An Ultra diffuse Galaxy in the NGC 5846 group from the VEGAS survey
  Many ultra diffuse galaxies (UDGs) have now been identified in clusters of
galaxies. However, the number of nearby UDGs suitable for detailed follow-up
remain rare. Our aim is to begin to identify UDGs in the environments of nearby
bright early-type galaxies from the VEGAS survey. Here we use a deep g band
image of the NGC 5846 group, taken as part of the VEGAS survey, to search for
UDGs. We found one object with properties of a UDG if it associated with the
NGC 5846 group, which seems likely. The galaxy, we name NGC 5846$\_$UDG1, has
an absolute magnitude of M$_g$ = -14.2, corresponding to a stellar mass of
$\sim$10$^8$ M$_{\odot}$. It also reveals a system of compact sources which are
likely globular clusters. Based on the number of globular clusters detected we
estimate a halo mass that is greater than 8$\times$10$^{10}$ M$_{\odot}$ for
UDG1.
