The thermal history of the intergalactic medium down to redshift z=1.5: a new curvature measurement

Abstract

According to the photo-heating model of the intergalactic medium (IGM), He II reionization is expected to affect its thermal evolution. Evidence for additional energy injection into the IGM has been found at $3\lesssim z\lesssim4$, though the evidence for the subsequent fall-off below $z\sim2.8$ is weaker and depends on the slope of the temperature--density relation, $γ$. Here we present, for the first time, an extension of the IGM temperature measurements down to the atmospheric cut-off of the H I Lyman-$α$ forest at $z\simeq1.5$. Applying the curvature method on a sample of 60 UVES spectra we investigated the thermal history of the IGM at $z<3$ with precision comparable to the higher redshift results. We find that the temperature of the cosmic gas traced by the Ly-$α$ forest [$T(\barΔ)]$ increases for increasing overdensity from $T(\barΔ)\sim 22670$ K to 33740 K in the redshift range $z\sim2.8-1.6$. Under the assumption of two reasonable values for $γ$, the temperature at the mean density ($T_{0}$) shows a tendency to flatten at $z\lesssim 2.8$. In the case of $γ\sim1.5$, our results are consistent with previous ones which indicate a falling $T_{0}$ for redshifts $z\lesssim2.8$. Finally, our $T(\barΔ)$ values show reasonable agreement with moderate blazar heating models.