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Deblending the MIGHTEE-COSMOS survey with XID+: the resolved radio source counts to S 1.4 ≈ 5μJy

Abstract:
Deep radio continuum surveys provide fundamental constraints on galaxy evolution, but source confusion limits sensitivity to the faintest sources. We present a complete framework for producing high-fidelity deblended radio catalogues from the confused MIGHTEE maps using the probabilistic deblending framework XID+ and prior positions from deep multi-wavelength data in the COSMOS field. To assess performance, we construct MIGHTEE-like simulations based on the Tiered Radio Extragalactic Continuum Simulation radio source population, ensuring a realistic distribution of star-forming galaxies and active galactic nuclei for validation. Through these simulations, we show that prior catalogue purity is the dominant factor controlling deblending accuracy: a high-purity prior, containing only sources with a high likelihood of radio detection, recovers accurate flux densities and reproduces input source counts down to (where thermal noise). On the other hand, a complete prior overestimates the source counts due to spurious detections. Our optimal strategy combines the high-purity prior with a mask that removes sources detected above Jy. Applied to the 1.3 deg area of the MIGHTEE-COSMOS field defined by overlapping multi-wavelength data, this procedure yields a deblended catalogue of 89 562 sources. The derived 1.4 GHz source counts agree with independent P(D) analyses and indicate that we resolve the radio background to Jy. We also define a recommended high-fidelity sample of 20 757 sources, based on detection significance, flux density, and goodness-of-fit, which provides reliable flux densities for individual sources in the confusion-limited regime.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1093/mnras/stag285

Authors

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Role:
Author
ORCID:
0000-0001-8945-2879
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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author
ORCID:
0000-0001-7039-9078
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Role:
Author
ORCID:
0000-0003-3892-3073
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Role:
Author
ORCID:
0000-0003-3483-3951
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Role:
Author
ORCID:
0000-0001-9708-253X


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Funder identifier:
10.13039/100014013
Grant:
EP/X026639/1
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Funder identifier:
10.13039/501100000271
Grant:
ST/S000488/1
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Funder identifier:
10.13039/100007431
Grant:
150551
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Funder identifier:
10.13039/100006129
Grant:
UIDB/04434/2020
More from this funder
Funder identifier:
10.13039/501100004608
Grant:
BK20242115


Publisher:
Oxford University Press
Journal:
Monthly Notices of the Royal Astronomical Society More from this journal
Volume:
547
Issue:
2
Pages:
stag285
Article number:
stag285
Publication date:
2026-02-12
Acceptance date:
2026-02-05
DOI:
EISSN:
1365-2966
ISSN:
0035-8711


Language:
English
Keywords:
Pubs id:
2375765
Local pid:
pubs:2375765
Source identifiers:
3827745
Deposit date:
2026-03-06
ARK identifier:
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