Tracing Large-scale Structure with the MeerKLASS On-the-Fly Survey: Angular Clustering of Radio Sources at 816 MHz
Abstract
We present the first measurement of the angular two-point correlation function \(w(θ)\) of radio sources from the MeerKAT Large Area Synoptic Survey (MeerKLASS) UHF on-the-fly (OTF) continuum Data Release~1. DR1 provides interferometric Stokes-\(I\) imaging at a reference frequency of 816\,MHz over \( 800~deg2\) within the DESI footprint. We detect a positive clustering signal over \(0.02 θ 10\). The measurement is stable to reasonable variations of the depth mask and flux threshold on intermediate and large scales. Modelling the intermediate-scale signal (\(0.112θ 1.36\)) with a fixed-slope power law (\(γ=1.8\)) yields \(A(1)=(1.4340.475)×10-3\), corresponding to \(10A=-2.843+0.124-0.175\). We infer an effective large-scale bias by fitting \(Λ\)CDM projected-matter templates \(w DM(θ)\) computed with CAMB and Limber projection, including an integral-constraint correction evaluated from random--random weights. Using two bracketing T-RECS redshift-distribution priors, we obtain \(b eff=1.9980.350\) (AGN prior) and \(b eff=1.5300.265\) (TOTAL prior), demonstrating that the dominant modelling uncertainty arises from \(N(z)\). As a derived summary we Limber-invert the power-law amplitude to obtain \(r0=6.181.13\) and \(5.591.02~h-1Mpc\) for the AGN and TOTAL priors, respectively. These results establish MeerKLASS UHF DR1 as a new wide-area, intermediate-frequency dataset for radio-continuum clustering. As MeerKLASS expands and overlapping optical/IR spectroscopy provides improved redshift calibration, future releases will enable population-split clustering and bias evolution measurements with substantially reduced modelling uncertainty.
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