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Task #478

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Task #476: Calibrations

Aerogel

Added by Richard Trotta almost 5 years ago. Updated almost 2 years ago.

Status:
Resolved
Priority:
Normal
Start date:
07/11/2019
Due date:
% Done:

100%

Estimated time:

Description

Vladimir and Mireille will keep this updated.


Files

N0_100k.png (12.7 KB) N0_100k.png Vladimir Berdnikov, 04/11/2020 01:26 PM
N1_100k.png (12.6 KB) N1_100k.png Vladimir Berdnikov, 04/11/2020 01:26 PM
N2_100k.png (12.5 KB) N2_100k.png Vladimir Berdnikov, 04/11/2020 01:26 PM
N3_100k.png (12 KB) N3_100k.png Vladimir Berdnikov, 04/11/2020 01:26 PM
N4_100k.png (12.2 KB) N4_100k.png Vladimir Berdnikov, 04/11/2020 01:26 PM
N5_100k.png (11.7 KB) N5_100k.png Vladimir Berdnikov, 04/11/2020 01:26 PM
N6_100k.png (12.2 KB) N6_100k.png Vladimir Berdnikov, 04/11/2020 01:26 PM
P0_100k.png (11.7 KB) P0_100k.png Vladimir Berdnikov, 04/11/2020 01:26 PM
P1_100k.png (12.2 KB) P1_100k.png Vladimir Berdnikov, 04/11/2020 01:26 PM
P2_100k.png (12 KB) P2_100k.png Vladimir Berdnikov, 04/11/2020 01:26 PM
fit_N.png (21.7 KB) fit_N.png Vladimir Berdnikov, 04/11/2020 01:27 PM
fit_P.png (25.9 KB) fit_P.png Vladimir Berdnikov, 04/11/2020 01:27 PM
P4_100k.png (12.2 KB) P4_100k.png Vladimir Berdnikov, 04/11/2020 01:27 PM
P5_100k.png (12 KB) P5_100k.png Vladimir Berdnikov, 04/11/2020 01:27 PM
P6_100k.png (12.6 KB) P6_100k.png Vladimir Berdnikov, 04/11/2020 01:27 PM
Actions #1

Updated by Richard Trotta almost 5 years ago

  • Parent task set to #476
Actions #2

Updated by Richard Trotta almost 5 years ago

  • Status changed from New to In Progress
Actions #3

Updated by Richard Trotta over 4 years ago

  • % Done changed from 0 to 70
Actions #4

Updated by Vladimir Berdnikov about 4 years ago

Richard Trotta wrote:

Vladimir and Mireille will keep this updated.

The Aerogel detector calibration procedure include:

  • The conversion of the flash ADC sample values to photoelectrons. The conversion coefficient is the difference between mean values of channel pedestal and first photoelectron peak which determined from Gauss fits of cosmic or beam data. This procedure needed for all channels and in the end you have set of conversions coefficients.
  • Second step is the control of the position of the single electron peak versus time for each channel. It achieved by fitting experimental data (fADC spectrum) with more complex function (Poisson + three Gauss) over all experiment period.

Work in progress...

Actions #5

Updated by Vladimir Berdnikov about 4 years ago

Richard Trotta wrote:

Vladimir and Mireille will keep this updated.

Actions #6

Updated by Richard Trotta almost 2 years ago

  • Status changed from In Progress to Closed
  • % Done changed from 70 to 100
Actions #7

Updated by Richard Trotta almost 2 years ago

  • Status changed from Closed to Resolved
Actions

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