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Table 1

Stellar parameters and photometry of the targets observed.

HD Sp. T. d vsini log(Age) θ V − K V H K FIR FIR references
number [pc] [km s-1] [Gyr] [mas] [mag] [mag] [mag] excess?
142 F7V 25.6 11 0.44 0.5198 5.7012 4.64676 4.47424 NO B09, E14
1581 F9.5V 8.6 2.3 0.60 1.14917 4.2238 2.88120 2.81520 NO T08, E14
2262 A5IV 23.5 225 − 0.15 0.69810 3.9372 3.54620 3.52320 YES S06
3302 F5V 36.2 17 0.21 0.4938 5.5082 4.62576 4.50226 NO Br06, T08
3823 G0V 25.5 2.3 0.83 0.5327 5.8908 4.67216 4.48615 NO T08
4150 A0IV 73.7 133 − 0.27 0.4577 4.3612 4.35476 4.30827 YES S06
7570 F9V 15.1 4.3 0.55 0.76210 4.9603 3.71320 3.66620 YES K09
7788 F6V 20.4 61 0.41 0.73911 4.9128 3.75020 3.70020 NO E14
10647 F9V 17.4 5.5 0.26 0.54772 5.5173 4.399234 4.340276 YES T08, E13
11171 F3III 23.6 58 0.02 0.626120 4.6523 3.470180 3.890389 YES K10
14412 G8V 12.7 0.0 0.57 0.5527 6.3354 4.69444 4.55116 NO T08, K09, E13
15008 A3V 41.5 190 − 0.38 0.5417 4.0742 3.97420 3.96220 NO S06, Kpc
15798 F5V 25.8 4.6 0.44 0.77011 4.7342 3.62720 3.58820 NO T08
16555 A6V 44.5 6.6 − 0.26 0.4687 5.2933 4.60023 4.52521 NO P09, Kpc
17051 F8V 17.2 6.5 0.12 0.6329 5.3962 4.13020 4.08020 NO Br06, T08, Kpc
17925 K1V 10.4 4.9 − 0.45 0.72510 6.0444 4.05020 4.04020 YES H08, T08, E13
19107 A8V 43.1 150 − 0.74 0.4056 5.2524 4.83442 4.74124 NO Kpc
20766 G4V 12.1 2.7 0.25 0.67610 5.5118 4.08820 4.00520 NO Br06, T08, E13
20794 G8V 6.02 2.0 0.91 1.295173 4.2568 2.709234 2.636278 YES K09
20807 G0V 12.1 2.7 0.60 0.74711 5.2288 3.82020 3.77020 YES E13
22001 F5V 21.4 13 0.36 0.70410 4.7054 3.74020 3.72020 NO Be06, Kpc
23249 K1IV 9.0 2.3 0.87 1.81025 3.5223 1.53920 1.90720 NO Be06, K09
25457 F6V 19.2 18 − 0.02 0.59111 5.3793 4.34276 4.18136 YES H08
28355 A7V 49.2 105 − 0.17 0.4395 5.0112 4.57014 4.55011 YES S06, C08
29388 A6V 45.9 89 − 0.14 0.5607 4.2624 4.078228 3.96016 NO S06
30495 G1.5V 13.3 3.6 0.02 0.67513 5.4813 4.116236 3.99936 YES T08, K09, E13
31295 A0V 37.0 11 − 1.12 0.44811 4.6464 4.51747 4.41647 YES S06
31925 F5V 43.2 7.2 0.35 0.5157 5.6734 4.64676 4.47916 NO T07
33111 A3III 27.2 180 − 0.41 1.18020 2.7822 2.439204 2.38030 NO Kpc
33262 F9V 11.7 15 − 0.12 0.87998 4.7082 3.407202 3.371234 YES Br06, T08
34721 G0V 24.9 4.4 0.70 0.4947 5.9544 4.748266 4.62020 NO T08, K09
38858 G4V 15.6 0.3 0.43 0.5768 6.1937 4.49920 4.44520 YES Be06, K09
39060 A6V 19.3 13 − 1.68 0.70710 3.8512 3.50020 3.48120 YES S84, S06
40307 K2.5V 12.8 1.6 0.61 0.5467 7.1577 4.96840 4.79316 YES E13
43162 G5V 16.7 5.5 − 0.45 0.4966 6.3623 4.86336 4.72616 NO E13
45184 G1.5V 22.0 2.5 0.52 0.4536 6.3663 4.96220 4.87120 YES L09, K10
53705 G0V 16.3 1.6 0.93 0.62311 5.5344 4.16420 4.14030 NO Be06, Kpc, E13
56537 A3V 28.9 154 − 0.22 0.65181 3.5722 3.495284 3.535262 NO Kpc
69830 G8V 12.6 1.6 0.70 0.6569 5.9454 4.364224 4.17020 NO E13
71155 A0V 38.3 14 − 0.96 0.5347 3.8812 3.93020 3.93220 YES S06
72673 G9V 12.2 0.0 0.54 0.59712 6.3773 4.763296 4.43836 NO Be06
76151 G3V 17.1 4.0 0.34 0.5379 5.9983 4.53020 4.50030 YES Br06, T08, E13
76932 G2V 21.3 2.6 1.05 0.56112 5.8093 4.38920 4.38043 NO Be06, Kpc
82434 F3IV 18.6 156 0.15 1.06518 3.5822 2.700234 2.76030 NO C05
88955 A2V 31.5 10 − 0.46 0.59710 3.8322 3.75820 3.74230 YES Z11
