At the 3σ level we confirmed two brightness peaks in the prominent, continent-sized bright feature on the leading side of Titan.
Signals of planetesimal rings would appear as brightness peaks in both northeast and southwest directions as well as both H- and K-bands.
We assess the statistical significance of brightness peaks by testing the null hypothesis that the observed brightness distribution is merely random noise superimposed on a smooth curve of radiation scattered by circumstellar dust.
The surface brightness peaks closer to SS433 in the high-energy band than in the low energy band, suggesting that the high energy electrons in the X-ray lobes lose energies by synchrotron emission as they travel away from SS433.
The light source has unique features such as the turntable radiation frequency, wide spectral range, high brightness and peak power, very short pulse time structure, etc.
And further, all control factors of brightness, contrast, peak detection algorithm, sampling range, and specific primary color for intensity computation are critical to the quality of range finding while using a color camera.
The flare of light reached peak brightness a month after it was detected, then slowly faded over the next 12 months.
The most common type shows a distinctive "plateau" in the light curve shortly after peak brightness where the visual luminosity stays relatively constant for several months before the decline resumes.
However, the DS has a peak brightness of 200 cd/m2, and the PSP has a peak brightness of 11 cd/m2.
The time evolution, that is, sudden appearance of emission, rapid decay, and high peak brightness, resembled that of the "mini-outburst", but the peak brightness was a factor of ~5 lower.
