Telescope Array

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Telescope Array Collaboration
the Telescope Arrayis not an array of telescopes…S=3 m2
Page 1 and 2: G.T. Zatsepin memorial readings,Mos
Page 3: Ultra-high-energy cosmic rays:exper
Page 7 and 8: A typical Surface-Detector event200
Page 9 and 10: TA fluorescent detector 1:Middle Dr
Page 11 and 12: A typical fluorescent-detector even
Page 13 and 14: Example of a TRIPLE STEREO HYBRID e
Page 15 and 16: Energy estimation:SD and FD see dif
Page 17 and 18: SD energy estimation: traditional (
Page 19 and 20: SD energy estimation: TAFULL MONTE-
Page 21 and 22: SD simulations: summary
Page 23 and 24: SD simulations: no-thinning
Page 25 and 26: SD simulations: dethinning
Page 27 and 28: SD energy estimation: TA
Page 29 and 30: SD data/MC comparison
Page 35 and 36: SD vs. FDSD energy: CORSIKAQGSJET-I
Page 37 and 38: SD vs. FD energies:approaches to th
Page 39 and 40: Telescope Array: FD calibrationELS
Page 41 and 42: RESULTS: COSMIC-RAY ENERGY SPECTRUM
Page 43 and 44: TA sees the GZK-like suppressiona
Page 45 and 46: Other experiments see the GZK-like
Page 47 and 48: TA spectra (different techniques)
Page 49 and 50: RESULTS: PRIMARY COMPOSITION
Page 51 and 52: Primary composition: protons or hea
Page 53 and 54: Primary composition: protons or hea
Page 55 and 56:
Anisotropy: data
Page 57 and 58:
Auger: AGN correlations weakened
Page 59 and 60:
TA autocorrelation
Page 61 and 62:
TA correlations with the large-scal
Page 63 and 64:
RESULTS: SEARCH for PHOTONS
Page 65 and 66:
TA photon search
Page 67 and 68:
TA future plans…
Page 69 and 70:
CONCLUSIONS• PRIMARY ENERGIES:‣
Page 71 and 72:
stereo: protons or nuclei?a
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