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Astrophotography by Bob Franke

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NGC 457 - The Owl Cluster

 

Click the image for a higher resolution view. (1400 x 1050 - 695 KB)

Instrument

12.5" RCOS @  ~f/9 (2880 mm fl) at 1.28 arcsec/pixel. Shown at 2.54 and 1.36 arcsec/pixel.

Mount

Paramount ME

Camera

SBIG STL-11000 w/ FW8 filter wheel, AstroDon Gen-2 Filters

Acquisition Data

12/22/2014 to 12/26/2014 Chino Valley, AZ... with CCD Commander & CCDSoft, AOL guided.

Exposure

RGB

480 min. (16 x 10 min. each)  Bin 2x2

Software & Processing Notes

  • CCDSoft, CCDStack, PixInsight & Photoshop CS6.

  • No SDSS stars were available for color balancing, so a standard image-train color calibration was used, as determined by eXcalibrator v4.30, and then adjusted for altitude extinction.

  • CCDBand-Aid to repair KAI-11000M vertical bars.

  • CCDStack to calibrate and register the sub exposures and create the RGB image..

  • PixInsight processing includes gradient repair and non-linear stretching with HistogramTransformation.

  • PhotoShop for the final touch up.

Comment

NGC 457 or Caldwell 13 is an open star cluster in the constellation Cassiopeia. It was discovered by William Herschel in 1787, and lies over 7,900 light years away from the Sun. It has an estimated age of 21 million years. The cluster is sometimes referred by amateur astronomers as the Owl Cluster. Two bright stars, magnitude 5 Phi-1 Cassiopeiae and magnitude 7 Phi-2 Cassiopeiae can be imagined as the eyes. The cluster features a rich field of about 150 stars of magnitudes 12-15.

Source: Wikipedia