Dust extinction curves: Grasil-like

These datasets are based on the models described in Benson (2018), and are intended to mimic the geometries used by Grasil.

Dust Properties

Dust grain properties are taken from Draine (2003) - specifically their model with either RV=3.1 or RV=5.5 as encoded in the file name with prefix dustD03.

Stellar Geometry

Galactic disks follow exponential profiles in both radial and vertical directions, with the vertical scale height equal to 0.1 or 0.5 times the radial scale length as encoded in the file name with prefix hzStars. Note that spheroid radii in this work are listed as the scale radius, rs, while Ferrara et al. (1999) listed the corresponding effective radius, re=rs/1.16.

Dust Geometry

Dust is distributed in the disk, and follows exponential profiles in both radial and vertical directions. The vertical scale height is set to a multiple, hz, of the stellar disk scale height. The value of hz is encoded in each file name with prefix hzDust.