تقرير
A blind Green Bank Telescope millimetre-wave survey for redshifted molecular absorption
| العنوان: | A blind Green Bank Telescope millimetre-wave survey for redshifted molecular absorption |
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| المؤلفون: | Kanekar, N., Gupta, A., Carilli, C. L., Stocke, J. T., Willett, K. W. |
| سنة النشر: | 2013 |
| المجموعة: | Astrophysics |
| مصطلحات موضوعية: | Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics |
| الوصف: | 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 ${\rm H_2}$ column densities $\gtrsim 3 \times 10^{21}$ cm$^{-2}$ in absorption at $5\sigma$ significance (using the CO-to-${\rm H_2}$ and HCO$^+$-to-${\rm H_2}$ 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 $N({\rm H_2}) \gtrsim 3 \times 10^{21}$ cm$^{-2}$. Comment: 6 pages, 2 figures. Accepted for publication in The Astrophysical Journal |
| نوع الوثيقة: | Working Paper |
| URL الوصول: | http://arxiv.org/abs/1312.3642 |
| رقم الأكسشن: | edsarx.1312.3642 |
| قاعدة البيانات: | arXiv |
| الوصف غير متاح. |