
rcf1245
100
Finished
Yes
11Gev<Pt<15Gev
Herwig 6.507, Y2004Y
rcf1244
200
Finished
Yes
  9Gev<Pt<11Gev
CuCu 62.4 Gev, Y2005C
rcf1243
5
Finished
No
same as 1242+ keep Low Energy Tracks
CuCu 62.4 Gev, Y2005C
rcf1242
5
Finished
No
SVT tracking test, 10 keV e/m process cut (cf. rcf1237)
10 J/Psi, Y2005X, SVT out
rcf1241
30
Finished
No
Study of the SVT material effect
10 J/Psi, Y2005X, SVT in
rcf1240
30
Finished
No
Study of the SVT material effect
100 pi0, Y2005X, SVT out
rcf1239
18
Finished
No
Study of the SVT material effect
100 pi0, Y2005X, SVT in
rcf1238
20
Finished
No
Study of the SVT material effect
CuCu 62.4 Gev, Y2005C
rcf1237
5
Finished
No
SVT tracking test, pilot run
Herwig 6.507, Y2004Y
rcf1236
8
Finished
No
Test run for initial comparison with Pythia, 5Gev<Pt<7Gev
Pythia, Y2004Y
rcf1235
100
Finished
No
MSEL=2, min bias
Pythia, Y2004Y
rcf1234
90
Finished
No
MSEL=0,CKIN(3)=0,MSUB=91,92,93,94,95
Pythia, Y2004Y, sp.2
(CDF tune A)
rcf1233
308
Finished
Yes
4<Pt<5, MSEL=1, GHEISHA
Pythia, Y2004Y, sp.2
(CDF tune A)
rcf1232
400
Finished
Yes
3<Pt<4, MSEL=1, GHEISHA
Pythia, Y2004Y, sp.2
(CDF tune A)
rcf1231
504
Finished
Yes
2<Pt<3, MSEL=1, GHEISHA
Pythia, Y2004Y, sp.2
(CDF tune A)
rcf1230
104
Finished
Yes
35<Pt, MSEL=1, GHEISHA
Pythia, Y2004Y, sp.2
(CDF tune A)
rcf1229
208
Finished
Yes
25<Pt<35, MSEL=1, GHEISHA
Pythia, Y2004Y, sp.2
(CDF tune A)
rcf1228
216
Finished
Yes
15<Pt<25, MSEL=1, GHEISHA
Pythia, Y2004Y, sp.2
(CDF tune A)
rcf1227
216
Finished
Yes
11<Pt<15, MSEL=1, GHEISHA
Pythia, Y2004Y, sp.2
(CDF tune A)
rcf1226
216
Finished
Yes
9<Pt<11, MSEL=1, GHEISHA
Pythia, Y2004Y, sp.2
(CDF tune A)
rcf1225
216
Finished
Yes
7<Pt<9, MSEL=1, GHEISHA
Pythia, Y2004Y, sp.2
(CDF tune A)
rcf1224
216
Finished
Yes
5<Pt<7, MSEL=1, GHEISHA
Pythia special tune2
Y2004Y, GCALOR
rcf1223
100
Finished
Yes
4<Pt<5, GCALOR
Pythia special tune2
Y2004Y, GHEISHA
rcf1222
100
Finished
Yes
4<Pt<5, GHEISHA
Pythia special run 3
Y2004C
rcf1221
100
Finished
Yes
ENER 200.0, MSEL 2, MSTP (51)=7,
MSTP (81)=1, MSTP (82)=1, PARP (82)=1.9,
PARP (83)=0.5, PARP (84)=0.2,
PARP (85)=0.33, PARP (86)=0.66,
PARP (89)=1000, PARP (90)=0.16,
PARP (91)=1.0, PARP (67)=1.0
Pythia special run 2
Y2004C
(CDF tune A)
rcf1220
100
Finished
Yes

ENER 200.0, MSEL 2, MSTP (51)=7,
MSTP (81)=1, MSTP (82)=4, PARP (82)=2.0,
PARP (83)=0.5, PARP (84)=0.4,
PARP (85)=0.9, PARP (86)=0.95,
PARP (89)=1800, PARP (90)=0.25,
PARP (91)=1.0, PARP (67)=4.0

