Table 1 -- Synthetic Large-Scale Filament Properties (Zucker, Smith, & Goodman 2019)

This is a machine readable (e.g. via astropy tables 'ascii' format) version of Table 1 found in Zucker, Smith, & Goodman 2019. The columns are as follows: gridnum -- the ID for the filament, defined using the lower left hand corner position of the AREPO grid it is identified on in the right panel of Figure 1 arm -- whether the filament lies in an arm (1) or an interarm region (0) length_perp -- the length of the filament (pc) in the perpendicular projection length_sun -- the length of the filament (pc) in the sun-like projection maskwidth_perp -- the width of the filament (pc) in the perpendicular projection maskwidth_sun -- the width of the filament (pc) in the sun-like projection medianN_perp -- the median H2 column density (cm^-2) of the filament in the perpendicular projection medianN_sun --the median H2 column density (cm^-2) of the filament in the sun-like projection mass_perp -- the mass of the filament (Msun) in the perpendicular projection mass_sun -- the mass of the filament (Msun) in the sun-like projection linemass_perp -- the linemass of the filament (Msun/pc) in the perpendicular projection linemass_sun -- the linemass of the filament (Msun/pc) in the sun-like projection height_perp -- the 2D projected separation (pc) between the filament and midplane in the perpendicular projection height_sun -- the 2D projected separation (pc) between the filament and the midplane in the sun-like projection pangle_perp -- the 2D projected orientation (degrees) between the filament and the midplane in the perpendicular projection pangle_sun -- the 2D projected orientation (degrees) between the filament and the midplane in the sun-like projection velgrad_perp -- the velocity gradient (km/s/pc) along the filament in the perpendicular projection velgrad_sun -- the velocity gradient (km/s/pc) along the filament in the sun-like projection