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A 22-GHz search for molecular absorption at z similar to 3 with the upgraded ATCA
List of Titles
A 22-GHz search for molecular absorption at z similar to 3 with the upgraded ATCA
Please use this identifier to cite or link to this item: http://hdl.handle.net/1959.3/42702
- Title
- A 22-GHz search for molecular absorption at z similar to 3 with the upgraded ATCA
- Author(s)
- Curran, Stephen J.; Murphy, Michael T.; Webb, J. K.; Pihlstrom, Ylva M.
- Abstract
- We report a λ. ≲ 1 cm search for rotational molecular absorption towards quasars, now possible with the upgraded Australia Telescope Compact Array (ATCA). The targets were PKS 0201+113, PKS 0336-017 and Q 0537-286, where known damped Lyman-alpha absorption systems (DLAs) could cause redshifted molecular absorption in the 12-mm band of the telescope. We place 3σ upper limits on any HCO+ 0 → 1 absorption features of <30 mJy per 3.4 km s-1 channel. The non-detections could be attributed to the inherent low metallicities in DLAs leading to generally low H2, and thus HCO+, column densities. In general, the detection of molecular rotational transitions in DLAs could be further hindered by a lower than expected CO-to-H2 conversion ratio, whether due either to photoionization of carbon or to its relative under-abundance at high redshift.
- Publication type
- Journal article
- Source
- Monthly Notices of the Royal Astronomical Society, Vol. 340, no. 1 (Mar 2003), pp. 139-142
- Publication year
- 2003
- Keyword(s)
- Alpha system; CO; Continuum galaxies; Early universe; Galaxies; Gravitational lens; High-redshift; Hydrogen; ISM; Lines; PKS1830-211; Quasars; Quasars absorption lines; Radio
- Publisher
- Wiley-Blackwell Publishing
- ISSN
- 0035-8711
- Publisher URL
- http://dx.doi.org/10.1046/j.1365-8711.2003.06273.x
- Copyright
- Copyright © 2003 the authors. Journal compilation copyright © 2003 Royal Astronomical Society. The accepted manuscript of the paper is reproduced here in accordance with the copyright policy of the publisher. The definitive publication is available at www.interscience.wiley.com.
- Full text

- Peer reviewed