Pythia special run 1
Y2004C
rcf1219
100
Finished
Yes
ENER 200.0, MSEL 2, MSTP (51)=7,
MSTP (81)=1, MSTP (82)=1, PARP (82)=1.9, PARP (83)=0.5, PARP (84)=0.2,
PARP (85)=0.33, PARP (86)=0.66,
PARP (89)=1000, PARP (90)=0.16,
PARP (91)=1.5, PARP (67)=1.0
Hijing 1.382 AuAu 200 GeV central
0< b < 3fm
rcf1218
50
Finished
Yes
Statistics enhancement of rcf1209 with
a smaller diamond: 60, +-30cm, Y2004a
Hijing 1.382 CuCu 200 GeV minbias
0< b < 14 fm
rcf1216
52
Finished
Yes
Geometry: Y2005x
Hijing 1.382 AuAu 200 GeV minbias
0< b < 20 fm
rcf1215
100
Finished
Yes
Geometry: Y2004a, Special D decays

2006

Description
Dataset name
Statistics, thousands
Status
Moved to HPSS
Comment
AuAu 200 GeV central

rcf1289

1

Finished

No

upgr06: Hijing, D0 and superposition
AuAu 200 GeV central

rcf1288

0.8

Finished

No

upgr11: Hijing, D0 and superposition
AuAu 200 GeV min bias

rcf1287

5

Finished

No

upgr11: Hijing, D0 and superposition
AuAu 200 GeV central

rcf1286

1

Finished

No

upgr10: Hijing, D0 and superposition
AuAu 200 GeV min bias

rcf1285

6

Finished

No

upgr10: Hijing, D0 and superposition
AuAu 200 GeV central

rcf1284

1

Finished

No

upgr09: Hijing, D0 and superposition
AuAu 200 Gev min bias

rcf1283

6

Finished

No

upgr09: Hijing, D0 and superposition
AuAu 200 GeV min bias

rcf1282

38

Finished

No

upgr06: Hijing, D0 and superposition
AuAu 200 GeV min bias

rcf1281

38

Finished

Yes

upgr08: Hijing, D0 and superposition
AuAu 200 GeV min bias

rcf1280

38

Finished

Yes

upgr01: Hijing, D0 and superposition
AuAu 200 GeV min bias

rcf1279

38

Finished

Yes

upgr07: Hijing, D0 and superposition
Extension of 1276: D0 superposition
rcf1278
5
Finished

No

upgr07: Z cut=+-300cm
AuAu 200 GeV min bias
rcf1277
Finished
No
upgr05: Z cut=+-300cm
AuAu 200 GeV min bias
rcf1276
35
Finished
No
upgr05: Hijing, D0 and superposition
Pythia 200 GeV + HF
rcf1275
23*4
Finished
No
J/Psi and Upsilon(1S,2S,3S) mix for embedding
AuAu 200 GeV min bias
rcf1274
10
Finished
No
upgr02 geo tag, |eta|<1.5 (tracking upgrade request)
Pythia 200 GeV
rcf1273
600
Finished
Yes
Pt <2 (Completing the rcf1224-1233 series)
CuCu 200 GeV min bias+D0 mix
rcf1272
50+2*50*8
Finished
Yes
Combinatorial boost of rcf1261, sigma: 60, +-30
Pythia 200 GeV
rcf1233
300
Finished
Yes
4< Pt <5 (rcf1233 extension)
Pythia 200 GeV
pds1232
200
Finished
Yes
3< Pt <4 (rcf1232 clone)
Pythia 200 GeV
pds1231
240
Finished
Yes
2< Pt <3 (rcf1231 clone)
Pythia 200 GeV
rcf1229
200
Finished
Yes
25< Pt <35 (rcf1229 extension)
Pythia 200 GeV
rcf1228
200
Finished
Yes
15< Pt <25 (rcf1228 extension)
Pythia 200 GeV
rcf1227
208
Finished
Yes
11< Pt <15 (rcf1227 extension)
Pythia 200 GeV
rcf1226
200
Finished
Yes
9< Pt <11 (rcf1226 extension)
Pythia 200 GeV
rcf1225
200
Finished
Yes
7< Pt <9 (rcf1225 extension)
Pythia 200 GeV
rcf1224
212
Finished
Yes
5< Pt <7 (rcf1224 extension)
Pythia 200 GeV Y2004Y CDF_A
rcf1271
120
Finished
Yes
55< Pt <65
Pythia 200 GeV Y2004A CDF_A
rcf1270
120
Finished
Yes
45< Pt <55
CuCu 200 GeV min bias
rcf1266
10
Finished
Yes
SVT study: clams and two ladders
CuCu 200 GeV min bias
rcf1265
10
Finished
Yes
SVT study: clams displaced
CuCu 200 GeV min bias
rcf1264
10
Finished
Yes
SVT study: rotation of the barrel
CuCu 62.4 GeV min bias+D0 mix
rcf1262
50*3
Finished
Yes
3 subsets: Hijing, single D0, and the mix
CuCu 200 GeV min bias+D0 mix
rcf1261
50*3
Finished
No
3 subsets: Hijing, single D0, and the mix
1 J/Psi over 200GeV minbias AuAu
rcf1260
10
Finished
No
J/Psi mixed with 200GeV AuAu Hijing Y2004Y 60/35 vertex

