An excess of star-forming galaxies in the fields of high-redshift QSOs
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AuthorStevens, Jason A.; Jarvis, Matt J.; Coppin, Kristen E. K.; Page, Mathew J.; Greve, Thomas R.; Carrera Troyano, Francisco Jesús; Ivison, Rob J.
© 2010 The Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, vol. 405, iss. 4, pag. 2623–2638 (2010)
The Royal Astronomical Society
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We present submillimetre (submm) and mid-infrared (MIR) imaging observations of five fields centred on quasi-stellar objects (QSOs) at 1.7< z<2.8. All five QSOs were detected previously at submm wavelengths. At 850 (450) µm, we detect 17 (11) submillimetre galaxies (SMGs) in addition to the QSOs. The total area mapped at 850 µm is ~28 arcmin2 down to rms noise levels of 1–2 mJy beam−1, depending on the field. Integral number counts are computed from the 850-µm data using the same analytical techniques adopted by ‘blank-field’ submm surveys. We find that the ‘QSO-field’ counts show a clear excess over the blank-field counts at deboosted flux densities of~2-4 mJy; at higher flux densities, the counts are consistent with the blank-field counts. Robust MIR counterparts are identified for all four submm detected QSOs and ~60 per cent of the SMGs. The MIR colours of the QSOs are similar to those of the local ultraluminous infrared galaxy (ULIRG)/active galactic nuclei (AGN) Mrk 231 if placed at 1< z<3 whilst most of the SMGs have colours very similar to those of the local ULIRG Arp 220 at 1< z<3. MIR diagnostics therefore find no strong evidence that the SMGs host buried AGN although we cannot rule out such a possibility. Taken together our results suggest that the QSOs sit in regions of the early universe which are undergoing an enhanced level of major star formation activity, and should evolve to become similarly dense regions containing massive galaxies at the present epoch. Finally, we find evidence that the level of star formation activity in individual galaxies appears to be lower around the QSOs than it is around more powerful radio-loud AGN at higher redshifts.
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