Presentation is loading. Please wait.

Presentation is loading. Please wait.

Bill Atwood, SCIPP/UCSC, Jan. 30, 2006 GLAST 1 Closer to Reality From Last Talk ( 7-Jan-06) – things seemed Great! However... 1) In estimating the SRD.

Similar presentations


Presentation on theme: "Bill Atwood, SCIPP/UCSC, Jan. 30, 2006 GLAST 1 Closer to Reality From Last Talk ( 7-Jan-06) – things seemed Great! However... 1) In estimating the SRD."— Presentation transcript:

1 Bill Atwood, SCIPP/UCSC, Jan. 30, 2006 GLAST 1 Closer to Reality From Last Talk ( 7-Jan-06) – things seemed Great! However... 1) In estimating the SRD I use the normalized (true) Extra Galactic Diff Rate instead of our absolute(meas.) rate... Iissue: the acceptance (Aeff) falls off at lower energies (there's almost a factor of 3 here) 2) Our intend operational mode is "Rocking" exposing our backside Issue: Large gaps between CalModules (there's another factor of ~ 1.3 here) This analysis: Input: 1) First day of 5B Bkg. Run: dataset v7r3p5 (Includes rocking) 2) Extra Galactic Diff: dataset v7r3p5 3) All Gamma rep-V7r3p4 dataset, runs 401-800 All these datasets are "CTnew" mean application of the cuts shown by Julie prior to download

2 Bill Atwood, SCIPP/UCSC, Jan. 30, 2006 GLAST 2 Input: CTnew FT1ZenithAngle > 100 High Energy e- Filter Scrambled Tkr Filter Heavy Ion Filter.0.3.4.5.65.75 SRD 1:1 Background and Diffuse Integral Rates 100 200 500 1000 2000 5000 10000 E min CTBGAM CTBCORE >.1 && CTBBestEnergyProb.1 Base Class 1: CTBGAM >.35 Base Class 3: CTBGAM >.55 see next chart for Filter Definitions

3 Bill Atwood, SCIPP/UCSC, Jan. 30, 2006 GLAST 3 ( (min(abs(Tkr1XDir),abs(Tkr1YDir)) 0 & AcdActDistTileEnergy >.2) | (Tkr1SSDVeto -3 & AcdActDistTileEnergy >.15) | ( AcdActiveDist3D >(-30 + 30*(Tkr1FirstLayer-2))) ) & CTBBestEnergy > 5000 Hi Energy e- Filter: Heavy Ion Filter: CTBBestEnergy > 5000 & ((CalTransRms - 1.5*Tkr1ToTTrAve) < 5) (Tkr1FirstLayer - Tkr2FirstLayer) 4 & Tkr2TkrHDoca > 100 Scrambled Track Filter: Cosmic Proton: Tkr1FirstLayer -80 & ((AcdActDistTileEnergy + AcdActiveDist3D/100) > 1)

4 Bill Atwood, SCIPP/UCSC, Jan. 30, 2006 GLAST 4 Base Class 3: CTBCORE >.35 && CTBBestEnergyProb >.35 Same Contours as before Base Class 3: CTBGAM >.50

5 Bill Atwood, SCIPP/UCSC, Jan. 30, 2006 GLAST 5 On Axis Aeff x FoV Base Class 3 Cuts THIS ONE

6 Bill Atwood, SCIPP/UCSC, Jan. 30, 2006 GLAST 6 Bkg. Diffuse Base Class 3 Cuts

7 Bill Atwood, SCIPP/UCSC, Jan. 30, 2006 GLAST 7 Hadronic Res. Bkg. QED Res. Bkg. 100-500 MeV 500-2500 MeV 2500-12500 MeV > 12500 MeV Residual Background Broken out by Sources and CTBBestEnergy Irreducible: e+ Conversions Cosmic (Hi E) e- Cosmic Protons – ACD Leakage? Same energy bins as above Correlated  's!

8 Bill Atwood, SCIPP/UCSC, Jan. 30, 2006 GLAST 8 ACD Leakage Correlated Events: McDirErr <.1 and not e+ McId != -1 72 events Side Ribbons don't go to top! Estimate 47 events are leaked in this way These are the Top Corner Leakers found in the hand-scan Require events start in Top Layer Tkr1Z0 > 590 Composition:

9 Bill Atwood, SCIPP/UCSC, Jan. 30, 2006 GLAST 9 Project Tracks to + Const. X Sides and fold to YSide > 0: YSide = min(abs(Tkr1Y0 - abs( (832-abs(Tkr1X0))/Tkr1XDir) * Tkr1YDir), 742) ZSide = min(abs(Tkr1Z0 - abs( (832-abs(Tkr1X0))/Tkr1XDir) * Tkr1ZDir), 800) All Data Data Inside Holes All Gamma Ineff. = 90/105090 =.1%

10 Bill Atwood, SCIPP/UCSC, Jan. 30, 2006 GLAST 10 Suspect the same is true on Const. Y Sides – Evidence poor – Const. X Sides Holes Removed Both Sides Holes Removed Difference Combined: BKG: 209 DIFF: 63 GAM: 220

11 Bill Atwood, SCIPP/UCSC, Jan. 30, 2006 GLAST 11 Remaining Base Class 3 Residuals Hadronic QED Next step: separate out the CTBBestEnergy > 1 GeV and hand scan 69 Events after X,Y Side Holes

12 Bill Atwood, SCIPP/UCSC, Jan. 30, 2006 GLAST 12 P Primary 12.17GeV Tracking error in Y e+ Back-Entering 1.71GeV Shower Stub in Tracker Uncorrelated Events

13 Bill Atwood, SCIPP/UCSC, Jan. 30, 2006 GLAST 13 P Primary 32.55 GeV Acd Tile McPosHit 49KeV Ribbon Slot (10 of these) P Primary 4..494GeV Acd Tile McPosHit 1.57 MeV No ACD Digi Correlated Events

14 Bill Atwood, SCIPP/UCSC, Jan. 30, 2006 GLAST 14 e- cosmic 6.65 GeV Ribbon Ineff. And so on...

15 Bill Atwood, SCIPP/UCSC, Jan. 30, 2006 GLAST 15 Speculation: We may be able to kill most(all) of the Correlated Bkg. > 1 GeV If so where will we be - Present Status Corr. Bkgs. Removed Goal  = 35 events

16 Bill Atwood, SCIPP/UCSC, Jan. 30, 2006 GLAST 16 Top Ribbon Ineff. And... 45% Already There: 16 of these events are CTBBestEnergy > 1 GeV Req. CTBBestZ0 > 590 (Starts at the Top) & McDirErr <.1 (Correlated Event) This will be an issue on the sides as well Need DOCA to nearest Ribbon whether or not it was hit.... 69 Events Total (out of 365)


Download ppt "Bill Atwood, SCIPP/UCSC, Jan. 30, 2006 GLAST 1 Closer to Reality From Last Talk ( 7-Jan-06) – things seemed Great! However... 1) In estimating the SRD."

Similar presentations


Ads by Google