2007

Unless stated otherwise, all pp collisions are modeled with Pythia, and all AA collisions with Hijing. Statistics is listed in thousands of events. Multiplication factor in some of the records refelcts the fact that event mixing was done for a few types of particles, on the same base of original event files.

Name System/Energy Statistics Status HPSS Comment Site
rcf1290 AuAu200 0<b<3fm, Zcut=5cm 32*5 Done Yes Hijing+D0+Lac2+D0_mix+Lac2_mix rcas
rcf1291 pp200/UPGR07/Zcut=10cm 10 Done Yes ISUB = 11, 12, 13, 28, 53, 68 rcas
rcf1292 pp500/UPGR07/Zcut=10cm 10 Done Yes ISUB = 11, 12, 13, 28, 53, 68 rcas
rcf1293 pp200/UPGR07/Zcut=30cm 205 Done Yes ISUB = 11, 12, 13, 28, 53, 68 rcas
rcf1294 pp500/UPGR07/Zcut=30cm 10 Done Yes ISUB = 11, 12, 13, 28, 53, 68 rcas
rcf1295 AuAu200 0<b<20fm, Zcut=30cm 20 Done Yes QA run for the Y2007 tag rcas
rcf1296 AuAu200 0<b<3fm, Zcut=10cm 100*5 Done Yes Hijing,B0,B+,B0_mix,B+_mix, Y2007 rcas
rcf1297 AuAu200 0<b<20fm, Zcut=300cm 40 Done Yes Pile-up simulation in the TUP studies, UPGR13 rcas
rcf1298 AuAu200 0<b<3fm, Zcut=15cm 100*5 Done Part Hijing,D0,Lac2,D0_mix,Lac2_mix, UPGR13 rcas
rcf1299 pp200/Y2005/Zcut=50cm 800 Done Yes Pythia, photon mix, pi0 mix rcas
rcf1300 pp200/UPGR13/Zcut=15cm 100 Done No Pythia, MSEL=4 (charm) rcas
rcf1301 pp200/UPGR13/Zcut=300cm 84 Done No Pythia, MSEL=1, wide vertex rcas
rcf1302 pp200 Y2006C 120 Done No Pythia for Spin PWG, Pt(45,55)GeV rcas
rcf1303 pp200 Y2006C 120 Done No Pythia for Spin PWG, Pt(35,45)GeV rcas
rcf1304 pp200 Y2006C 120 Done No Pythia for Spin PWG, Pt(55,65)GeV rcas
rcf1296 Upsilon S1,S2,S3 + Hijing 15*3 Done No Muon Telescope Detector, ext.of 1296 rcas
rcf1306 pp200 Y2006C 400 Done Yes Pythia for Spin PWG, Pt(25,35)GeV rcas
rcf1307 pp200 Y2006C 400 Done Yes Pythia for Spin PWG, Pt(15,25)GeV rcas
rcf1308 pp200 Y2006C 420 Done Yes Pythia for Spin PWG, Pt(11,15)GeV rcas
rcf1309 pp200 Y2006C 420 Done Yes Pythia for Spin PWG, Pt(9,11)GeV rcas
rcf1310 pp200 Y2006C 420 Done Yes Pythia for Spin PWG, Pt(7,9)GeV rcas
rcf1311 pp200 Y2006C 400 Done Yes Pythia for Spin PWG, Pt(5,7)GeV rcas
rcf1312 pp200 Y2004Y 544 Done No Di-jet CKIN(3,4,7,8,27,28)=7,9,0.0,1.0,-0.4,0.4 rcas
rcf1313 pp200 Y2004Y 760 Done No Di-jet CKIN(3,4,7,8,27,28)=9,11,-0.4,1.4,-0.5,0.6 rcas
rcf1314 pp200 Y2004Y 112 Done No Di-jet CKIN(3,4,7,8,27,28)=11,15,-0.2,1.2,-0.6,-0.3 Grid
rcf1315 pp200 Y2004Y 396 Done No Di-jet CKIN(3,4,7,8,27,28)=11,15,-0.5,1.5,-0.3,0.4 Grid
rcf1316 pp200 Y2004Y 132 Done No Di-jet CKIN(3,4,7,8,27,28)=11,15,0.0,1.0,0.4,0.7 Grid
rcf1317 pp200 Y2006C 600 Done Yes Pythia for Spin PWG, Pt(4,5)GeV Grid
rcf1318 pp200 Y2006C 690 Done Yes Pythia for Spin PWG, Pt(3,4)GeV Grid
rcf1319 pp200 Y2006C 690 Done Yes Pythia for Spin PWG, Minbias Grid
rcf1320 pp62.4 Y2006C 400 Done No Pythia for Spin PWG, Pt(4,5)GeV Grid
rcf1321 pp62.4 Y2006C 250 Done No Pythia for Spin PWG, Pt(3,4)GeV Grid
rcf1322 pp62.4 Y2006C 220 Done No Pythia for Spin PWG, Pt(5,7)GeV Grid
rcf1323 pp62.4 Y2006C 220 Done No Pythia for Spin PWG, Pt(7,9)GeV Grid
rcf1324 pp62.4 Y2006C 220 Done No Pythia for Spin PWG, Pt(9,11)GeV Grid
rcf1325 pp62.4 Y2006C 220 Done No Pythia for Spin PWG, Pt(11,15)GeV Grid
rcf1326 pp62.4 Y2006C 200 Running No Pythia for Spin PWG, Pt(15,25)GeV Grid
rcf1327 pp62.4 Y2006C 200 Running No Pythia for Spin PWG, Pt(25,35)GeV Grid
rcf1328 pp62.4 Y2006C 50 Running No Pythia for Spin PWG, Pt(35,45)GeV Grid

