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Planck 2013 results
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Table 1

PCCS characteristics.

Channel
30 44 70 100 143 217 353 545 857
Frequency [GHz] ...................... 28.4 44.1 70.4 100.0 143.0 217.0 353.0 545.0 857.0
Wavelength, λ [μm] ...................... 10 561 6807 4260 3000 2098 1382 850 550 350
Beam FWHMa [arcmin] ...................... 32.38 27.10 13.30 9.65 7.25 4.99 4.82 4.68 4.33
Pixel size [arcmin] ...................... 3.44 3.44 3.44 1.72 1.72 1.72 1.72 1.72 1.72
S/N thresholds:
Full sky ................. 4.0 4.0 4.0 4.6 4.7 4.8 ... ... ...
Extragalactic zoneb ................. ... ... ... ... ... ... 4.9 4.7 4.9
Galactic zoneb ................. ... ... ... ... ... ... 6.0 7.0 7.0
Full sky ................. 1256 731 939 3850 5675 16 070 13 613 16 933 24 381
| b | > 30deg ................. 572 258 332 845 1051 1901 1862 3738 7536
N( >S)c:
Full sky ................. 934 535 689 3425 5229 15 107 13 184 15 781 23 561
| b | > 30deg ................. 373 151 191 629 857 1409 1491 2769 6773
| b | ≤ 30deg ................. 561 384 498 2796 4422 13 698 11 693 13 012 16 788
Flux densities:
Minimumd [mJy] ................. 461 825 566 266 169 149 289 457 658
90% completeness [mJy] ................. 575 1047 776 300 190 180 330 570 680
Uncertainty [mJy] ................. 109 198 149 61 38 35 69 118 166
Position uncertaintye [arcmin] ................. 1.8 2.1 1.4 1.0 0.7 0.7 0.8 0.5 0.4

Notes.

(a)

FEBeCoP band-averaged effective beam. This table shows the exact values that were adopted for the PCCS. For HFI channels, these are the FWHM of the mean best-fit Gaussian. For the LFI channels, we use , where Ωeff is the FEBeCoP band-averaged effective solid angle (see Planck Collaboration IV 2014 and Planck Collaboration VII 2014 for a full description of the Planck beams). When we constructed the PCCS for the LFI channels we used a value of the effective FWHM slightly different (by ≪1%) than the final value specified in the Planck Collaboration IV (2014) paper. This small correction will be made in later versions of the catalogue.

(b)

The Galactic and extragalactic zones are defined in Sect. 2.3.

(c)

Number of sources above the 90% completeness level.

(d)

Minimum flux density of the catalogue at | b | > 30deg after excluding the faintest 10% of sources.

(e)

Positional uncertainty (median value) derived by comparison with PACO sample (Massardi et al. 2011; Bonavera et al. 2011; Bonaldi et al. 2013) up to 353 GHz and with Herschel samples in the other channels (see Sect. 3.2.3 for more details).

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