2003MNRAS.339..695W

Query : 2003MNRAS.339..695W

2003MNRAS.339..695W - Mon. Not. R. Astron. Soc., 339, 695-700 (2003/March-1)

The clustering of sub-mJy radio sources in the Bootes Deep Field.

WILMAN R.J., ROETTGERING H.J.A., OVERZIER R.A. and JARVIS M.J.

Abstract (from CDS):

We measure the angular clustering of ∼2000 radio sources in the Bootes Deep Field, covering 5.3deg2 down to S1.4GHz= 0.2mJy. With reference to work by Blake & Wall, we show that the size distribution of multi-component radio galaxies dominates the overall clustering signal, and that its amplitude extrapolates smoothly from their measurements above 5 mJy. The upper limits on any true galaxy-galaxy clustering are consistent with the clustering of sub-mJy radio-loud active galatic nuclei (AGN) being effectively diluted by the more weakly clustered IRAS -type starburst galaxies. Source count models imply that the survey contains ≃400 of the latter galaxies above 0.2 mJy out to z ∼ 1-2. Measurement of their clustering must await their identification via the optical and infrared data due on this field.

Abstract Copyright: RAS

Journal keyword(s): surveys - galaxies: active - galaxies: starburst - large-scale structure of Universe

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 NAME NOAO Deep Wide Field reg 14 32 05.75 +34 16 47.5           ~ 430 0

Query : 2003MNRAS.339..695W

Basic data :
NAME NOAO Deep Wide Field -- Region defined in the Sky
Other object types: otypes_help 		reg ()
ICRS coord. (ep=J2000) : 		14 32 05.75 +34 16 47.5 [ ] D 2002AJ....123.1784D
FK4 coord. (ep=B1950 eq=1950) : 		14 29 59.98 +34 29 59.7 [ ]
Gal coord. (ep=J2000) : 		057.44983 +67.28315 [ ]
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Identifiers (4) :
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NAME NOAO Deep Wide Field NAME NDWF NAME Bootes Deep Field NAME Bootes Field

References (430 between 1850 and 2026) (Total 430)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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