Canadian astronomer Ren?Racine assumed the use of the globular cluster luminosity function ( GCLF ) would lead to a better approximation.
22.
The luminosity function that describes the perceived brightnesses of different wavelengths is thus roughly analogous to the spectral sensitivity of M cones.
23.
For a light source with mixed wavelengths, the number of lumens per watt can be calculated by means of the luminosity function.
24.
In practice, the integral is replaced by a sum over discrete wavelengths for which tabulated values of the luminosity function are available.
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The small excess fractional value comes from the slight mismatch between the definition of the lumen and the peak of the luminosity function.
26.
This shifts the peak of the luminosity function from the faint end to a brighter luminosity and changes the shape of the luminosity function.
27.
This shifts the peak of the luminosity function from the faint end to a brighter luminosity and changes the shape of the luminosity function.
28.
Having very overdense or underdense regions of objects will cause an inferred change in our average absolute magnitude and luminosity function, according with the structure.
29.
We find that the luminosity functions and total stellar mass densities are in agreement with observations when plausible assumptions about reddening at z ~ 6 are made.
30.
Note that the term " function " is slightly misleading, and the luminosity function might better be described as a luminosity " distribution ".
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