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Table B.1:

Submm and mm photometry of all debris disks that have been detected at submm and longer wavelengths.
Star Other name $\lambda$ $F_{\nu}$ Reference
    ($\mu $m) (Jy)  
HD 105   870 $10.7\pm5.9$a 1

HD 377

  1200 $4.0\pm1.0$ 11

HD 8907

  1200 $3.2\pm0.9$ 11

HD 14055

$\gamma$ Tri 850 $5.5\pm1.8$ 3

HD 15115

  850 $4.9\pm1.6$ 3

HD 17206

${\tau}^{1}$ Eri 1300 $20.7\pm3.9$ 6

HD 21997

  870 $8.3\pm2.3$ 3
    870 $17.6\pm8.0$ 1

HD 22049

${\epsilon}$ Eri 450 $225\pm10$ 12
    850 $40.0\pm1.5$ 12
    1300 $24.2\pm3.4$ 6

HD 30447

  870 $6.9\pm5.0$a 1

HD 32297

  1300 $5.1\pm1.1$ 10

HD 38393

  850 $2.4\pm1.0$ 12

HD 39060

$\beta$ Pic 850 $58.3\pm6.5$ 4
    870 $63.6\pm6.7$ 2
    1200 $24.3\pm3.0$ 5
    1300 $24.9\pm2.6$ 6

HD 39944

  1350 $3.7\pm0.9$ 14

HD 48682

56 Aur 850 $5.5\pm1.1$ 12

HD 61005

  350 $95\pm12$ 11

HD 95086

  870 $41.3\pm18.4$ 1

HD 98800b

TV Crt 870 $33.6\pm8.4$ 1
    1350 $36.8\pm4.2$ 14
    2000 $24.8\pm3.4$ 14

HD 104860

  350 $50.1\pm9.3$ 11
    1200 $4.4\pm1.1$ 11

HD 107146

  350 $319\pm6$ 11
    450 $130\pm40$ 7
    850 $20\pm4$ 7

HD 109085

${\eta}$ Cor 850 $7.5\pm1.2$ 12

HD 109573

HR 4796 450 $180\pm150$ 12
    850 $19.1\pm3.4$ 8, 12
    870 $21.5\pm6.6$ 1

HD 123160

  850 $13\pm4.3$ 14
    1350 $4.7\pm0.9$ 14

HD 128167

$\sigma $ Boo 850 $6.2\pm1.7$ 12

HD 131835

  870 $8.5\pm4.4$ 1

HD 141569b

  450 $66\pm23$ 12
    850 $14\pm1$ 12
    870 $12.6\pm4.6$ 1
    1300 $9.39\pm3.72$ 13
    1350 $5.3\pm1.1$ 14

HD 152404b

AK Sco 450 $242\pm32$ 15
    800 $83\pm9$ 15
    870 $42.9\pm9.8$ 1
    1100 $36\pm4$ 15

HD 161868

$\gamma$ Oph 870 $12.8\pm5.2$ 1

HD 170773

  870 $18.0\pm5.4$ 1

HD 172167

Vega 850 $45.7\pm5.4$ 4, 12
    1300 $11.4\pm1.7$ 16

HD 181327

  870 $51.7\pm6.2$ 2

HD 191089

  350 $54\pm15$ 11

HD 195627

  870 $13.0\pm7.1$a 1

HD 197481

AU Mic 850 $14.4\pm1.8$ 9

HD 207129

  870 $5.1\pm2.7$ 1

HD 216956

Fomalhaut 450 $595\pm35$ 12
    850 $97\pm5$ 12
    850 $81\pm7.2$ 4

HD 218396

V342 Peg 850 $10.3\pm1.8$ 3

HIP 23200

V1005 Ori 850 $4.8\pm1.2$ 9

Notes.  (a) Marginally detected. (b) Debris disk status disputed.

References. (1) This paper; (2) Nilsson et al. (2009); (3) Williams & Andrews (2006); (4) Holland et al. (1998); (5) Liseau et al. (2003); (6) Chini et al. (1991); (7) Williams et al. (2004); (8) Greaves et al. (2000); (9) Liu et al. (2004); (10) Maness et al. (2008); (11) Roccatagliata et al. (2009); (12) Sheret et al. (2004); (13) Walker & Butner (1995); (14) Sylvester et al. (2001); (15) Jensen et al. (1996); (16) Wilner et al. (2002).


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