Astrophotography diagnosis of NGC 6085: Noise / underexposure, sensor tilt and 2 others
ProcessedLL 20×60s (total ~0.3 h)04 juin 2026
The Doc examined this image of NGC 6085 (processed, L, L 20×60s (total ~0.3 h)). Estimated overall technical quality: 5/10. 4 defects found: Noise / underexposure (severity 3/5), Sensor tilt (severity 2/5), Satellite trail (severity 2/5), Light pollution gradient (severity 2/5).
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Info
- Cible
- NGC 6085
- Date
- 04 juin 2026, 00:00
Tough conditions for this target: an 85% Moon combined with a broadband L filter on a faint galaxy field is about the worst possible pairing. Lunar luminance drowns the SNR and drives the measured oriented gradient (23% amplitude). Galaxies in a group like NGC 6085 need a dark sky and lots of signal; here the e_margin of 1.47 confirms an under-exposed background swamped by sky glow. Move this target away from full Moon (illumination below 30%) to gain several magnitudes of contrast, or reserve bright-Moon nights for emission targets with a dual-band filter. As is, processing spends its time fighting the background rather than revealing the galaxies.
Setup
- Type d'image
- Traitée
- Télescope
- Explore Scientific ED APO 127mm f/7.5 FCD-100 CF HEX
- Caméra
- ZWO ASI2600MC DUO
- Filtre
- L
- Monture
- Sky-Watcher Wave 150i Strainwave Mount
- Exposition
- L 20×60s (total ~0.3 h)
- Phase de lune
- 85%
- Notes
- Logiciels : Photoshop, SharpCap
The ED APO 127 f/7.5 at about 950 mm with the ASI2600MC gives comfortable sampling (center FWHM 2.37 px, well above the floor) and a wide field suited to a galaxy group. The Wave 150i tracking is excellent (center elong 1.02, scattered PA). Two points: a slight sensor tilt degrades the right side (FWHM 3.42 vs 2.65), to fix by squaring the optical train to even out the field. Above all, the L filter + galaxy target combo demands lots of exposure: 20x60s is far short. Move to 180-300s subs and aim for several hours total. The setup is healthy; it is the acquisition strategy that under-uses the instrument.
The diagnosis in detail
The PSF panel shows a sharp center (FWHM 2.37 px, elong 1.02 at the field floor) and flawless strainwave tracking: no drift, PE or oscillation signature. The shape defect is purely field optics: horizontal FWHM asymmetry (0.136 versus 0.047 vertical), corner/center ratio 1.31, right side spread out (TR 3.42, R 3.12, BR 3.08) against a sharp left side (TL 2.65, L 2.72, BL 2.81). This is the signature of a slight sensor tilt, to fix by squaring the train, not urgent given its moderate amplitude.
The real limiter is acquisition: 20x60s, about 0.3 h of broadband luminance under an 85% Moon. The histogram confirms it (e_margin 1.47, dark clipping 1.46%): under-exposed background, SNR at the floor. The field galaxies struggle to emerge, and the measured oriented gradient (23%, plane dominance 2.13) betrays poorly corrected lunar luminance before the Photoshop processing.
An un-rejected satellite trail crosses the upper-right quadrant, a consequence of the short stack. Nothing optically prohibitive: it is the acquisition strategy that needs rethinking to reveal this galaxy group.
Priority actions
- Greatly increase total integration (several hours) with 180-300s subs to lift the SNR
- Reschedule the target away from full Moon (illumination below 30%) to limit gradient and sky glow
- Extract the gradient (GraXpert/DBE) before stretching in Photoshop
- Correct the slight sensor tilt by squaring the optical train to even out the right side
- Strengthen rejection at integration to remove the satellite trail
Similar diagnoses

SH 2-73
Light pollution gradient

M42 - The Great Orion Nebula 1st capture (2019)
Oversaturation

Dumbbell Nebula (M27, NGC 6853)
Noise / underexposure
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