2009

 

qqqqqqqqqqqqqqqqqqqqqqqqqqq
Name   SystemEnergy
Range   Statistics  Comment
 rcf9001  pp200, y2007g 03_04gev  690k  Jet Study AuAu200(PP200) JLC PWG
 rcf9002   04_05gev  686k  
 rcf9003   05_07gev  398k  
 rcf9004   07_09gev  420k  
 rcf9005   09_11gev  412k  
 rcf9006   11_15gev  420k  
 rcf9007   15_25gev  397k  
 rcf9008   25_35gev  400k  
 rcf9009   35_45gev  120k  
 rcf9010   45_55gev  118k  
 rcf9011   55_65gev  120k  
         

 

  Name   SystemEnergy  Range  Statistics        Comment
 rcf9021 pp200,y2008       03_04 GeV  690k  Jet Study AuD200(PP200) JLC PWG
 rcf9022    04_05 GeV  686k  
 rcf9023    05_07 GeV  398k  
 rcf9024    07_09 GeV  420k  
 rcf9025    09_11 GeV  412k  
 rcf9026    11_15 GeV  420k  
 rcf9027    15_25 GeV  397k  
 rcf9028    25_35 GeV  400k  
 rcf9029    35_45 GeV  120k  
 rcf9030    45_55 GeV  118k  
 rcf9031    55_99 GeV  120k  

 

