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First Look at AN for p-Al (Day160)
We have downloaded and analyzed about 5 to 6 hours of data from Day160 (first p-Al data).
The runs are:
The prescale factors are seen on his pages www.star.bnl.gov/protected/spin/dilks/trgmon15pAu/200/prescale_canv_zoomed_pAl.png
We see that these are in the early fill region where prescaling is agressive.
The reconstruction of pions was done with an "all ones" set of calibration corrections. I am in the process of generating better gain correction factors for our new voltage settings.
As I have before, I show the distribution of pi0 events as a function of pT for each of the 9 triggers (Bsum small(x3), Bsum large(x3), JetPatch(x3)).
drupal.star.bnl.gov/STAR/system/files/callptDay160_6hrs.pdf
For comparison, this is the trigger distribution at the start of pAu (Day126)
drupal.star.bnl.gov/STAR/system/files/Save128129.pdf
I also include a corresponding trigger analysis for pi0 events from Day070 at the beginning of pp running,
drupal.star.bnl.gov/STAR/system/files/callpt_0.pdf I should note that there were hardware fixes after Day70.
Based on comparing rates for reconstructed forward pion production, this 5 to 6 hours of p-Al data looks like it is equivalent to between 0.7 and 1 pb^(-1) of pp data.
On figure the right, the asymmetries are shown for pions of energy 25<E<35 GeV as a function of pT. The p-Al data points are plotted with "star" markers and points are joined by solid lines. For comparison to a 29 pb^(-1) pp data set, the pp data are plotted with circles as markers and joined with dashed lines.
For the p-Aluminum AN point at pT=3.2 GeV, the Cos(Phi) distribution is shown (upper left). Remember the slope of the Cos(Phi) distribution is proportional to AN. The p-Al mass distribution for this pT=3.2 GeV point is shown in the lower left.
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