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Contains:  NGC 2366, NGC2363, NGC2366
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NGC 2366, 


            Frank Colosimo
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NGC 2366

Technical card

Dates:Dec. 11, 2018

Frames: 145x600" bin 0x0

Integration: 24.2 hours

Avg. Moon age: 3.84 days

Avg. Moon phase: 15.79% job: 2421747

RA center: 7h 28' 56"

DEC center: +69° 13' 32"

Pixel scale: 0.440 arcsec/pixel

Orientation: -36.414 degrees

Field radius: 0.255 degrees

Resolution: 3326x2504

Locations: Blue Mountain Vista Observatories, New Ringgold, Pennsylvania, United States

Data source: Backyard


NGC 2366 is a barred irregular dwarf galaxy located in the constellation Camelopardalis. It is part of the M81 group of galaxies, and lies about 10 million light years away. The southern end of NGC 2366 has a large, luminous HII region known as Markarian 71. Inside Mrk 71 there are two super star clusters (SSC) which are named 'A' and 'B' or 'Knot A' and 'Knot B'. To the side of Mrk 71 is another dwarf galaxy NGC 2363 which is interacting with NGC 2366.
This was a dim, challenging object, with an apparent magnitude of only 11.4, but the components were spread over an area of 8.1 x 3.3 arc minutes, so it was at least large enough to attempt to capture.

Date: Nov-Dec 2018
Location: Blue Mountain Vista Observatories,New Ringgold PA

Optics: Celestron EdgeHD 1100 on Paramount MX
Camera: Sbig STL-11000 for RGB

Optics: Starizona Hyperion f/8 12.5 inch, FL 2540 mm on Paramount ME
Camera: Apogee U8300 for Lum

Guiding: ST-402 on Innovations Foresight On-Axis Guider and STL-11000 Self guiding

Exposure: LRGB: L:74x10 R:28x10 min, G:22x10 min, B:21x10 min for a total of 24.2 hrs (145 subs at avg of 600 sec)
Processing: Image acquisition using CCD Autopilot. Initial processing was done using Maxim DL with subsequent processing with Photoshop.



Frank Colosimo
License: Attribution-NonCommercial-NoDerivs Creative Commons

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NGC 2366, 


            Frank Colosimo