Sentence examples for luminosity distribution from inspiring English sources

The redshift-total IR (TIR) luminosity distribution.

Figure 3 shows the redshift-TIR luminosity distribution.

We also present some computations of the photocenter displacement produced by extended objects having a given surface luminosity distribution, corresponding to asteroids obeying different possible scattering laws.

For example, for constructing a bivariate (FIR-FUV) galaxy luminosity distribution, he proposed H (x,y) = C N (F (x ,G (y); ρ), x,y ∈ R, where X ∼ F is far-infrared luminosity and Y ∼ G is far-ultraviolet luminosity.

Since the entropy of an image is usually used as an index that quantitatively represents the information of the luminosity distribution of the image, entropy criterion is used to analyze the performance for the complete aperture case.

Moreover, the choice of spectral model (i.e., free vs. fixed photon index) has a pronounced effect on the derived JVH distribution and, to a lesser extent, the X-ray luminosity distribution.

While a connection between more powerful winds and brighter X-ray emission is expected in intrinsic models, the scatter in X-ray luminosity at given bolometric luminosity is so far unexplained and several observational features like X-ray light curves and flaring, luminosity distributions and spectral properties are often similar to those of low-mass stars.

Here, we take advantage of the long term monitorings now available with Swift/XRT to construct for the first time the cumulative luminosity distributions of a number of SFXTs and the classical SgXB IGR J18027-2016 in the soft X-ray domain with a high sensitivity focusing X-ray telescope (0.3 10 keV).

The usage of cumulative luminosity distributions, constructed thanks to the long-term observations available through wide field hard X-ray imagers, has been recently exploited to study the averaged high energy emission (>17 keV) from supergiant fast X-ray transients (SFXTs) and classical Supergiant High Mass X-ray Binaries (SgXBs).

Moreover, the luminance distribution would split up all chromaticity bases down into certain subbases for better representing the degree of luminosity gradient of our chromaticity bases.

The bolometric luminosity versus brightness temperature distribution shows a correlation between these two components, except a few scattered objects, mostly RBLs.