Deep radio imaging of the SCUBA 8-mJy survey fields: sub-mm source identifications and redshift distribution

Details Deep radio imaging of the SCUBA 8-mJy survey fields: sub-mm source identifications and redshift distribution Deep radio imaging of the SCUBA 8-mJy survey fields: sub-mm source identifications and redshift distribution

2002-06-25

arxiv.org/abs/astro-ph/0206432v2

Mon.Not.Roy.Astron.Soc. 337 (2002) 1

Astronomy and Astrophysics

Astrophysics

In press at MNRAS. Extra IR imaging now included. 27 pages; 14 figures, mostly colour. The resolution of Figs 1 and 2 has been

Scientific paper

10.1046/j.1365-8711.2002.05900.x

The SCUBA 8-mJy survey is the largest submm extragalactic mapping survey undertaken to date, centred on the Lockman Hole and ELAIS N2 regions. Here, we present new 1.4-GHz imaging of the depth and resolution necessary to reliably identify radio counterparts for 18 of 30 submm sources. Armed with this greatly improved positional information, we present and analyse new optical, near-IR and XMM-Newton X-ray imaging to identify optical/IR host galaxies to half of the submm-selected sources in those fields. As many as 15% of the submm sources detected at 1.4 GHz are resolved by the 1.4'' beam and a further 25% have more than one radio counterpart, suggesting that radio and submm emission arise from extended starbursts and that interactions are common. We note that less than a quarter of the submm-selected sample would have been recovered by targeting optically faint radio sources, underlining the selective nature of such surveys. At least 60% of the radio-confirmed optical/IR host galaxies appear to be morphologically distorted; many are composite systems - red galaxies with relatively blue companions; just over half are found to be very red or extremely red; contrary to popular belief, most are sufficiently bright to be tackled with spectrographs on 8-m telescopes. We estimate the median redshift of the S(850um) ~ 8 mJy submm galaxy population: if the radio/far-IR correlation holds at high redshift, and our sample is unbiased, we derive a conservative median z >= 2.0, or >= 2.4 using spectral templates more representative of known submm galaxies [abridged].

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