Celestial hemisphere:  Southern  ·  Constellation: Ophiuchus (Oph)  ·  Contains:  Hourglass nebula  ·  IC 4592  ·  IC 4604  ·  IC 4605  ·  IC 4701  ·  IC 4715  ·  Lagoon nebula  ·  M 17  ·  M 20  ·  M 7  ·  M 8  ·  NGC 6281  ·  NGC 6334  ·  NGC 6357  ·  NGC 6383  ·  NGC 6475  ·  NGC 6514  ·  NGC 6523  ·  NGC 6526  ·  NGC 6618  ·  Omega nebula  ·  Part of the constellation Ophiuchus (Oph)  ·  Part of the constellation Sagittarius (Sgr)  ·  Part of the constellation Scorpius (Sco)  ·  The star Antares (αSco)  ·  The star Dschubba (δSco)  ·  The star Graffias (β1Sco)  ·  The star Kaus Australis (εSgr)  ·  The star Lesath (υSco)  ·  The star Media (δSgr)  ·  And 6 more.
Getting plate-solving status, please wait...
Milky Way Core to Rho Ophiuchi, Andrew Klinger
Milky Way Core to Rho Ophiuchi
Powered byPixInsight

Milky Way Core to Rho Ophiuchi

Getting plate-solving status, please wait...
Milky Way Core to Rho Ophiuchi, Andrew Klinger
Milky Way Core to Rho Ophiuchi
Powered byPixInsight

Milky Way Core to Rho Ophiuchi

Equipment

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Acquisition details

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Description

Equipment:

Lens: Rokinon 24mm f/1.4 (stopped to f/4)

Mount: Orion Sirius EQ-G (HEQ-5)

Imaging camera: ZWO ASI1600MM-Cool

Software:

SGP

PHD2

CdC

PixInsight

Acquisition:

Location: Atoka, Oklahoma (Bortle 3)

Dates: 5/12/18

Gain: 76 Offset: 15

Camera temp: -10C

R: 9x180"

G: 10x180"

B: 10x180"

Total integration time: 1hr 27min

64x darks per calibration (master dark in library)

No flats (had issue with them)

200x bias (master bias in library)

Preprocessing:

Batch PreProcessing script to generate calibrated images

StarAlignment to register all frames to a reference

DynamicCrop each master

DBE on each master

RGB processing:

BackgroundNeutralization

ColorCalibration

SCNR green 50%

TGV and MMT noise reduction (via Jon Rista's method)

ArcsinhStretch and HistogramTransformation

SCNR green 100%

Duplicated the image to create a starless version, using a starmask and several iterations of MMT and MT. Then pushed the faint nebulosity in the starless version using PixelMath expression: "1-(1-$T)*(1-$T)".

Combined the starless version with the image using PixelMath expression "F=0.4; (1-(1-$T)*(1-s)*F)+($T*~F)" followed by the same expression but F=0.2 (s=starless photo).

CurvesTransformation for saturation

ExponentialTransformation with a mask to further push faint nebulosity

ColorSaturation to selectively saturate blues

MorphologicalTransformation for slight star reduction

Comments

Sky plot

Sky plot

Histogram

Milky Way Core to Rho Ophiuchi, Andrew Klinger