 Name  SystemEnergy   Range   Statistics      Comment  
 rcf9041    PP500, Y2009  03_04gev  500k Spin Study PP500 Spin group(Matt,Jim,Jan) 2.3M evts
 rcf9042   04_05gev  500k  
 rcf9043   05_07gev  300k  
 rcf9044   07_09gev  250k  
 rcf9045   09_11gev  200k  
 rcf9046   11_15gev  100k  
 rcf9047   15_25gev  100k  
 rcf9048   25_35gev  100k  
 rcf9049   35_45gev  100k  
 rcf9050   45_55gev    25k  
 rcf9051   55_99gev    25k  
         
 rcf9061  CuCu200,y2005h  B0_14  200k CuCu200 radiation length budget, Y.Fisyak, KyungEon Choi.
 rcf9062 AuAu200, y2007h  B0_14  150k AuAu200 radiation length budget  Y.Fisyak ,KyungEon Choi

 

2010

Information on Monte Carlo Data Samples

 
You do not have access to view this node
 
Geometry y2009a
Library SL09g
Generator Pythia 6.4.22
Tune 320
Field -5.0
ETA -10 < η < +10
PHI -π < φ < +π
vertex 0, 0, -2
width 0.015, 0.015, 42.0
  
Sample  Channel Events
rcf10000 W+ → e+ nu 10k
rcf10001 W- → e- nu 6k
rcf10002 W+ → tau+ nu
W- → tau- nu
10k
rcf10003 pp → W+/- + jet 10k
rcf10004 Z e+e-, no Z/gamma interference 4k
rcf10005 Z all but e+e- 10k
rcf10006 QCD w/ partonic pT > 35 GeV 100k

 

Geometry Tag Options

 This page documents the options in geometry.g which define each of the production tags.

 This page documents the options in geometry.g which define each of the production tags.

 This page documents the options in geometry.g which define each of the production tags.

 This page documents the options in geometry.g which define each of the production tags.

 This page documents the options in geometry.g which define each of the production tags.

 This page documents the options in geometry.g which define each of the production tags.

Geometry Tag Options II

The attached spreadsheets document the production tags in STARSIM on 11/30/2009.  At that time the y2006h and y2010 tags were in development and not ready for production.

Material Balance Histograms

.

Y2008a

 y2008a full and TPC only material histograms

 

y2008aStar

 

1 2

 

y2008aTpce

 

 

y2005g

 

 .

 

y2005gStar

 

2
3

 

y2005gTpce

 

 

y2008yf

.

y2008yfStar

 

111
  `

 

y2008yfTpce

 

1

 

y2009

.

y2009Star

 

.
.

 

y2009Tpce

 

.

 

STAR AgML Geometry Comparison with STARSIM/AgSTAR

STAR Geometry Comparison: AgML vs AgSTAR

At the left is a general status for each geometry tag which compiles in AgML.  All volumes are tested recursively except for the "IBEM" and similar support structures for the VPD, and the Endcap SMD strips.  (The ESMD planes are tested as a unit, rather than test all 2*12*288 SMD strips).

Color codes:

Green: No differences larger than 1%

Yellow: The volume did not appear in AgSTAR geometry

Orange: Difference was larger than 1%, but absolute difference is absolutely negligible.

Red: A difference larger than 1% was detected for a significant amount of material; or a negligible but widespread difference was detected. 

At the right is a PDF file for each geometry tag. For each volume we show two plots. The top plot shows the absolute number of radiation lengths which a geantino encounters traversing the geometry, starting at the geometry and following a straight line at the given pseudorapidity. We average over all phi. The left (right) hashes show the AgML (AgSTAR) geometry. The difference (expressed as a fractional value) of the two histograms is shown the lower plot. Frequently the differences are small, e.g. 10^-6, and ROOT rescales the plots accordingly. Since it is difficult to read the scales of so many plots at once, we have color coded the plots. (Coding seems to fail in the generation of some histograms)... The meaning of the color coding is summarized below.