90132 A8V 40.5 270 − 1.15 0.4266 5.3312 4.789 4.68621 NO Kpc
91324 F9V 21.9 8.3 0.58 0.79380 4.8882 3.588204 3.582214 NO Be06
99211 A7V 25.7 7.3 − 0.25 0.705188 4.0723 3.523570 3.546526 NO Kpc
102365 G2V 9.2 0.7 0.83 0.94314 4.8818 3.37720 3.30820 NO Be06, Kpc
104731 F5V 24.2 15 0.19 0.6048 5.1532 4.11720 4.08520 NO B06, T08
108767 A0IV 27.0 236 − 0.48 0.79211 2.9534 3.04920 3.05520 NO S06, Kpc
109787 A2V 40.4 296 − 0.38 0.5778 3.4852 3.71520 3.70220 NO Kpc
115617 G7V 8.5 3.9 0.66 1.147129 4.7278 2.974176 2.956236 YES B06, T08
120136 F6IV 15.6 15 0.14 0.85612 4.4802 3.40020 3.35020 NO T08, B09, E13
128898 A7V 16.4 13 ... 1.00525 3.1742 2.73030 2.74050 NO E13
129502 F2V 18.7 47 0.12 1.02714 3.8653 2.93820 2.89520 YES E14
130109 A0V 39.5 285 − 0.41 0.61321 3.7262 3.628202 3.67070 NO Kpc
134083 F5V 19.7 44 0.17 0.6617 4.9262 3.90520 3.88010 NO T08, Br06, E13
135379 A3V 29.6 68 − 0.61 0.5698 4.0602 3.89020 3.88020 YES M09mir
136202 F8IV 24.7 4.8 0.63 0.62385 5.0483 3.947284 4.008284 YES K10mir
139664 F5V 17.5 1.8 0.02 0.72310 4.6383 3.68020 3.66020 YES Be06
141891 F1 12.3 92 0.76 1.43320 2.8262 2.13220 2.08520 YES K10mir
149661 K2V 9.8 2.2 0.13 0.77611 5.7624 3.91020 3.85520 NO Br06, T08
152391 G8.5V 16.9 3.0 0.11 0.4878 6.6498 4.94244 4.83529 NO Br06, T08
160032 F4V 21.9 16 0.35 0.66294 4.7544 3.702218 3.830294 YES E14
160915 F5V 17.5 12 0.42 0.65588 4.8613 3.787270 3.877280 NO K10*
164259 F2IV 23.2 69 0.25 0.71610 4.6204 3.70020 3.67020 NO Be06
165777 A4IV 25.4 65 − 0.33 0.71712 3.7113 3.426216 3.42030 NO Kpc
172555 A7V 29.2 116 − 1.68 0.4949 4.7692 4.251212 4.29831 YES R08
178253 A2V 39.8 20 − 0.41 0.51467 4.0942 3.915252 4.049272 YES M09mir
182572 G8IV 15.6 2.2 0.76 0.85818 5.1522 3.54520 3.53040 NO K10*
188228 A0V 32.5 89 − 1.42 0.58772 3.9462 3.762234 3.800258 YES S06, B13
192425 A2V 47.1 180 − 0.37 0.3785 4.9403 4.80134 4.76717 YES M09
195627 F0V 27.6 122 − 0.70 0.57865 4.7492 4.016228 4.044236 YES R08
197157 A9IV 24.2 150 − 0.28 0.63982 4.5063 3.692280 3.820268 NO P09, Kpc
197692 F5V 14.7 41 0.14 0.949119 4.1392 3.104184 3.094262 NO B06, T08, Kpc
202730 A5V 29.8 135 − 0.31 0.5188 4.4822 4.22476 4.14526 NO P09
203608 F9V 9.2 3.7 0.69 1.07815 4.2234 2.99020 2.91720 NO B06, T08, Kpc
206860 G0V 18.4 10 − 0.15 0.51410 5.9534 4.59836 4.55938 YES B06, T08, E13
207129 G2V 15.6 3.5 0.25 0.6279 5.5672 4.20020 4.14020 YES T08, E13
210049 A1.5IV 40.0 307 − 0.51 0.4556 4.4883 4.35120 4.34920 NO S06, Kpc
210277 G0 21.3 1.8 0.92 0.4887 6.5354 4.95731 4.79920 YES E13
210302 F6V 18.7 14 0.35 0.70510 4.9294 3.82020 3.78020 NO T08, E13
210418 A1V 29.6 144 − 0.28 0.73410 3.5202 3.38020 3.33020 NO S06, Kpc
213845 F7V 22.7 35 0.07 0.52382 5.2063 4.266258 4.327326 YES E14
214953 F9.5V 23.6 4.5 0.59 0.5267 5.9914 4.59520 4.53220 NO Kpc
215648 F7V 16.3 6.7 0.69 1.08941 4.2034 3.078214 2.89580 NO Be06, K09, Kpc
215789 A2IV 39.8 235 − 0.24 0.89942 3.4802 3.162268 3.000100 YES E14
216435 G0V 33.3 5.7 0.65 0.4728 6.0203 4.74120 4.71130 YES B09, K09
219482 F6V 20.6 7.5 0.05 0.5277 5.6493 4.606228 4.43715 YES B06, E13
219571 F4V 22.0 79 0.42 1.00314 3.9922 3.02520 2.96820 NO K10*
224392 A1V 48.7 20 − 0.38 0.3685 4.9942 4.94931 4.82421 NO D12, Z11

