So, astrophysicists developed an ingenious work - around method: measuring the EBL indirectly through measuring the attenuation of — that is, the absorption of — very high energy gamma rays from
distant blazars.
Observations of blazars by NASA's Fermi Gamma Ray Telescope spacecraft for the first time detected that gamma rays from
distant blazars are indeed attenuated more than gamma rays from nearby blazars, a result announced on November 30, 2012, in a paper published in Science, as theoretically predicted.
The attached figure illustrates how energetic gamma rays (dashed lines) from
a distant blazar strike photons of extragalactic background light (wavy lines) and produce pairs of electrons and positrons.
Not exact matches
Looking at a
distant galaxy: the radio chart (left) shows the image of the
blazar PKS 1830 - 211 distorted by the gravitational lens effect.