I read this on amastro

and thought some of our more adventurous imagers
Might be interested in giving it a go at taking a picture

Several weeks ago, during a DSS survey of the outer Milky Way in Sagittarius, I
came across a new and bright (!) obvious planetary nebula candidate in the
vicinity of Barnard's Galaxy NGC 6822 which may be of interest for some of the
PN folks here on amastro.
Coordinates of the candidate are 19 37 43.77 -13 51 20, size is approx.
0.7'x0.45'. The appearance of the nebula on the (blue) DSS-I image suggests a
mild bipolar morphology; the red DSS-II image shows also a central star
candidate immediately N of a superimposed star. Nothing in SIMBAD or NED at this
position. VIZIER shows a double entry of the object in the LEDA catalogue of
Paturel et al. (LEDA 932285 and LEDA 932333) but the object is clearly a line
emitter and not a pair of (interacting) galaxies. There is no IRAS or radio
source present at this position, which is probably one of the reasons why the
object has remained unnoticed until now. The PN candidate is only 1.5 degrees
distant from NGC 6818 (2 degrees from NGC 6822) and easily found 6' N of the 7
mag star SAO 162831.
I managed to observe the object last week with my new 15" under good
transparency (ZLM ~ 6m,8 - 7m,0). Even without filter a very faint glow appeared
at the position of the PN candidate. An OIII filter boosted the visibility of
the object considerably and showed it as a roundish glow with approx. 20" size
that could be held easily with averted vision. I also tried to see the two lobes
individually but failed to do so, probably due the lack of contrast and the
faintness of the object. The total brightness of the object I estimate to be ~15
mag, so it should be possible seeing it with apertures of 12" or even less.
Clear skies!
Matthias