The importance of jet bending in gamma-ray AGN - revisited
  We investigate the hypothesis that {\gamma}-ray-quiet AGN have a larger
tendency for jet bending than {\gamma}-ray-loud AGN, revisiting the analysis of
Tingay, Murphy & Edwards (1998). We perform a statistical analysis using a
large sample of 351 radio-loud AGN along with {\gamma}-ray identifications from
the Fermi Large Area Telescope (LAT). Our results show no statistically
significant differences in jet-bending properties between {\gamma}-ray-loud and
{\gamma}-ray-quiet populations, indicating that jet bending is not a
significant factor for {\gamma}-ray detection in AGN.
