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Landau Functions

Trying to understand why fitting with nMip>2 seems to not work….

I ripped out just the definition part of Mike’s fitting routine:

noise pickup at STAR

scope capture from 2/12/2019

Conditions:

Test 1

100' twinax cable connected to port 1 of GGDII board 1.

TPC data volume spikes II. (GG Driver)

After yesterdays 10am mtg the east/west GG driver cables were swapped.   

2019 sQM

 

SQM abstract

TPC data volume spikes

 I've been looking at the sizes for the TPC data volume spikes.  

W A_L DIS2019 abstract

 

Dijet Sivers Asymmetry in Run12+Run15 pp200

 

GSTAR devices

As far as I know, STAR has never been able to simulate the entire detector when it includes forward (eta>2) detectors like EPD or BBC.  (Is ETOF included?  FCAL?)

EPD Calibration check for 2018

In this blog by Mike, he noted as expected the first mip peaks of the EPD are the same for both the Isobar runs (at 200 GeV) and for the 27 GeV Au+Au run: