M31 (Andromeda), Daniele Malleo

M31 (Andromeda)

M31 (Andromeda), Daniele Malleo

M31 (Andromeda)

Equipment

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Acquisition details

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Description

Another go at reprocessing data from earlier in the season.

I have concentrated on reducing the FWHM of my blue stars, as well as revealing the details in the bright core of the galaxies (M31 and M32!), which were very much lost on my first attempt.

Also, this is the first time I have used (successfully?) a deconvolution process synthesizing a PSF from a sample of 50 or so stars in the frame.

Constructive criticism always welcome: is this too much? Is there possibly more detail that could be eked out?

From Wikipedia:

The Andromeda Galaxy is a spiral galaxy approximately 2.5 million light-years (2.4×1019 km) from Earth in the Andromeda constellation. Also known as Messier 31, M31, or NGC 224, it is often referred to as the Great Andromeda Nebula in older texts.

The Andromeda Galaxy is the largest galaxy of the Local Group, which also contains the Milky Way, the Triangulum Galaxy, and about 30 other smaller galaxies.

At an apparent magnitude of 3.4, the Andromeda Galaxy is one of the brightest Messier objects, making it visible to the naked eye on moonless nights even when viewed from areas with moderate light pollution. Although it appears more than six times as wide as the full Moon when photographed through a larger telescope, only the brighter central region is visible to the naked eye or when viewed using binoculars or a small telescope.

Technical Details:

Acquired on August 2, 2013 from Blue Canyon, CA

L: 7 x 20m

R,G,B:7 x 10m each (2x2 bin)

Total exposure time: ~6 hours

Main Camera: QSI 583 WSG

Guide Camera: SXV Lodestar (on OAG)

Mount: Astro-Physics Mach 1

Scope: Explore Scientific 102 f/7 (FL: 696mm)

Image Aquisition software MaximDL

Registed, Calibrated and Stacked in MaximDL

Post Processed with PixInsight 1.8

Comments

Histogram

M31 (Andromeda), Daniele Malleo