[d2n-analysis-talk] Fwd: LHRS Scintillator Calibration Study
Brad Sawatzky
brads at jlab.org
Fri Mar 5 11:04:51 EST 2010
On Thu, 04 Mar 2010, David Flay wrote:
> On Thu, Mar 4, 2010 at 10:16 AM, Brad Sawatzky <brads at jlab.org> wrote:
>
> > I assume you're referring to the second band in the S1 time average at
> > 67ns. That is usually indicates that you're histogramming two different
> >
> > trigger types: ie. T3, T4. Double check that your trigger cut is doing
> > what you think it's doing.
>
> Yeah -- that's the band I'm talking about... These are the cuts I use:
>
> //one track from the target
> cut0 = Form("(L.tr.n==1)");
> //trigger cuts
> cut0 += Form("&&(DL.edtpl==0)&&((DL.
> evtypebits&(1<<3))==(1<<3))");
>
> I've always used this trigger cut, and I haven't seen any structure that
> looked 'odd' until now... For comparison, here's a comparison of run 20263
> (p = 1.42 GeV, 5-pass) and run 20207 (p = 1.70 GeV, 5-pass)... strange.
> Notice how the band becomes more prominent at higher p.
Vince pointed out the answer. Your cuts are working correctly -- the
second band are cosmics going through the stack 'backwards'. Note that
for good electrons (bulk of the data) t_2m-t_s1=6ns, but for the second
band: t_2m-t_s1=-6ns. At high p0 we have so few electrons that cosmics
actually compete. Interesting.
-- Brad
--
Brad Sawatzky, PhD <brads at jlab.org> -<>- Jefferson Lab / Hall C / C111
Ph: 757-269-5947 -<>- Pager: 757-584-5947 -<>- Fax: 757-269-7848
The most exciting phrase to hear in science, the one that heralds new
discoveries, is not "Eureka!" but "That's funny..." -- Isaac Asimov
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