  We demonstrate a newly developed mid-infrared planetary nebula (PN) selection
technique. It is designed to enable efficient searches for obscured, previously
unknown, PN candidates present in the photometric source catalogues of Galactic
plane MIR sky surveys. Such selection is now possible via new, sensitive,
high-to-medium resolution, MIR satellite surveys such as those from the Spitzer
Space Telescope and the all-sky Wide-Field Infrared Survey Explorer (WISE)
satellite missions. MIR selection is based on how different colour-colour
planes isolate zones (sometimes overlapping) that are predominately occupied by
different astrophysical object types. These techniques depend on the
reliability of the available MIR source photometry. In this pilot study we
concentrate on MIR point source detections and show that it is dangerous to
take the MIR GLIMPSE (Galactic Legacy Infrared Mid-Plane Survey Extraordinaire)
photometry from Spitzer for each candidate at face value without examining the
actual MIR image data. About half of our selected sources are spurious
detections due to the applied source detection algorithms being affected by
complex MIR backgrounds and the de-blending of diffraction spikes around bright
MIR point sources into point sources themselves. Nevertheless, once this
additional visual diagnostic checking is performed, valuable MIR selected PN
candidates are uncovered. Four turned out to have faint, compact, optical
counterparts in our H-alpha survey data missed in previous optical searches. We
confirm all of these as true PNe via our follow-up optical spectroscopy. This
lends weight to the veracity of our MIR technique. It demonstrates sufficient
robustness that high-confidence samples of new Galactic PN candidates can be
extracted from these MIR surveys without confirmatory optical spectroscopy and
imaging. This is problematic or impossible when the extinction is large.

Instrumentation and Methods for Astrophysics;Astrophysics of Galaxies