<?php
/********************************************************************** START OF PHP */

/* =======================================================
   Helper function to show the status_yXXXX.png
   ======================================================= */
function showImage( $tag, $dir ) {

   echo
"<img src=\"$dir/status_$tag.png\" />";

}

/* =======================================================
   Helper function to show the PDF file
   ======================================================= */
function showGoogle( $tag, $dir ) {
  
/*
   echo "<iframe border=\"0\" url=\"http://docs.google.com/gview?url=$dir$tag.pdf&amp;embedded=true\" style=\"width: 562px; height: 705px;\"> </iframe>";
   */

echo

"<iframe frameborder=\"0\" style=\"width: 562px; height: 705px;\" src=\"http://docs.google.com/gview?url=$dir/$tag.pdf&amp;embedded=true\"></iframe>"

;
}


/* =======================================================
   First some PHP input... find the date of the comparison
   ======================================================= */
$YEAR="2011";
$DATE="06-15-2011";
$DIR="http://www.star.bnl.gov/~jwebb/".$YEAR."/".$DATE."/AgML-Comparison/";
$TAGS=$DIR."TAGS";
/* =======================================================
   Output header for this page
   ======================================================= */

echo "<h3>STAR AgML vs AgSTAR Comparison on ".$DATE."</h3>";

/* =======================================================
   Read in each line in the TAGs file
   ======================================================= */
$handle = @fopen("$TAGS", "r");
if (
$handle) {
    while ((
$buffer = fgets($handle, 4096)) !== false) {

       
/* Trim the whitespace out of the string */
       
$buffer=trim($buffer);

       
/* Draw an HRULE and specify which geometry tag we are using */
       
echo "<hr><p>STAR Geometry Tag $buffer</p>";

       
/* Now build a 2-entry table with the status PNG on the left
           and the summary PDF ala google docs on the right */

       
showImage( $buffer, $DIR );

       
showGoogle( $buffer, $DIR );

    }
    if (!
feof($handle)) {
        echo
"Error: unexpected fgets() fail\n";
    }
   
fclose($handle);
}

/************************************************************************ END OF PHP */
?>

STAR AgML Language Reference

STAR Geometry Page

R&D Tags

The R&D conducted for the inner tracking upgrade required that a few specialized geometry tags be created. For a complete set of geometry tags, please visit the STAR Geometry in simulation & reconstruction page. The below serves as additional documentation and details.

Taxonomy:

  • SSD: Silicon strip detector
  • IST: Inner Silicon Tracker
  • HFT: Heavy Flavor Tracker
  • IGT: Inner GEM Tracker
  • HPD: Hybrid Pixel Detector

The TPC is present in all configuration listed below and the SVT is in none.

   Tag    

 SSD IST HFT IGT HPD Contact Person  Comment

UPGR01

+

 

+

 

 

   

UPGR02

 

+

+

 

 

   

UPGR03

 

+

+

+

 

   

UPGR04

+

 

 

 

+

 Sevil

retired

UPGR05

+

+

+

+

+

 Everybody

retired

UPGR06

 +

 

+

 

+

 Sevil

retired

UPGR07

 +

+

+

+

 

Maxim

 

UPGR08

 

+

+

+

+

Maxim

 

UPGR09

 

+

+

 

+

Gerrit

retired  Outer IST layer only

UPGR10

+

+

+

   

Gerrit

Inner IST@9.5cm

UPGR11

+

+

+

 

 

Gerrit

IST @9.5&@17.0

UPGR12

+

+

+

+

+

Ross Corliss

retired  UPGR05*diff.igt.radii

UPGR13

+

+

+

+

 

Gerrit

UPGR07*(new 6 disk FGT)*corrected SSD*(no West Cone)
UPGR14  +    +  +    Gerrit  UPGR13 - IST  
UPGR15 + + +     Gerrit  Simple Geometry for testing, Single IST@14cm, hermetic/polygon Pixel/IST geometry. Only inner beam pipe 0.5mm Be. Pixel 300um Si, IST 1236umSi  
UPGR20  +         Lijuan   Y2007 + one TOF  
UPGR21   +         Lijuan   UPGR20 + full TOF  

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Eta coverage of the SSD and HFT at different vertex spreads:

Z cut, cm

eta SSD eta HFT

5

1.63 

2.00

10

1.72

2.10

20

1.87

2.30

30

2.00

2.55

 

 

 

 

 

 

Material balance studies for the upgrade: presented below are the usual radiation length plots (as a function of rapidity).

 

Full UPGR05:

 

 

Forward region: the FST and the IGT ONLY:

 

 

Below, we plot the material for each individual detector, excluding the forward region to reduce ambiguity.

 

SSD:

 

 

IST:

 

 

HPD:

 

 

HFT: