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The difference between the angular resolution and the interval comes from an in-effective region (±5 mm) produced between stacked modules.
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It is confirmed that the rejection power against proton backgrounds is better than 4 × 10−4 in the energy range between 10 GeV and 100 GeV, the energy resolution ranges 15∼18 %, and the angular resolution is 0°.8∼1°.3.
However, the angular resolution is equivalent to a single antenna 36 km (22 miles) in diameter.
The angular resolution is 27'.3 and 12 8 FWHM at Q and W bands, respectively.
We study the effect of the angular resolution on the determination of the angular properties of the facular radiance.
The angular resolution is easily determined by the size of diffraction-plane aperture.
Various approaches to determine the angular resolution of the muon tracking detector are discussed.
In addition, the angular resolution is easily determined by the size of the diffraction plane aperture.
"Milli-arcsecond Imaging with the CHARA Interferometer" Under the best conditions, telescope diffraction limits the angular resolution for astronomical imaging.
Different concepts are studied by means of simulation concerning the angular resolution and efficiency.
In addition, using trajectory simulation, the angular resolution was numerically estimated.
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