Table 4
Positions and fluxes of the 11 submillimeter sources identified in the 4.4 × 4.4arcmin2 field around PSZ1 G045.85+57.71, measured by fitting Gaussian models to the Herschel maps at each wavelength as described in Sect. 3.2.
| Source | 250 μm source position | 250 μm | 350 μm | 500 μm | 1.15 mm | 2.05 mm | 2.05 mm | rms |
| [mJy] | [mJy] | [mJy] | [mJy] | measured [mJy] | expected [mJy] | [mJy] | ||
|
|
||||||||
| SMG1 | 15:18:22.382, +29:29:03.42 | 43.6 ± 2.4 | 51.4 ± 3.4 | 61.2 ± 4.8 | 1.9 ± 2.2 | 0.33 ± 0.42 | 0.27 ± 0.09 | 0.42 |
| SMG2 | 15:18:16.978, +29:27:14.60 | 36.7 ± 2.3 | 27.3 ± 3.0 | 13.6 ± 3.5 | −2.1 ± 1.9 | ** | 0.04 ± 0.03 | 0.36 |
| SMG3 | 15:18:21.859, +29:28:30.33 | 27.0 ± 2.4 | −1.9 ± 9.3 | 2.1 ± 9.8 | −1.3 ± 2.1 | ** | 0.01 ± 0.01 | 0.38 |
| SMG4 | 15:18:22.277, +29:26:49.87 | 24.1 ± 2.5 | 9.5 ± 9.3 | 3.6 ± 9.1 | −0.2 ± 1.9 | −0.22 ± 0.36 | 0.07 ± 0.05 | 0.36 |
| SMG5 | 15:18:25.577, +29:28:46.96 | 19.4 ± 2.2 | −4.1 ± 9.5 | 0.6 ± 9.9 | −1.8 ± 2.2 | 0.27 ± 0.43 | 0.01 ± 0.02 | 0.43 |
| SMG6 | 15:18:17.270, +29:28:33.72 | 18.2 ± 2.4 | 14.6 ± 3.4 | −0.6 ± 9.3 | 2.3 ± 2.1 | 0.08 ± 0.38 | 0.01 ± 0.01 | 0.39 |
| SMG7 | 15:18:18.969, +29:26:20.75 | 14.0 ± 2.2 | −2.6 ± 9.2 | 9.0 ± 10.2 | 1.7 ± 2.1 | 0.26 ± 0.39 | 0.09 ± 0.05 | 0.39 |
| SMG8 | 15:18:23.657, +29:27:36.72 | 13.9 ± 2.2 | −1.9 ± 9.4 | −6.9 ± 9.8 | −0.8 ± 1.9 | 0.21 ± 0.36 | 0.04 ± 0.05 | 0.36 |
| SMG9 | 15:18:29.306, +29:27:03.83 | 13.9 ± 2.3 | 17.3 ± 3.1 | 9.7 ± 9.8 | 3.2 ± 3.3 | −0.29 ± 0.48 | 0.02 ± 0.01 | 0.48 |
| SMG10 | 15:18:19.522, +29:26:44.27 | 11.1 ± 2.1 | 9.7 ± 3.1 | 6.7 ± 10.0 | 1.1 ± 1.9 | 0.51 ± 0.38 | 0.04 ± 0.02 | 0.36 |
| SMG11 | 15:18:18.545, +29:27:57.47 | 8.1 ± 2.2 | −4.0 ± 9.0 | −3.1 ± 9.7 | 0.7 ± 1.8 | ** | 0.01 ± 0.01 | 0.36 |
Notes. The 260 GHz NIKA map is also used to constrain each source SED at low frequency. Fluxes at 150 GHZ, which are not available because of the tSZ contamination are denoted by double stars **. The expected fluxes at 150 GHz are computed by integrating the estimated SED in the NIKA bandpass. The final column corresponds to the NIKA 150 GHz band rms noise at the source locations.
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