A blind Green Bank Telescope millimetre-wave survey for redshifted molecular absorption

Abstract

We present the methodology for ``blind'' millimetre-wave surveys for redshifted molecular absorption in the CO/HCO${}^{+}$ rotational lines. The frequency range $30-50$ GHz appears optimal for such surveys, providing sensitivity to absorbers at $z\gtrsim 0.85$. It is critical that the survey is ``blind'', i.e. based on a radio-selected sample, including sources without known redshifts. We also report results from the first large survey of this kind, using the Q-band receiver on the Green Bank Telescope (GBT) to search for molecular absorption towards 36 sources, 3 without known redshifts, over the frequency range $39.6-49.5$ GHz. The GBT survey has a total redshift path of $\Delta z\approx 24$, mostly at $0.81<z<1.91$, and a sensitivity sufficient to detect equivalent ${\mathrm{H}}_2$ column densities $\gtrsim 3\times 10^{21}$ cm${}^{-2}$ in absorption at $5\sigma$ significance (using the CO-to-${\mathrm{H}}_2$ and HCO${}^{+}$-to-${\mathrm{H}}_2$ conversion factors of the Milky Way). The survey yielded no confirmed detections of molecular absorption, yielding the $2\sigma$ upper limit $n(z=1.2)<0.15$ on the redshift number density of molecular gas at column densities $N({\mathrm{H}}_2)\gtrsim 3\times 10^{21}$ cm${}^{-2}$.

arXiv comment6 pages, 2 figures. Accepted for publication in The Astrophysical Journal