Location & Date	Backyard, Abbott Observatory- Long Island, NY,  July 2022
Telescope	Orion ED80 F/7 APO, Moonlite focuser, iOptron GEM45G, Pegasus Falcon rotator Image scale 2.54 arcsec/pixel
Camera	SBIG ST-2000XM Baader  L R G B  filters CCD temp -15°C
Exposures	L- 20 x 3m  Red- 10 x 3m  Green - 10 x 3m  Blue- 10 x 3m  Bin 1x1 for each of the 6 panels
Planning & Acquisition	Sequence Generator Pro Mosaic Tool - 6 panel mosaic
Processing	CCDStack -  Calibration, Deconvolution Astro Pixel Processor - Registration, mosaic panel assembly, LRGB combine Adobe PS -  Color adjustments, Noise reduction, Sharpen, JPEG conversion RC-Astro Star XTerminator, NoiseXTerminator ProDigital - Star glow effects This is a 6 panel mosaic

Wikipedia-

    Collinder 399, Cr 399 also known as Al Sufi's Cluster or Brocchi's Cluster, is a random grouping of stars located in the constellation Vulpecula near the border with Sagitta. The members of the star cluster form an asterism which has given rise to its name as the Coathanger.

  It was first described by the Persian astronomer Al Sufi in his Book of Fixed Stars in 964.

In the 17th century, it was independently rediscovered by the Italian astronomer G. B. Hodierna.

In the 1920s, Dalmero Francis Brocchi, an amateur astronomer and chart maker for the American Association of Variable Star Observers (AAVSO), created a map of this object for use in calibrating photometers. In 1931, Swedish astronomer Per Collinder listed it in his catalogue of open clusters.

  The status of this group as a star cluster has changed in recent years. The group was considered to be a cluster for most of the 20th century. Looking at a variety of criteria, however, a study in 1970 concluded that only 6 of the brightest stars formed an actual cluster. Several independent studies since 1998 have now determined that this object is not a true cluster at all, but rather just a chance alignment of stars. These recent studies have generally based their findings on improved measurements of parallax and proper motion provided by the Hipparcos satellite which were first published in 1997.

  The asterism is made up of 10 stars ranging from 5th to 7th magnitude which form the conspicuous "coathanger", a straight line of 6 stars with a "hook" of 4 stars on the south side. An additional 30 or so fainter stars are sometimes considered to be associated as well.

Left of CR399 is NGC6802 an Open Galactic Cluster also in the constellation of Vulpecula.
Above CR399 towards the right you can see SH2-83, a small emission nebula.

NGC6802 position shown relative to our location (Sun) in the Milky Way Galaxy

Galatic Longitude: 55.3

Galatic Latitude: 0.9

Distance from Galatic Plane:148 ly above the galatic plane

Above image and info provided by Our Galaxy 3D Atlas application and used with permission by Otherwise