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Table 3

Statistical results obtained from applying CoSch-CLEAN, MS-CLEAN, and CS to all the datasets A, B, and C.

Point source (Sect. 3.2.1) CoSch-CLEAN CS

Relative flux density error high S/N, low S/N 3%–23% 3%–25%
Effective angular resolution () 3.18′ × 2.55′ 1.55′ × 1.09′
Astrometric error () <2 <1

Grid of point sources (Sect. 3.2.2) CoSch-CLEAN CS

Relative flux density error (Jy) Fig. 4
Residuals: Std-dev in I (Jy/beam) 1.7 3.6
W50 (Sect. 3.3.1) CoSch-CLEAN MS-CLEAN CS

Effective angular resolution () 2.8′ × 2.4′ 2.8′ × 3.3′ ~ 1′ × ~ 1′
Reconstructed: total flux density in S (Jy) 229.19 229.41 229.72
Reconstructed: peak flux density in I (Jy/beam) 0.72 0.96 0.79
Residuals: rms in S (Jy/beam) 4.6 × 10-4 2.71 × 10-2 3.1 × 10-4
Residuals: Std-dev in I (Jy/beam) 4.1 × 10-4 1.3 × 10-2 3.2 × 10-4
Error: mean square error in I (Jy/pixel) 8.9 × 10-5 1.0 × 10-4 4.8 × 10-5
DR 1729:1 75:1 2446:1

Cygnus A (Sect. 3.3.2) CoSch-CLEAN MS-CLEAN CS

Effective angular resolution () 6.1′′ × 5.0′′ 6.1′′ × 5.0′′ 2.8′′ × 2.8′′
Reconstructed: total flux density in S (Jy) 10 576 10 560 10 506
Reconstructed: Peak flux density in I (Jy/beam) 315.5 309.3 465.7
Residuals: rms in S (Jy/beam) 0.37 0.35 0.09
Residuals: Std-dev in I (Jy/beam) 0.17 0.19 0.05
DR 1799:1 1619:1 8392:1

Notes. The statistics are defined in the text and appear when applicable. I means that the quantity has been evaluated on the entire image, S in a defined region of the image (typically around the source).

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