Celestial hemisphere:  Northern  ·  Constellation: Cygnus (Cyg)  ·  Contains:  IC 1340  ·  NGC 6960  ·  NGC 6992  ·  NGC 6995  ·  Part of the constellation Cygnus (Cyg)  ·  The star 49Cyg  ·  The star 52Cyg  ·  The star Gienah (εCyg)  ·  The star ζCyg  ·  Veil Nebula
The arrows of time pinpoint us all, stille
The arrows of time pinpoint us all
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The arrows of time pinpoint us all

The arrows of time pinpoint us all, stille
The arrows of time pinpoint us all
Powered byPixInsight

The arrows of time pinpoint us all

Equipment

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Acquisition details

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Description

Veil Nebula in Perseid times. Funny how many of the meteors I've seen ended up being neither Perseids nor Kappa Cygnids nor anything identifyable.

Processing:

1 stack of 60 images, Canon 800D at ISO 800, Takumar 135mm f2.5 lens at f4, 30s exposures, tracked with Omegon minitrack lx2. a couple dozen darks, 120 biases. Processed in PixInsight as below

***** Integration

lightvortexastronomy tutorial (https://www.lightvortexastronomy.com/tutorial-pre-processing-calibrating-and-stacking-images-in-pixinsight.html)

* img 3027 has a meteor on it

* weighing:

15*(1-(FWHM-FWHMMin)/(FWHMMax-FWHMMin))

+ 25*(1-(Eccentricity-EccentricityMin)/(EccentricityMax-EccentricityMin))

+ 20*(SNRWeight-SNRWeightMin)/(SNRWeightMax-SNRWeightMin)

+ 40

img 2989 ref

drizzle integration

***** Meteor stack and initial adjustments

* take aligned meteor image, denoise with EZDenoise on default, integer upsample 2x

* dynamic crop both integration and meteor image to width 11250 height 7500 anchor x 5985 anchor y 3945

* extract RGB channels in drizzle, linearfit on green, recombine. Also linearfit the meteor image's channels to integration green. Clean up that geostationary that's too close to the meteor

** Mask generation

* iif( meteor_G > 0.0253 & d2seg(3395, 1894, 6233, 3754) < 50, 1, 0)

* clean up with clone stamp, blur 4 MLT layers - meteor_mask

* merge the two: meteor * meteor_mask + (1 - meteor_mask) * drizzle_integration

***** Linear processing

* DBE, tolerance 3, hand-placed points

* photometric CC, background neutralization on right corner, FL 135 pixel 2, centered on Veil

* SNCR green 0.95, with protected meteor

* Denoise with EZDenoise, lower TGV exponent by 1

** Remove halos

* blue mask: veil_B - (veil_G + veil_R) / 2, stretch mids = 0.003. clonestamp out nebula, stretch shadows 0.05 mids 0.15

* with mask on, SNCR blue, then green

***** Nonlinear processing

*** Initial stretch

* EzsoftStretch

* ACDNR on meteor trail, with lightness mask (blurred 4 layers)

* EZStarReduction, 8 iterations

***MLT stretch

http://www.stelleelettroniche.it/en/2014/09/astrophoto/m42-ngc1975-multilayer-processing-first-part/

**Initial (fine details)

* extract first 5 MLT layers, diff

* extract luma from original, stretch shadows 0.2 mids 0.25, then iif($T > 0.7, 0.7, $T), apply as mask on left

* sum back together, rescaled

**Second (Veil nebula)

* extract first 6 MLT layers, diff

* on mlt: star mask, boost RGB and saturation

* on left: extract luminance, stretch shadows 0.15 mids 0.15, iif($T > 0.8, 0.8, $T), blur 4 layers of MLT, apply as mask. Then curve boost RGB (some) and saturation(sharply)

* sum back together, rescaled

*** Finishers

* with star mask on, pump star saturation

* LHE kernel 24 contrast 1.5, blend 50% with original image

* MMT sharpen, 6 layers biases 0.05 0.05 0.025 0.025 0.012 0.005 on luminance

* on a clone, apply EZDenoise with no modifications. Meld back into original image by veil_clone * meteor_mask + (1 - meteor_mask) * veil

* desaturate meteor slightly

Comments

Sky plot

Sky plot

Histogram

The arrows of time pinpoint us all, stille