Not exact matches
Thus, measuring how much gamma rays of
different energies are attenuated or weakened from blazars
at different distances from Earth indirectly gives a measurement of how many EBL
photons of
different wavelengths exist along the line of sight from blazar to Earth over those
different distances.
If we could carefully measure the number and energy (
wavelength) of all those
photons — not only
at the present time, but also back in time — we might learn important secrets about the nature and evolution of the Universe, including how similar or
different ancient galaxies were compared to the galaxies we see today.
Re 1 Timothy — the idea of an effecive emitting altitude is a useful though rough approximation — the
photons leaving for space originate over a range of altitudes
at any given frequency (
wavelength), and that range shifts over
different wavelengths.