For each simulation, we provide these files (grouped in a tar file):

• the mock SDSS-g band, PSF-convolved and noise-added images for each viewing angle, timestep
  hlsp_diggss_theory_*simname-cam?*_v1_img.tar.gz --> imgs/hlsp_diggss_theory_*simname*-cam?-t?_g_v1_img.fits

• the corresponding galaxy segmentation maps for each viewing angle, timestep
  hlsp_diggss_theory_*simname-cam?*_v1_seg.tar.gz --> segs/hlsp_diggss_theory_*simname*-cam?-t?_g_v1_seg.fits

• the output SUNRISE mock SDSS-g band images with no noise, no PSF convolution for each viewing angle, timestep
  hlsp_diggss_theory_*simname-cam?*_v1_raw.tar.gz --> segs/hlsp_diggss_theory_*simname*-cam?-t?_g_v1_raw.fits

• 'data' tables for each viewing angle, with timesteps, star-formation rates, galaxy separations, and morphologies
  hlsp_diggss_theory_*simname*_v1_morph.tar.gz --> morph/hlsp_diggss_theory_*simname*-cam?_v1_morph.fits

For more information about the products and files see the readme file.

Click on the Names to see a list of the files downloadable through the browser. Data are also available via anonymous ftp from archive.stsci.edu. cd /pub/hlsp/diggss.

Isolated Galaxy Simulations (Lotz et al. 2010a)

Equal-Mass Galaxy Simulations (Lotz et al. 2008)

[a] Initial orientation of galaxy with respect to the plane of the orbit in spherical coordinates, theta=arctan( sqrt(x² + y²))/z) and phi = arctan(y/x).
[b] Pericentric distance of the initial orbit, in kpc.
[c] Eccentricity of the orbit, where a parabolic orbit has e = 1.
[d] Supernova feedback polytropic index n where P ~ rho^{(1 + n/2)} .

Unequal-Mass Galaxy Simulations (Lotz et al. 2010a)