Table 1.
Best-fitting positions of the point sources and the negative CMB distortion fitted to the continuum NOEMA uv table.
| RA | Dec | Source | uv_fit function | LSB flux | USB flux | FWHM |
|---|---|---|---|---|---|---|
| J2000 | J2000 | [μJy] | [μJy] | [arcsec] | ||
| 12:26:58.12 (0.21) | +33:32:48.7 (0.3) | PS9 | point | 72.7 ± 9.5 | 64.5 ± 6.7 | |
| 12:27:00.09 (0.30) | +33:32:34.5 (1.0) | PS260-S | point | 80.8 ± 16.4 | 121.8 ± 14.9 | |
| 12:27:00.02 (0.60) | +33:32:43.7 (0.8) | PS260-N | point | 51.0 ± 15.2 | 40.0 ± 11.5 | |
| 12:26:57.97 (0.50) | +33:32:45.9 (0.6) | cluster tSZ | circular Gaussian | 32.7 ± 2.1 |
Notes. Positional uncertainties are given in brackets. We indicate the function used to model each of the sources, the primary-beam-corrected flux of the point sources measured from the LSB (∼74 GHz) and USB (∼90 GHz) data, and the best-fitting size of the Gaussian function we used to describe the cluster signal (not corrected for the primary beam; see Sect. 4.1 for the fitted negative amplitude of the tSZ).
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