cls upper limits造句
造句與例句
手機(jī)版
- The subsequent decay of axions to gamma rays allows constraints on the axion mass to be placed from observations of neutron stars in gamma-rays using the Fermi LAT . From an analysis of 4 neutron stars, Berenji et al . obtained a 95 % CL upper limit on the axion mass of 0.079 eV.
- Based on 11 months of data from Fermi-LAT, 95 % CL upper limits on the size of extra dimensions R from each source are obtained, as well as 95 % CL lower limits on the ( n + 4 )-dimensional Planck scale M _ D . In addition, the limits from all of the analyzed NSs have been combined statistically using two likelihood-based methods.
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