2nd MayNova in PerseusDSLR piggybacked on main scope. 200mm 5x90 seconds CCD camera Nova has dimmed a bit since 30th April 5th MayA bit dimmer still:I have not imaged M51 with the QSI camera, or with the 20cm reflector. It was last imaged in colour when the supernova occured in August 2011. This is 14x600 seconds in luminance: A cropped image: 6th May M109 8x600 seconds 7th May 4x600 seconds on M108 8th May 4x600 seconds on ngc2787 ngc3079 4x600 seconds 10th May A fairly dim and sparse galaxy ic2574 4x10 minutes ngc2403 2x10 minutes M82 2x10 minutes 13th May M106 2x 600 seconds I took several images of Phecda to investigate the flare present on the images of M109 on May 6th. With the star near the centre of the image there is no flare: Near the corner still no flare. Extra diffraction type artefact which often occurs when a bright star is near the edge of the ccd sensor. With the star off the sensor the flare is more pronounced: Now a large oval ghost appears: 17th May M17 8 x 120 seconds from iTelescopes in Australia |