Alexandreas First Time

Wang et al., Survey of Northern Sky for TeV Point Sources

Many of the blazars exhibit time variability, while the pulsars seem to be ..1999, A&A, 342, 69 First citation in article | NASA ADS; Alexandreas.

Search for Continuous Emission from Cygnus X-3

On the zenith angle pointed out by Alexandreas et al.[46] of a function of spatial coordinates and a function of time First the functional.

First astronomical results from the ARGO-YBJ detector

Time structure of the shower front in a detailed way. The RPC time resolution of about 1 ns and the detector [6] D. E. Alexandreas, D. Berley, S. Biller.

My talk at the XXIV ICRC (1995)

Of an all sky search for short time emission above twenty TeV with the HEGRA detector. was recorded during the first year of operation of AIROBICC.

An All-Sky Search for Steady VHE Gamma-Ray Sources

Milagrito was the first large-aperture gamma-ray detector with sensitivity to background estimation method has been discussed in Alexandreas (1993).

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Phys. Rev. Lett. 64, 2973 (1990): Alexandreas et al. - Study of

No significant signal was observed by the CYGNUS experiment over time scales Sa Cygnus X-3 was first discovered as a y-ray source at energies above -1 .

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Search for sources of cosmic rays in the region of the knee: Part II

Your browser may not have a PDF reader available. Google recommends visiting our text version of this document.First, for every extensive air shower with an arrival. direction (θ, ϕ) in the local coordinate system, the. arrival time t' of another shower is chosen in.

Search for Short Duration Bursts of TeV Gamma Rays with the Milagrito

To our knowledge this is the first such search in this energy regime. In correct local apparent sidereal time. bin should be larger (Alexandreas 1993).

An All-Sky Search for Steady VHE Gamma-Ray Sources

File Format: PDF/Adobe Acrobat - View as HTMLYour browser may not have a PDF reader available. Google recommends visiting our text version of this document.the first air-shower array with sensitivity to gamma rays below 1 TeV. Because Milagrito had a large field. of view (>1 sr) and operated all the time.

ArXiv:astro-ph/0610944 v1 31 Oct 2006

File Format: PDF/Adobe Acrobat - View as HTMLYour browser may not have a PDF reader available. Google recommends visiting our text version of this document.on the method of Alexandreas et al. [4]. This method utilizes the full amount First, for every shower with an arrival direction (θ, ϕ) an arrival time t.

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UltraHigh-Energy Gamma-Ray Emission

Due to an energy-dependent mean escape time from the Galaxy, the observed ..Alexandreas, D. E., et al. 1991, Phys. Rev. D, 43, 1735 First citation in.

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Phys. Rev. D 43, 1735 (1991): Alexandreas et al. - Observation of

This is the first observation of such shadowing. .Both the parti- cle count and the relative arrival time are measured by each detector.

University of Chicago Press - Significance Tests and Background

Top, Standard time‐swapping implementation is used (Alexandreas et al. 1993); bottom, exclusion method .First citation in article, CrossRef, NASA ADS.

Study of the Shadow of the Moon and Sun with VHE Cosmic Rays

File Format: PDF/Adobe Acrobat - View as HTMLYour browser may not have a PDF reader available. Google recommends visiting our text version of this document.background was calculated using the time-sloshing method. (Alexandreas etal.,1993). The data and background maps. were then smoothed with square bins.