The evolution of neutral hydrogen over the past 11 Gyr via HI 21 cm absorption

Abstract

We present the results of a blind search for intervening HI 21 cm absorption toward 260 radio sources in the redshift range 0<z<2.74 with the Green Bank Telescope. The survey has the sensitivity to detect sub-damped Lyman-alpha (DLA) systems for HI spin temperatures $T_s/f$ = 100 K, and despite the successful re-detection of ten known 21 cm absorbers in the sample, we detect no new absorption lines in the full survey. Sources detected in 21 cm absorption were also searched for hydroxyl (OH) 18 cm absorption and we re-detect 1667 MHz OH absorption toward PKS 1830-211. We searched for intervening HI 21 cm absorption along the line of sight in each source achieving a total redshift coverage of $\Delta z$ = 88.64 (comoving absorption path of $\Delta X$ = 159.5) after removing regions affected by radio frequency interference. We compute a 95% confidence upper limit on the column density frequency distribution $f(N_{\mathrm{HI}})$ and set a statistical constraint on the spin temperature $T_s$ in the range 100-1000 K, consistent with prior redshifted optical DLA surveys and HI 21 cm emission observations at the same redshifts. We infer a value for the cosmological mass density of neutral gas, ${\Omega }_{\mathrm{HI}}$. Through comparison with prior ${\Omega }_{\mathrm{HI}}$ measurements, we place a statistical constraint on the mean spin temperature of $T_s/f$ = 175 K. Our derived ${\Omega }_{\text{HI}}$ values support a relative mild evolution in ${\Omega }_{\text{HI}}$ over the last 11 Gyr and are consistent with other methods that measure ${\Omega }_{\text{HI}}$.

arXiv comment21 pages, 8 figures, 4 tables, accepted for publication in MNRAS

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