no code implementations • 18 Mar 2019 • N. Pol, M. T. Lam, M. A. McLaughlin, T. J. W. Lazio, J. M. Cordes
This approach yields an integrated intergalactic DM of $\rm DM_{\rm IGM}(z = 1) = 940^{+8200}_{-200}$ pc cm$^{-3}$, with the large errors representative of the structure in the IGM.
High Energy Astrophysical Phenomena Cosmology and Nongalactic Astrophysics
