POINT-AGAPE pixel lensing survey of M 31
Astronomy & Astrophysics EDP Sciences 443:3 (2005) 911-928
Precision measurements of the timelike electromagnetic form factors of pion, kaon, and proton.
Physical review letters 95:26 (2005) 261803
Abstract:
Using 20.7 pb(-1) of e(+)e(-) annihilation data taken at sq.rt(r) = 3.671 GeV with the CLEO-c detector, precision measurements of the electromagnetic form factors of the charged pion, charged kaon, and proton have been made for timelike momentum transfer of |Q(2)| = 13.48 GeV(2) by the reaction e(+)e(-) --> h(+)h(-). The measurements are the first ever with identified pions and kaons of |Q(2)| > 4 GeV(2), with the results F(13.48 GeV(2)) = 0.075 +/- 0.008(stat) +/- 0.005(syst) and F(K)(13.48 GeV(2)) = 0.063 +/- 0.004(stat) +/- 0.001(syst). The result for the proton, assuming G(p)(E) = G(p)(M), is G(p)(M)(13.48 GeV(2)) = 0.014 +/- 0.002(stat) +/- 0.001(syst), which is in agreement with earlier results.Search for Bs0â†Î+Î- and Bd0â†Î +Î- Decays in pp Collisions with CDF II
Physical Review Letters 95:22 (2005)
Abstract:
We report on a search for Bs0â†Î+Î- and Bd0â†Î+Î- decays in ppÂcollisions at s=1.96TeV using 364â€â€pb-1 of data collected by the CDF II detector at the Fermilab Tevatron Collider. After applying all selection requirements, we observe no candidates inside the Bs0 or Bd0 mass windows. The resulting upper limits on the branching fractions are B(Bs0↠Î+Î-)<1.5Ã-10-7 and B(Bd0â†Î+Î-) <3.9Ã-10-8 at 90% confidence level. © 2005 The American Physical Society.The Growth, Polarization, and Motion of the Radio Afterglow from the Giant Flare from SGR 1806–20
The Astrophysical Journal American Astronomical Society 634:1 (2005) l93-l96
Structure in the radio counterpart to the 2004 Dec 27 giant flare from SGR 1806-20
(2005)