Notes. Uncertainties on the stellar diameters and magnitudes are given in μas and 10-3 mag, respectively. The note “mir” added to some reference for the far-infrared detection means that only mid-infrared data or only upper limits in the far-infrared are available, but the detected mid-infrared excess strongly suggests the presence of excess at longer wavelengths.

Reference. Distances were taken from the Hipparcos catalog (Perryman et al. 1997). References for the far-infrared excesses are B09: Bryden et al. (2009), B13: Booth et al. (2013), Be06: Beichman et al. (2006), Br06: Bryden et al. (2006), C05: Chen et al. (2005), C08: Cieza et al. (2008), D12: Donaldson et al. (2012), E13: Eiroa et al. (2013), E14: this work, see Sect. 2, H08: Hillenbrand et al. (2008), K09: Kóspál et al. (2009), K10: Koerner et al. (2010), K10*: Koerner et al. (2010), observed but no detection published, Kpc: Herschel/DEBRIS data, G. Kennedy, personal communication, L09: Lawler et al. (2009), M09 Morales et al. (2009), P09: Plavchan et al. (2009), R08: Rebull et al. (2008), S06: Su et al. (2006), S84: Smith & Terrile (1984), T07: Trilling et al. (2007), T08: Trilling et al. (2008), Z11: Zuckerman et al. (2011a). Stellar parameters were collected from Malagnini & Morossi (1990); Allende Prieto & Lambert (1999); Gerbaldi et al. (1999); Feltzing et al. (2001); Erspamer & North (2003); Mallik et al. (2003); Głȩbocki & Gnaciński (2005); Valenti & Fischer (2005); Gray et al. (2006); Saffe et al. (2008); Sousa et al. (2008); Önehag et al. (2009); Lafrasse et al. (2010); Soubiran et al. (2010); Casagrande et al. (2011); Díaz et al. (2011); Wu et al. (2011); Ammler-von Eiff & Reiners (2012); van Belle (2012); Zorec & Royer (2012). Stellar ages were collected from Edvardsson et al. (1993); Marsakov & Shevelev (1995); Rocha-Pinto & Maciel (1998); Gerbaldi et al. (1999); Lachaume et al. (1999); Zuckerman & Webb (2000); Feltzing et al. (2001); Chen et al. (2001); Ibukiyama & Arimoto (2002); Lambert & Reddy (2004); Rocha-Pinto et al. (2004); Thorén et al. (2004); Wright et al. (2004); Bensby et al. (2005); Riekeet al. (2005); Valenti & Fischer (2005); Reddy et al. (2006); Barnes (2007); Ramírez et al. (2007); Rhee et al. (2007); Takeda et al. (2007); Mamajek & Hillenbrand (2008); Holmberg et al. (2009); Chauvin et al. (2010); Ghezzi et al. (2010); Gonzalez et al. (2010); Casagrande et al. (2011); Tetzlaff et al. (2011); Trevisan et al. (2011); Maldonado et al. (2012); Vican (2012); Zorec & Royer (2012); Eiroa et al. (2013); Maldonado et al. (2013); Pace (2013); Tsantaki et al. (2013).

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