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Table 14

Excess sources.

HIP SpT PACS70 S70 χ 70 PACS100 S100 χ 100 PACS160 S160 χ 160 Ld/L⋆ T d R d MIPS70 Notes
(mJy) (mJy) (mJy) (mJy) (mJy) (mJy) (K) (AU) (mJy)
171 G3V 22.90 ± 0.44 11.70 ± 1.26 11.22 ± 0.21 0.38 12.48 ± 2.36 4.38 ± 0.08 3.43 ≤21.6e-06 ≤25 ≥97.1 44.10 ± 13.63 H, p, c
544 K0V 15.24 ± 0.34 54.12 ± 1.00 7.47 ± 0.17 47.15 23.03 ± 2.06 2.92 ± 0.07 9.86 4.8e-05 90 7.5 102.6 ± 7.83 e
4148 K2V 13.66 ± 1.37 8.98 ± 0.13 3.42 11.33 ± 1.17 4.40 ± 0.06 5.92 15.64 ± 1.72 1.72 ± 0.02 8.09 9.4e-06 32 41.2 37.10 ± 6.59 p
7978 F8V 896.20 ± 26.90 17.48 ± 0.99 32.67 897.10 ± 26.90 8.56 ± 0.48 33.03 635.90 ± 31.80 3.35 ± 0.19 19.89 3.1e-04 60 26.6 863.4 ± 58.68 e
13402 K1V 20.72 ± 0.37 51.77 ± 1.11 10.15 ± 0.18 37.50 36.94 ± 2.94 3.97 ± 0.07 11.21 1.7e-05 52 17.9 67.70 ± 7.06 e
14954 F8V 26.43 ± 1.17 39.45 ± 1.75 12.95 ± 0.58 15.14 31.75 ± 1.16 5.06 ± 0.22 23.01 4.2e-06 40 95.0 42.50 ± 4.76 e, !
15371 G1V 44.50 ± 2.50 25.78 ± 0.33 7.49 40.40 ± 2.50 12.63 ± 0.16 11.11 42.60 ± 2.50 4.93 ± 0.06 15.07 1.0e-05 40 47.7 45.40 ± 4.95 e
17420 K2V 15.99 ± 1.81 9.36 ± 0.13 3.66 14.79 ± 0.84 4.58 ± 0.06 12.15 10.65 ± 1.30 1.79 ± 0.03 6.82 9.2e-06 45 20.7 23.60 ± 5.44 H, p, s
17439 K1V 74.80 ± 4.10 8.61 ± 0.14 16.14 75.00 ± 4.20 4.22 ± 0.07 16.85 74.60 ± 4.70 1.65 ± 0.03 15.52 8.1e-05 48 21.3 88.50 ± 7.46 e
22263 G3V 21.13 ± 0.38 77.60 ± 2.00 10.35 ± 0.18 33.62 47.00 ± 3.00 4.04 ± 0.07 14.32 2.9e-05 70 15.4 113.6 ± 8.53 e
27887 K3V 14.60 ± 1.43 10.01 ± 0.19 3.21 8.05 ± 0.95 4.90 ± 0.10 3.32 8.02 ± 1.50 1.92 ± 0.04 4.07 3.8e-06 29 46.2 17.20 ± 4.94 H, p
28103 F1V 56.33 ± 0.31 45.46 ± 1.42 27.60 ± 0.15 12.58 9.37 ± 1.84 10.78 ± 0.06 –0.77 6.3e-05 100 18.3 93.90 ± 7.76 p, s
29271 G5V 35.50 ± 0.42 17.80 ± 1.30 17.40 ± 0.21 0.31 14.35 ± 2.00 6.80 ± 0.08 3.78 ≤29.7e-06 ≤22 ≥147.3 42.60 ± 10.50 H, e, c
32480 G0V 264.00 ± 4.10 22.33 ± 0.27 58.94 252.30 ± 3.18 10.94 ± 0.13 75.90 182.09 ± 3.77 4.27 ± 0.05 47.17 6.9e-05 60 28.5 262.8 ± 18.29 e
42438 G1.5Vb 18.12 ± 0.25 17.31 ± 0.80 8.88 ± 0.12 10.54 6.73 ± 2.04 3.47 ± 0.05 1.60 1.1e-05 99 7.8 41.20 ± 4.16 p, s
43726 G3V 13.48 ± 0.26 15.77 ± 0.76 6.60 ± 0.13 12.07 6.09 ± 1.42 2.58 ± 0.05 2.47 1.6e-05 99 7.9 32.50 ± 4.13 p, s
