Cr. Benn et Jv. Wall, STRUCTURE ON THE LARGEST SCALES - CONSTRAINTS FROM THE ISOTROPY OF RADIO-SOURCE COUNTS, Monthly Notices of the Royal Astronomical Society, 272(3), 1995, pp. 678-698
We show how the size of the largest scales of cellular structure in th
e Universe may be deduced from the anisotropy of the sky distribution
of extragalactic radio sources. Using a Voronoi tessellation to repres
ent the skeleton structure of the galaxy distribution, together with a
n evolving luminosity function for the mean space density of extragala
ctic radio sources, we have calculated the source-count anisotropy exp
ected as a function of tessellation scale rho(-1/3), radio-survey dept
h and survey angular diameter. Deep pencil-beam surveys of opening ang
le less than or similar to 0.1 rad provide strong limits on rho. We fi
nd, for example, that, if the density parameter Omega = 1 and rho(-1/3
) similar to 100 h(-1) Mpc, significant ( > root N) area-to-area fluct
uations are expected for counts from pencil-beam surveys slightly deep
er than the deepest yet achieved, S-1GHz < 0.1 mJy for a 0 degrees.5-d
iameter survey, S-1GHz < 3 mJy for a 5 degrees-diameter survey. The an
alysis demonstrates (a) the way in which deep radio-survey data can be
used to constrain large-scale structure, and (b) the care which must
be exercised in defining cosmologically representative samples of fain
t radio sources. We review the isotropy (or otherwise) of (1) large-ar
ea radio surveys, typically covering several steradians to similar to
1 Jy, and (2) pencil-beam radio surveys to mJy and mu Jy levels. Large
-area surveys limit rho(-1/3) less than or similar to 250 h(-1) Mpc (i
f Omega = 1). The counts from the 5C pencil-beam surveys (3000 sources
in 10 fields to S-408MHz > 10 mJy) limit rho(-1/3) less than or simil
ar to 150 h(-1) Mpc (for Omega = 1). A similar rho(-1/3) less than or
similar to 100 h(-1) Mpc can be inferred from the isotropy (or margina
l anisotropy) of deep VLA and WSRT radio surveys. We show how spectros
copy of low-redshift (z < 0.4) optical identifications from deep penci
l-beam surveys can be used to trace large-scale structure directly, an
d we illustrate this with some results from the 5C12 surveys.