Tracing Large-scale Structure with the MeerKLASS On-the-Fly Survey: Angular Clustering of Radio Sources at 816 MHz
Sourabh Paul, Suman Chatterjee, Keith Grainge, Laura Wolz, Aishrila Mazumder, Steven Cunnington, Sarvesh Mangla, Joseph J. Mohr, Mario G. Santos, Oleg Smirnov, Cyril Tasse
astro-ph.CO, astro-ph.GA
Submitted: 2026-06-21
Comments: 16 pages, 11 figures, Submitted to MNRAS
Project page: https://cartavis.github.io
License: http://creativecommons.org/licenses/by/4.0/
The gist: We present the first measurement of the angular two-point correlation function w(theta) of radio sources from the MeerKAT Large Area Synoptic Survey (MeerKLASS) UHF on-the-fly (OTF) continuum Data
Terminology
Abstract
We present the first measurement of the angular two-point correlation function w(theta) 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 about 800 deg squared within the DESI footprint. We detect a positive clustering signal over 0.02 theta 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 (0.112 theta 1.36) with a fixed-slope power law (gamma=1.8) yields A(1)=(1.434 plus or minus0.475) times10-3, corresponding to 10A=-2.843+0.124-0.175. We infer an effective large-scale bias by fitting CDM projected-matter templates w DM(theta) 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=1.998 plus or minus0.350 (AGN prior) and b eff=1.530 plus or minus0.265 (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 r 0=6.18 plus or minus1.13 and 5.59 plus or minus1.02 h-1 Mpc 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.
Sources
- Detection of the Cosmological 21 cm Signal in Auto-correlation at z ~ 1 with the Canadian Hydrogen Intensity Mapping Experiment
- The MeerKLASS On-the-Fly continuum survey: pipeline design and validation
- The DESI Experiment Part I: Science,Targeting, and Survey Design
- The MeerKLASS L-band On-the-Fly Continuum Survey: Data Release 1
- A direct detection of neutral hydrogen intensity mapping on Mpc scales at $z\approx 0.32$ and $z\approx 0.44$
- The MeerKLASS UHF On-the-Fly Continuum Survey -- Data Release I
- Measuring redshift-space distortions with future SKA surveys
- MeerKLASS: MeerKAT Large Area Synoptic Survey
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