Survival of pure disk galaxies over the last 8 billion years
  Pure disk galaxies without any bulge component, i.e., neither classical nor
pseudo, seem to have escaped the affects of merger activity inherent to
hierarchical galaxy formation models as well as strong internal secular
evolution.
  We discover that a significant fraction (15 - 18 %) of disk galaxies in the
Hubble Deep Field (0.4 < z < 1.0) as well as in the local Universe (0.02 < z <
0.05) are such pure disk systems (hereafter, PDS). The spatial distribution of
light in these PDS is well described by a single exponential function from the
outskirts to the centre and appears to have remained intact over the last 8
billion years keeping the mean central surface brightness and scale-length
nearly constant. These two disk parameters of PDS are brighter and shorter,
respectively, than of those disks which are part of disk galaxies with bulges.
  Since the fraction of PDS as well as their profile defining parameters do not
change, it indicates that these galaxies have not witnessed either major
mergers or multiple minor mergers since z~1. However, there is substantial
increase in their total stellar mass and total size over the same time range.
This suggests that smooth accretion of cold gas via cosmic filaments is the
most probable mode of their evolution. We speculate that PDS are dynamically
hotter and cushioned in massive dark matter halos which may prevent them from
undergoing strong secular evolution.
