3.4 micron Background Induced MCMC Prior Chain

Extragalactic background light (EBL) at 3.4 microns from galaxies as predicted using the mean spectral energy distribution (SED) of galaxies measured in Lake and Wright (2016, DOI: 10.21105/astro.1603.0729) and a Markov chain Monte Carlo (MCMC) prior chain for the Luminosity function (LF) from Lake et al. (2018b). The LF prior chain is unpublished, because the prior is analytically computable. The first column is the background from galaxies at redshifts closer than z=1 and the second column is the prediction from the same parameters closer than z=5, all in kilo-Janskies per steradian. The files are gzipped ( http://www.gzip.org/ ) IPAC tables ( http://irsa.ipac.caltech.edu/applications/DDGEN/Doc/ipac_tbl.html ). A full description of how these files were produced is in Lake et al. (2019, in preparation).