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2006 Relative Luminosity

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2006 Relative Luminosity. Tai Sakuma MIT 6/13/2007. Contents. 2006 Fill Pattern (bxing masking) Determination from CDEV Confirmation with BBC coincidence SpinDB 2006 Relative Luminosity Release BBC-ZDC comparison Preparation for 2008 Issues to be resolved before run 2008. - PowerPoint PPT Presentation
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QuickTime TIFF (Uncomp are needed 2006 Relative Luminosity Tai Sakuma Tai Sakuma MIT MIT 6/13/2007 6/13/2007
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Page 1: 2006 Relative Luminosity

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2006 Relative Luminosity2006 Relative Luminosity

Tai Sakuma Tai Sakuma MITMIT

6/13/20076/13/2007

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• 2006 Fill Pattern (bxing masking)– Determination from CDEV– Confirmation with BBC coincidence– SpinDB

• 2006 Relative Luminosity– Release– BBC-ZDC comparison

• Preparation for 2008– Issues to be resolved before run 2008

ContentsContents

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2006 Fill Pattern (bxing mask)2006 Fill Pattern (bxing mask)

• Spin sorted yields and relative luminosity should use the same set of the bxings.

• Choose bxings which are not in the abort gaps, not kicked, or lost.

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Determination of Fill Pattern (bxing mask)Determination of Fill Pattern (bxing mask)

• Determination of the fill patterns (bxing mask) from CDEV– <measuredFillPatternM>– Logical AND is taken to

determine one fill pattern (mask) for a RHIC fill.

• Confirmation with BBC coincidence– Minimum conincidence rates for

each bxing.

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Summary on Fill Pattern (bxing mask)Summary on Fill Pattern (bxing mask)

• 159 fills (2508 runs)– The number of the fills for which

the fill patterns (bxing mask) are

determined from CDEV. These patterns (masks) will be entered into SpinDB.

• 127 fills (2023 runs)– The number of the fills for which

the fill patterns (bxing mask) are confirmed with the BBC coincidence counts.

• 32 fills– No scaler files for those fills.

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2006 Relative Luminosity2006 Relative Luminosity

• Preliminary Release– http://deltag5.lns.mit.edu/~sakuma/protected/star/scaler/2006/prelim_release.shtml

– Used the fill patterns (bxing masks) that I determined– 566 runs for 80 fills

• Final Release– There will be the final release with the systematic

uncertainty.

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BBC-ZDC ComparisonBBC-ZDC Comparison

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The ratio of the ZDC and BBC coincidence counts jumps

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BBC-ZDC ComparisonBBC-ZDC Comparison

• Leading bunch effect– The ratio is large for the first ten bunches for the yellow and

blue beam

• Ripple effect– The ratio oscillates with low frequency

• Saw tooth effect– The ratio oscillates with high frequency

The ratio of the ZDC and BBC coincidence counts for bxings.

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Issues to be resolved for 2008Issues to be resolved for 2008

• Timestamp– For 2006, the clock used for the timestamp on the scaler files was not

synchronized with the STAR run time.

• BBC Coincidence Counts– For Board 6 for each run, the 1st file behaved differently from the 2nd and

after the 2nd files.– Board 7 and 8 don’t have good a vertex distribution.– Board 5, 6 timebin and board 6 bit 16 for 2nd and after the 2nd files are

consistent with board 11, 12 bit16. Board 5, 7, 8 bit 16 and board 6 bit 16 for 1st file are consistent with one another but not with board 11, 12.

• BBC - ZDC comparison– Coincidence counts is not flat over the time– Coincidence counts is not flat over the bxings.

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The Board Number

5 6(1st file)

6(2nd file~)

7 8 11 12

Bit 16 Timebin N/A N/A

: consistent with one another

: consistent with one another

and are not consistent with each other

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