Coincidentally I photographed M101 on 17 May 2023, two days before supernova SN2023ixf was discovered. On 19 may I could confirm the supernova during a short break in the clouds. The wheather cleared on 24 May and the few astronomically dark hours enabled me to photograph M101 and SN2023ixf in L and RGB. Below the results are presented in different ways: A gif switching between 17 May and 24/25 May 2023, the images of the two dates side by side and the sum of both dates to obtain a higher quality image of M101. (Click on the images for a larger version.) Image information: Equipment: 25cm Newton f/D=5.7 with FTT1010M CCD and RGB filterwheel Sub-image exposures: 17 May: Luminance 15*120sec 24 May: Luminance 30*120sec 25 May: RGB 30*120sec eachFoV: 0.48x0.44 deg |
Gif switching between 17 and 24/25 May 2023 |
17 May and 24 May side by side | Sum of 17 and 24/25 May images |
|
25cm Newton prime focus, f/D=5.7 FTF2020-M (binned), MYC-filters and H-alpha Each color 20x90sec Lum.= M+Y+C 21 may 2004 + b/w-image of 2 june 2002 R-component = H-alpha image 30x120sec FoV: 0.7x0.5 degr. |
FTF2020-M CCD, binned 25cm Newton, f/D=5.7 Sum of 37 exposures of 90 sec |