Table A.1: Standard c2d conversion factors for masses and column densities from dust emission. For each bolometer camera employed by the c2d collaboration we list the effective wavelength, the half power beam width, the dust opacity at the effective wavelength (per gram of ISM), the conversion factors between intensity and column density, and between integrated flux density and mass (this for a distance of $100~\rm pc$), respectively.
Camera $\lambda$ $\theta_{\rm HPBW}$ $\kappa_{\nu}$ $N_{\rm H_2} / F_{\nu}^{\rm beam}$ $M / F_{\nu} (d = 100~{\rm pc})$
  $\rm\mu m$ arcsec $\rm cm^2~g^{-1}$ $\rm cm^{-2} ~ (mJy~beam^{-1})^{-1}$ $M_{\odot}~\rm Jy^{-1}$
SHARC II 350 8.5 0.101 $7.13 \times 10^{19}$ 0.031
SCUBA 450 7 0.0619 $1.42 \times 10^{19}$ 0.041
  850 15 0.0182 $1.34 \times 10^{20}$ 0.18
BOLOCAM 1120 31 0.0114 $6.77 \times 10^{19}$ 0.39
MAMBO 1200 11 0.0102 $6.69 \times 10^{20}$ 0.47
SIMBA 1200 24 0.0102 $1.41 \times 10^{20}$ 0.47


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