Here is the brief list of what are in the Down Scale DST files:
NOTE: There is no event cuts - all events are taken.
The main advantage of DownScaleDst files is smaller size compared to STAR MuDst files. It is about 50 times smaller than those of MuDst files. The smaller size results in faster data analysis.
Down Scale files could be used in flow analysis of charged or strange particles, high pt correlations.
mZdcAdcAttentuatedSumWest
mZdcAdcAttentuatedSumEast
mZdcSmdWest[16]
mZdcSmdEast[16]
mCtbMultiplicity
mPrimaryVertexX
mPrimaryVertexY
mPrimaryVertexZ
mX[2][3][2][31] // X component of the event plane vector
mY[2][3][2][31] // Y component of the event planevector
// Q[charge][harmonic][subEvent][etaBin]; harmonic = 0 => multiplicity;
//ETA BINS: FTPCE -4.1 < eta < -2.5 (8 bins); FTPCW 2.5 < eta < 4.1 (8 bins); TPC -1.5 < eta < 1.5 (15 bins)
mEventId
mRunId
mNumberOfGoodPrimaryTracks
mNumberOfV0Tracks
mNumberOfPrimaryTracks
mNominalTriggerId[32]
mCentrality // centrality calculated according to the standard STAR refMult regions
mRefMult
mRefMultEtaWide // refMult calculated from tracks with wide eta cut |eta|<0.8
V0.mTypeOfStrangeParticle // 0 Lambda; 1 Anti-Lambda; 2 K0Short
V0.mMomPos.fX
V0.mMomPos.fY
V0.mMomPos.fZ
V0.mMomNeg.fX
V0.mMomNeg.fY
V0.mMomNeg.fZ
V0.mPtV0
V0.mPtPos
V0.mPtNeg
V0.mIsPosPrimary // need to remove auto correlations if the pos V0 track is in Event Plane
V0.mIsNegPrimary // if the neg V0 track is in Event Plane v0IsPrimary = etaBin+1-(nEtaTotal+1)*(1-subEvent)
V0.mPseudoRapV0
V0.mPseudoRapPos
V0.mPseudoRapNeg
V0.mMassLambda
V0.mMassAntiLambda
V0.mMassK0Short
Primary.mId
Primary.mCharge
Primary.mMaxPoints
Primary.mFitPoints
Primary.mTrackInEventPlaneFlag // need to remove auto correlations if track is in Event Plane TrackInEventPlane = etaBin+1-(nEtaTotal+1)*(1-subEvent)
Primary.mDEdx
Primary.mPt
Primary.mPhi
Primary.mEta
Primary.mDcaGlobal.mX1
Primary.mDcaGlobal.mX2
Primary.mDcaGlobal.mX3