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CO observations of high-z radio galaxies MRC 2104−242 and MRC 0943−242: spectral-line performance of the Compact Array Broadband Backend


Emonts, BHC and Norris, RP and Feain, I and Miley, G and Sadler, EM and Villar-Martin, M and Mao, MY and Oosterloo, TA and Ekers, RD and Stevens, JB and Wieringa, MH and Coppin, KEK and Tadhunter, CN, CO observations of high-z radio galaxies MRC 2104−242 and MRC 0943−242: spectral-line performance of the Compact Array Broadband Backend, Monthly Notices of the Royal Astronomical Society, 415, (1) pp. 655-664. ISSN 1365-2966 (2011) [Refereed Article]

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DOI: doi:10.1111/j.1365-2966.2011.18737.x


We present the first 7-mm observations of two high-redshift, Lyα-bright radio galaxies (MRC 2104−242 and MRC 0943−242) performed with the 2 × 2 GHz instantaneous bandwidth of the Compact Array Broadband Backend (CABB) at the Australia Telescope Compact Array (ATCA). The aim was to search for 12CO(1−0) emission in these systems and test the millimetre capabilities of CABB for performing spectral line observations at high redshifts. We show that the stable band and enhanced velocity coverage of CABB, combined with hybrid array configurations, provide the ATCA with excellent 7-mm capabilities that allow reliable searches for the ground transition of CO at high redshifts. In this paper we explicitly discuss the calibration procedures used to reach our results. We set a firm upper limit to the mass of molecular gas in MRC 2104−242 (z= 2.5) of MH2 2 × 1010 (αx/0.8)M. For MRC 0943−242 (z= 2.9) we derive an upper limit of MH2 2 × 1010 (αx/0.8)M. We also find a tentative 3σ CO detection in the outer part of the giant Lyα halo that surrounds MRC 0943−242. The 30-33 GHz radio continuum of MRC 2104−242 and MRC 0943−242 is reliably detected. Both radio sources show a spectral index of α ≈ −1.5 between 1.4 and 30 GHz, with no evidence for spectral curvature within this range of frequencies.

Item Details

Item Type:Refereed Article
Keywords:techniques: interferometric; galaxies: active; galaxies: high-redshift; galaxies: individual: MRC 0943−242; galaxies: individual: MRC 2104−242; galaxies: ISM
Research Division:Physical Sciences
Research Group:Astronomical sciences
Research Field:Cosmology and extragalactic astronomy
Objective Division:Expanding Knowledge
Objective Group:Expanding knowledge
Objective Field:Expanding knowledge in the physical sciences
UTAS Author:Mao, MY (Miss Minnie Mao)
ID Code:75122
Year Published:2011
Web of Science® Times Cited:19
Deposited By:Mathematics and Physics
Deposited On:2012-01-11
Last Modified:2014-02-03

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