49908 K8V 55.55 ± 2.11 22.50 ± 0.90 24.59 ± 1.03 -2.33 16.00 ± 1.70 9.61 ± 0.40 3.16 ≤21.6e-06 ≤22 ≥56.6 38.70 ± 4.69 H, e, c
51459 F8V 31.14 ± 0.53 19.71 ± 1.42 15.26 ± 0.26 3.13 9.17 ± 2.79 5.96 ± 0.10 1.15 9.1e-07 50 38.6 33.80 ± 4.43 H
51502 F2V 16.57 ± 0.22 47.25 ± 2.00 8.12 ± 0.11 19.57 72.45 ± 2.22 3.17 ± 0.04 31.21 1.3e-05 30 145.0 39.60 ± 3.79 e, !
62207 G0V 13.45 ± 0.11 55.06 ± 2.39 6.59 ± 0.05 20.28 44.49 ± 3.17 2.57 ± 0.02 13.22 2.1e-05 66 18.3 55.70 ± 5.20 e
65721 G5V 42.07 ± 0.36 40.73 ± 0.66 20.61 ± 0.17 30.48 26.97 ± 1.39 8.05 ± 0.07 13.61 3.8e-06 45 66.1 79.00 ± 8.09 p
71181 K3V 15.06 ± 1.30 9.98 ± 0.16 3.91 8.79 ± 1.00 4.89 ± 0.08 3.90 1.63 ± 1.63 1.91 ± 0.03 –0.17 8.0e-06 70 7.9 29.20 ± 8.04 H, p, s
72848 K2V 21.45 ± 1.06 19.60 ± 2.00 10.51 ± 0.52 4.55 13.30 ± 1.12 4.11 ± 0.20 8.21 2.8e-06 40 34.2 33.50 ± 6.41 H, e
73100 F7V 14.42 ± 0.23 13.84 ± 0.81 7.06 ± 0.11 8.37 12.46 ± 2.27 2.76 ± 0.04 4.27 2.7e-06 30 144.8 24.70 ± 3.17 p, c, !
85235 K0V 12.83 ± 0.19 34.70 ± 1.18 6.29 ± 0.09 24.08 28.00 ± 2.52 2.46 ± 0.04 10.13 2.0e-05 45 24.6 58.00 ± 4.92 e
92043 F6V 59.00 ± 3.50 48.70 ± 0.68 2.94 30.20 ± 2.40 23.90 ± 0.33 2.63 21.90 ± 3.80 9.34 ± 0.13 3.31 7.0e-07 30 213.3 69.80 ± 8.93 H, e, c
103389 F7V 44.00 ± 2.30 13.45 ± 0.23 13.28 26.30 ± 1.70 6.59 ± 0.11 11.59 7.70 ± 2.50 2.57 ± 0.04 2.05 1.7e-05 90 13.6 46.60 ± 4.93 p, s, !
107350 G0V 12.51 ± 0.17 15.10 ± 1.30 6.13 ± 0.08 6.90 4.40 ± 2.30 2.39 ± 0.03 0.87 1.2e-05 100 8.1 28.40 ± 3.15 p, s
107649 G2V 284.00 ± 1.50 18.38 ± 0.20 177.0 311.00 ± 1.00 9.01 ± 0.10 301.9 211.00 ± 1.50 3.52 ± 0.04 138.3 1.0e-04 55 28.7 278.2 ± 21.46 e
109378 G0 9.51 ± 0.13 8.50 ± 1.00 4.66 ± 0.07 3.84 12.40 ± 1.60 1.82 ± 0.03 6.61 5.4e-06 22 160.2 7.90 ± 2.26 H, p, c, !
114948 F7V 14.08 ± 0.19 40.80 ± 1.60 6.90 ± 0.09 21.19 13.30 ± 2.20 2.69 ± 0.04 4.82 2.7e-05 90 13.1 68.70 ± 5.51 p, s, !

Notes.PACS fluxes (PACSλ) together with the photospheric predictions (Sλ) and the significance at each band. The fractional luminosities and the black body temperatures and radii of the dust are also given as well as Spitzer fluxes at 70 μm. Column Notes: H = new Herschel debris disc, p = point-like object, e = resolved object, c = cold disc, s = steep source, ! = stars of the 20−25 pc subsample.

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