Class URB

Class Documentation

class URB

Extragalactic background light model from Protheroe & Biermann 1996.

Extragalactic background light model by Nitu et al.

Extragalactic background light model based on ARCADE2 observations, by Fixsen et al. Note that this model does not cover the same energy range as other URB models. Here, only ~10 MHz - 10 GHz is considered. Therefore, it only makes sense to use this model in very specific studies.

Source info: DOI:10.1016/S0927-6505(96)00041-2 https://www.sciencedirect.com/science/article/abs/pii/S0927650596000412

Source info: DOI:10.1088/0004-637X/734/1/5 https://iopscience.iop.org/article/10.1088/0004-637X/734/1/5

Source info: DOI:10.1016/j.astropartphys.2020.102532 https://www.sciencedirect.com/science/article/pii/S0927650520301043?