I finally got tired of looking at the bottom of cloud cover and rented some time from iTelescope last night. Using their T3 rig in New Mexico I got this image of IC 344. It is composed of ten-300 second color images shot with a SBIG ST-4000XCM camera mounted on a Takahashi TOA-150 Apo refractor. Nebulosity 4 was used for initial processing with fine tuning in Lightroom 5 and Apple's Photos Apps. I spent about six hours processing this image as it was a booger to pull the details out of the surrounding H-a cloud while retaining detail. I would like to go back and reshoot this object in narrow band as I suspect it will be quite interesting.
For those interested in such things, IC 443 is a supernova remnant about 5,000 ly or 1.5 kpc from earth with a surface magnitude of +12 located in Gemini. It is also known as the Jellyfish Nebula, and SH 2-248. The hydrogen-alpha emission is not the result of the origin neutron-star's radiation but rather, like the Veil Nebula, from the molecular shockwave's impact on a relatively dense dark hydrogen cloud that had nothing to do with the supernova. The origin neutron star (CXOU J061705.3+222127) is only visible in the x-ray band by satellite. It is located to the lower right, outside the image and is traveling approximately 800,000 km/hr away from the remnant shell. It is an oddly behaving neutron star with a comet-like tail. There is a good article about it at https://www.sciencedaily.com/releases/2006/06/060601212933.htm.