© James Janusz 2000 thru 2015 All Rights Reserved |
Telescope: Astro-Physics Ricardi-Honders Astrograph (RHA) | Designation: The Sadr region, or IC 1318, is the diffuse emission nebula surrounding Sadr or Gamma Cygni. Sadr lies in the center of Cygnus's cross. The Sadr region is one of the surrounding nebulous regions; others include the Butterfly Nebula and the Crescent Nebula. It contains many dark nebulae in addition to the emission diffuse nebulae.Sadr itself has approximately a magnitude of 2.2. The nebulous regions around the region are also fairly bright. (Wiki) |
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Mount: Astro-Physics AP1600 GTO | Constellation: Cygnus |
Camera: Apogee U16-M with Astrodon Ver. 2 Filters | Remotely Imaged With CCD Commander - Maxim |
Guiding: Baader Guidescope with Astro-Physics Mount System, SBIG ST-i Guider | Type: Nebula |
Exposure Data: HA 3 hours. | Position: R.A. 20 hr 23 min , Dec +40 18016' |
Processed using PixInsight, PhotoShop CS3 | Date: May 2015 |
Data Acquisiton, Reduction and Processing by Jim Janusz | Imaging Location: Cave Creek Canyon Observatory |
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