Niebla is an open-source phenomenological code for computing the EBL spectrum via stellar population evolution and multiple dust re-emission models, with three fitted versions and a blazar simulation demonstrating infrared sensitivity.
For example, poly- cyclic aromatic hydrocarbon and very small grains are heated in galaxies toT∼ O(100 K), and therefore emit in the mid infrared (MIR) [13, 20]
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Niebla: an open-source code for modeling the extragalactic background light
Niebla is an open-source phenomenological code for computing the EBL spectrum via stellar population evolution and multiple dust re-emission models, with three fitted versions and a blazar simulation demonstrating infrared sensitivity.