Ultra steep spectrum radio sources in the lockman hole: Servs identifications and redshift distribution at the faintest radio fluXES
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Ultra steep spectrum (USS) radio sources have been successfully used to select powerful radio sources at high redshifts (z ~>2). Typically restricted to large-sky surveys and relatively bright radio flux densities, it has gradually become possible to extend the USS search to sub-mJy levels, thanks to the recent appearance of sensitive low-frequency radio facilities. Here a first detailed analysis of the nature of the faintest USS sources is presented. By using Giant Metrewave Radio Telescope and Very Large Array radio observations of the Lockman Hole at 610 MHz and 1.4 GHz, a sample of 58 USS sources, with 610 MHz integrated fluxes above 100 μJy, is assembled. Deep infrared data at 3.6 and 4.5 μm from the Spitzer Extragalactic Representative Volume Survey (SERVS) are used to reliably identify counterparts for 48 (83%) of these sources, showing an average total magnitude of [3.6]AB = 19.8 mag. Spectroscopic redshifts for 14 USS sources, together with photometric redshift estimates, improved by the use of the deep SERVS data, for a further 19 objects, show redshifts ranging from z = 0.1 to z = 2.8, peaking at z ~ 0.6 and tailing off at high redshifts. The remaining 25 USS sources, with no redshift estimate, include the faintest [3.6] magnitudes, with 10 sources undetected at 3.6 and 4.5 μm (typically [3.6] ~>22-23 mag from local measurements), which suggests the likely existence of higher redshifts among the sub-mJy USS population. The comparison with the Square Kilometre Array Design Studies Simulated Skies models indicates that Fanaroff-Riley type I radio sources and radio-quiet active galactic nuclei may constitute the bulk of the faintest USS population, and raises the possibility that the high efficiency of the USS technique for the selection of high-redshift sources remains even at the sub-mJy level.
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Ultra steep spectrum radio sources in the Lockman Hole: SERVS identifications and redshift distribution at the faintest radio fluxesBizzocchi, L.; Afonso, J.; Ibar, E.; Grossi, M.; Simpson, C.; Chapman, S.; Jarvis, M.; Rottgering, H.; Norris, R.; Dunlop, J.; Ivison, R.; Messias, H.; Pforr, J.; Vaccari, M.; Seymour, Nick; Best, P.; Gonz, E.; Farrah, D.; Huang, J.; Lacy, M.; Marastron, C.; Marchetti, L.; Mauduit, J.; Oliver, S.; Rigopoulou, D.; Stanford, S.; Surace, J.; Zeimann, G. (2012)Ultra Steep Spectrum (USS) radio sources have been successfully used to select powerful radio sources at high redshifts (z > 2). Typically restricted to large-sky surveys and relatively bright radio flux densities, it has ...
Coppejans, R.; van Velzen, S.; Intema, Hubertus; Müller, C.; Frey, S.; Coppejans, D.; Cseh, D.; Williams, W.; Falcke, H.; Körding, E.; Orrú, E.; Paragi, Z.; Gabányi, K. (2017)High-redshift quasars are important to study galaxy and active galactic nuclei evolution, test cosmological models and study supermassive black hole growth. Optical searches for high-redshift sources have been very ...
Wu, J.; Brandt, W.; Anderson, S.; Diamond-Stanic, A.; Hall, P.; Plotkin, Richard; Schneider, D.; Shemmer, O. (2012)We report on the X-ray and multiwavelength properties of 11 radio-quiet quasars with weak or no emission lines identified by the Sloan Digital Sky Survey (SDSS) with redshift z = 0.4-2.5. Our sample was selected from the ...