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Figure 2 Relationship between the integrated luminosity per one cell and vertical distance from the NP source.

Figure 2 illustrates the relationship between the integrated luminosity per one cell and vertical distance from the cell holder to the suspension surface (see relationship between the integrated luminosity per one cell and horizontal distance from the NP source in Figure S1 in Additional file 1).

Until the end of 2006 the integrated luminosity collected by the ZEUS experiment is 350pb−1, most of it with good vertex detector data (99%).

Associated with the increase in instantaneous luminosity is a rise of the target integrated luminosity from 730 to about 3000 fb−1 which directly translates into significantly higher radiation damage.

In order to increase the discovery potential of the experiments at the Large Hadron Collider, the high-luminosity phase of the LHC (HL-LHC) is expected to deliver a total of 3000 fb−1 integrated luminosity.

Dependence of the integrated luminosity per one cell on the vertical distance between the cell holder and the suspension surface for two cases: open and confined air.

Early observations of hydroxyl megamasers indicated a correlation between the isotropic hydroxyl luminosity and far infrared luminosity, with LOH \propto LFIR2.

Black, red and blue lines in the panel (b) indicate the whole luminosity, Gaussian fitting curves for L1 and L2, and difference between the whole luminosity and that of L1 and L2, respectively.

The observed relationship between the hydroxyl luminosity and far infrared luminosity suggests that hydroxyl megamasers in such galaxies may be tens to hundreds of times more luminous than observed hydroxyl megamasers.

In contrast, at IR, the luminosity related to the SF activity is the one integrated over a whole range of IR wavelengths (λ = 8 1000 μ m), L tir, where the subscript TIR stands for the total IR.

In principle, the density distribution can be calculated by integrating the stellar luminosity function.