Celestial hemisphere:  Southern  ·  Constellation: Leo (Leo)  ·  Contains:  HD96363  ·  NGC 3521  ·  PGC 1143972  ·  PGC 1146703  ·  PGC 1146993  ·  PGC 1148913  ·  PGC 1149859  ·  PGC 1151550  ·  PGC 1151710  ·  PGC 1153557  ·  PGC 1157159  ·  PGC 1157434  ·  PGC 1157827  ·  PGC 1158782  ·  PGC 1158908  ·  PGC 1159494  ·  PGC 1160557  ·  PGC 1160720  ·  PGC 1161037  ·  PGC 1161170  ·  PGC 1161454  ·  PGC 1161646  ·  PGC 1163026  ·  PGC 1163606  ·  PGC 135770  ·  PGC 135771  ·  PGC 135772  ·  PGC 135773  ·  PGC 156258  ·  PGC 33536  ·  And 1 more.
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The Bubble Galaxy: Processing Insight 0.4 meter telescope data, Rick Veregin
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The Bubble Galaxy: Processing Insight 0.4 meter telescope data

Getting plate-solving status, please wait...
The Bubble Galaxy: Processing Insight 0.4 meter telescope data, Rick Veregin
Powered byPixInsight

The Bubble Galaxy: Processing Insight 0.4 meter telescope data

Equipment

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Acquisition details

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Description

As I wait for more data under skies that continue to worsen as we get into late fall, to complete my projects, my need to process is (partly) satisfied by purchased data from Insight.

The Galaxy
Often known as the Bubble Galaxy, because of the huge halo, NGC 3521 is a flocculent spiral about 35 million light-years from us.  The spiral arms, and indeed much is the galaxy, is broken up into fluffy patches of stars and dust. Thus, the spiral character is somewhat ill-defined. There is a slight bar, a weak inner ring, and moderate to loosely wound arm structure, thus it is categorized as an intermediate spiral: SAB(rs)bc. The galaxy is about one-half the diameter on our Milky way, about 50,000 light years across and is inclined by 72.7° to our line of sight.

The core has an HII region and  a low-ionization nuclear emission-line region (Liner). The spectra  for a Liner core typically includes line emission from weakly ionized or neutral atoms, such as O, O+, N+, and S+ (ie. OI, OII, NII and SII), while emission from strongly ionized atoms, such as O++, Ne++, and He+ (OIII, NeIII and HeII) is relatively weak. The mechanism for the ionization is not clear, it maybe be there is an active galactic nucleus (AGN) with a supermassive black hole, or the emission is powered by star forming regions.

The Insight HaLRGB Data
  • Total Integration: 7 hrs 35 min
  • Lum: 32x300 s = 2h 40 m
  • RGB: 15x300 s = 1h 15m each
  • Ha: 7x600 s = 1 h 10 m

The Insight setup is ATEO-1, which is:
  • Dreamscope 16" f/3.7 Astrograph
  • Software Bisque Paramount ME Mount
  • FLI Proline 16803 Camera
  • SkyPi Remote Observatory in Pie Town, New Mexico

My Processing
I produced individual LRGB and Ha  stacks using DeepSkyStacker. The Halpha data had been binned 2x so I used a 2X drizzle to match the LRGB data. 

I composed the image in StarTools, cropping and binning slightly (bin =0.71), followed by wipe (background extraction), a digital development with some adjustments to gamma, HDR, deconvolution, Ha accents addition,  initial color, star reduction and a superstructure isolation.

​​​​​​​In Photoshop I separated the galaxies from the stars using StarXterminator, then did an APF-R multi-scale unsharp mask on the galaxies only.  Stars were added back in with a linear dodge (add). Both layers were then adjusted for color, noise reduction using Astronomy Tools and NoiseXterminator.

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The Bubble Galaxy: Processing Insight 0.4 meter telescope data, Rick Veregin