4.7 Article

A 22-GHz search for molecular absorption at z∼3 with the upgraded ATCA

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 340, Issue 1, Pages 139-142

Publisher

BLACKWELL PUBLISHING LTD
DOI: 10.1046/j.1365-8711.2003.06273.x

Keywords

galaxies : ISM; quasars : absorption lines; early Universe; radio continuum : galaxies

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We report a lambdagreater than or similar to1 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 3sigma 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 H-2 , 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-H-2 conversion ratio, whether due either to photoionization of carbon or to its relative under-abundance at high redshift.

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