Top Banner
Gamma-ray Large Gamma-ray Large Area Space Area Space Telescope Telescope Understanding Understanding SVAC CalMip SVAC CalMip Variables Variables Monica Pepe Stefano Germani INFN Perugia Instrument Analysis Meeting December 16, 2005
9

Gamma-ray Large Area Space Telescope Understanding SVAC CalMip Variables Monica Pepe Stefano Germani INFN Perugia Instrument Analysis Meeting December.

Dec 16, 2015

Download

Documents

Norah Byrd
Welcome message from author
This document is posted to help you gain knowledge. Please leave a comment to let me know what you think about it! Share it to your friends and learn new things together.
Transcript
Page 1: Gamma-ray Large Area Space Telescope Understanding SVAC CalMip Variables Monica Pepe Stefano Germani INFN Perugia Instrument Analysis Meeting December.

Gamma-ray Large Area Gamma-ray Large Area Space TelescopeSpace Telescope

Understanding Understanding SVAC CalMip VariablesSVAC CalMip Variables

Monica PepeStefano Germani

INFN Perugia

Instrument Analysis MeetingDecember 16, 2005

Page 2: Gamma-ray Large Area Space Telescope Understanding SVAC CalMip Variables Monica Pepe Stefano Germani INFN Perugia Instrument Analysis Meeting December.

SVAC Instrument Analysis Meeting, December 16, 2005

Stefano Germani & Monica Pepe 2

OutlookOutlook

• Aim of the work:– First look to the new CalMip variables in the

SVAC ntuple• Consistency check (Monica)• Direction and Correlation with tracks (Stefano)

• Data:– Surface Muons 1M Montecarlo

• SVAC Ntuple/nfs/farm/g/glast/u11/InstrumentAnalysis/MC/EngineeringModel-v5r0703p3/LAT_Surface_Muons/surface_muons_1M_svac.root

Page 3: Gamma-ray Large Area Space Telescope Understanding SVAC CalMip Variables Monica Pepe Stefano Germani INFN Perugia Instrument Analysis Meeting December.

SVAC Instrument Analysis Meeting, December 16, 2005

Stefano Germani & Monica Pepe 3

CalMipNumCalMipNum

All Events TkrNumTracks=1 Events

CalMipNum CalMipNum

Why zero Mips?

Why more than one Mip?

CalMipNum Event Fraction

0 42.9 %

1 52.4 %

2 4.6 %

3 0.03 %

4 8E-6

Page 4: Gamma-ray Large Area Space Telescope Understanding SVAC CalMip Variables Monica Pepe Stefano Germani INFN Perugia Instrument Analysis Meeting December.

SVAC Instrument Analysis Meeting, December 16, 2005

Stefano Germani & Monica Pepe 4

Why 1 Track and 0 Mip (Why 1 Track and 0 Mip (II) ?) ?

Tkr1NumHits Tkr1NumHits

1 Track and 0 Mip 1 Track and 1 Mip

The Track may not reach the CAL

as seen in next slides

Page 5: Gamma-ray Large Area Space Telescope Understanding SVAC CalMip Variables Monica Pepe Stefano Germani INFN Perugia Instrument Analysis Meeting December.

SVAC Instrument Analysis Meeting, December 16, 2005

Stefano Germani & Monica Pepe 5

Why 1 Track and 0 Mip (Why 1 Track and 0 Mip (IIII) ?) ?

Tkr1EndPos 0 Mip

Tkr1EndPos 1 Mip

Tkr1EndPos

No Mip found if track ends on LAT edge

Page 6: Gamma-ray Large Area Space Telescope Understanding SVAC CalMip Variables Monica Pepe Stefano Germani INFN Perugia Instrument Analysis Meeting December.

SVAC Instrument Analysis Meeting, December 16, 2005

Stefano Germani & Monica Pepe 6

Why 1 Track and 0 Mip (Why 1 Track and 0 Mip (IIIIII) ?) ?

Tkr1 Extrapolation to Cal: 0 Mip

Tkr1 Extrapolation to Cal: 1 Mip

Tkr1 Extrapolation at CAL entry

No Mip found if track extrapolation do not enter in CAL

Page 7: Gamma-ray Large Area Space Telescope Understanding SVAC CalMip Variables Monica Pepe Stefano Germani INFN Perugia Instrument Analysis Meeting December.

SVAC Instrument Analysis Meeting, December 16, 2005

Stefano Germani & Monica Pepe 7

Why 1 Track and >1 Mip ?Why 1 Track and >1 Mip ?

Mip Finder algorithm can find several Mip Track segments due to CAL segmentation and position resolution (Thanks Fred!)

CalMip2Pos(X) vs CalMip1Pos(X)

CalMip2Pos(Z) vs CalMip1Pos(Z)

CalMip2Pos(Y) vs CalMip1Pos(Y)

The two Mip segments belong to the same TRUE Mip (separated along Z: if Mip1 is at High Z Mip2 is at Low Z)

mm

mm

mm

mm

mm

mm

Page 8: Gamma-ray Large Area Space Telescope Understanding SVAC CalMip Variables Monica Pepe Stefano Germani INFN Perugia Instrument Analysis Meeting December.

SVAC Instrument Analysis Meeting, December 16, 2005

Stefano Germani & Monica Pepe 8

MIP EnergyMIP Energy

CalMip1Ecor

MeV

MeV

CalMip1Erm CalMip1Erm vs Mip Track Length

mm

MeV

CalMip1Ecor

is the mean vertical-equivalent energy averaging path length corrected energy on layer basis

CalMip1Erm

is the total energy in a cylinder of

1 Moliere radius (35 mm in CsI)

Page 9: Gamma-ray Large Area Space Telescope Understanding SVAC CalMip Variables Monica Pepe Stefano Germani INFN Perugia Instrument Analysis Meeting December.

SVAC Instrument Analysis Meeting, December 16, 2005

Stefano Germani & Monica Pepe 9

ConclusionsConclusions

• CalMip Ntuple – variables seems to be correctly filled

• Mip Finder – behaves as expected when the muon track

reaches the CAL

– Multiple Mips associated to the same track are actually segments of the same MIP

• Would it be necessary to improve the algorithm in order to take into account these topologies?