Sentence examples for a maximum luminosity of from inspiring English sources

A maximum luminosity of 2×1032 cm−2s−1 and an energy resolution of about 100 keV at lower luminosity are main objectives of the HESR concept.

energy range from 2 to 5 GeV with a maximum luminosity of 1035cm−2s−1 is designed to study physics of τ lepton, charmed hadrons and e+e− annihilation with very high precision.

For the IH, a measurement of the maximum luminosity of the breakout burst could be used to differentiate between nuclear equations of state.

Super-Kamiokande(Super-K) and Jiangmen Underground Neutrino Observatory JUNO lack the mass needed to make an accurate measurement.For the IH, the time of the maximum luminosity of the breakout burst can be measured in Hyper-K to an accuracy of∼3 ms at 7 kpc, in DUNE to∼2 ms at 4 kpc, and JUNO and Super-K can measure the time of maximum luminosity to an accuracy of∼2 ms at 1 kpc.

This is done by using the plugin 'Temporal-Color Coder' in ImageJ which provides as a last step a merged image that shows pixel by pixel the frame number in which the maximum luminosity of the stacked frames is reached (Miura 2008).

For the IH, the maximum luminosity of the breakout burst can be measured at 10 kpc to accuracies of∼30% for Hyper-Kamiokande(Hyper-K) and∼60% for the Deep Underground Neutrino Experiment DUNE).

From the images of OH PLIF and CH chemiluminescence and the Rayleigh concentration measurement, it has been shown that the positions of maximum luminosity in direct photographs of lifted tribrachial flames can reasonably be located along the stoichiometric contour.

Near the time of maximum luminosity, the spectrum contains lines of intermediate-mass elements from oxygen to calcium; these are the main constituents of the outer layers of the star.

A nova reaches maximum luminosity within hours after its outburst and may shine intensely for several days or occasionally for a few weeks, after which it slowly returns to its former level of luminosity.

Flame areas defined by the loci of maximum luminosity and by schlieren contours were recorded, so that saturation current densities, CH∗ and C∗2 emission per unit flame area, as well as burning velocities could be deduced.

The peak luminosity of the light curve is extremely consistent across normal Type Ia supernovae, having a maximum absolute magnitude of about −19.3.