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Re: comparison of run8 results
- To: Claude Petitjean <claude.petitjean@psi.ch>
- Subject: Re: comparison of run8 results
- From: Tom Banks <tbanks@socrates.berkeley.edu>
- Date: Wed, 27 Sep 2006 14:45:55 -0700 (PDT)
- Cc: Peter Kammel <kammel@npl.uiuc.edu>, analysis -- Tom Banks <tbanks@socrates.berkeley.edu>, Steve Clayton <smclayto@uiuc.edu>, Tim Gorringe <gorringe@pa.uky.edu>, Fred Gray <fegray@socrates.berkeley.edu>, David Hertzog <hertzog@uiuc.edu>, Malte Hildebrandt <malte.hildebrandt@psi.ch>, Brendan Kiburg <kiburg@npl.uiuc.edu>, Sara Knaack <sknaack@uiuc.edu>, Berhard Lauss <lauss@socrates.berkeley.edu>, Marat Vznuzdaev <marat@mail.pnpi.spb.ru>, Levchenko Mikhail <mishelev@pnpi.spb.ru>, Francoise Mulhauser <Francoise.Mulhauser@psi.ch>, "R. Prieels" <prieels@fynu.ucl.ac.be>, Vladimir Tishchenko <tishenko@pa.uky.edu>, Peter Winter <peter.winter@psi.ch>
- In-reply-to: <451ADCD9.1000008@psi.ch>
- References: <Pine.LNX.4.21.0609262227510.9748-100000@one.npl.uiuc.edu><451ADCD9.1000008@psi.ch>
Dear Claude,
we are on the same wavelength: Last night I wrote an addendum to my report
(Appendix E.4, p.86) which contains a table with a side-by-side comparison
of my and Steve's reported results. It looks essentially like your
comparison below, although not as detailed. I will try to incorporate
some of your additional fields into my table so that we can have a good
reference for the meeting.
Regarding some of your questions:
> - Steve sees less mu-scatters, but this may be due to a different
> track finding algorithm
Steve's scatters-removed rate shift is definitely smaller in magnitude
than mine (-1.1 Hz vs. -3.1), but it's difficult to compare our results
until I know his identified scatter fraction. It could be that our rate
shifts are consistent if we normalize to the same scatter fraction.
> 7) cosmics errors adjusted -3.1 (-0.2 incl in 1)
> (n.a.)
> - why is the adjustment of cosmics error so different? Needs to be
> discussed
There is actually not a problem here; I'm afraid that my report was a
little misleading in this respect, for the following reason: In my last
production analysis, I formed the cosmics lifetime histogram using the
data set in which scatters had been removed. Thus the -3.1 shift which
you are attributing to the cosmic error adjustment is actually due to the
removal of muon scatters. As I mention in the text, adjusting the bin
errors to account for cosmics has almost no effect on the decay rate, but
produces a dramatic improvement in the chi2 of the fit. Steve has seen
essentially the same behavior.
Most of your other questions will have to await the meeting.
Regards,
Tom