Astrophotography diagnosis of SH2-119: Backfocus error, noise / underexposure and 1 other

Processed35x300s

The Doc examined this image of SH2-119 (processed, 35x300s). Estimated overall technical quality: 7/10. 3 defects found: Backfocus error (severity 2/5), Noise / underexposure (severity 2/5), Clipped stars (severity 1/5).

Annotated image
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Info

Cible
SH2-119

A last crescent at 30% illumination is a very comfortable condition for an emission nebula like SH2-119. In narrowband or with a selective filter, this phase adds almost no parasitic background as long as the target stays at a good angular distance from the Moon, and the crescent rises late in the second half of the night, leaving a clean window early on. The background measurement shows no characteristic lunar gradient either: azimuthal anisotropy is low (0.1) and the profile stays a gentle radial one. In other words, conditions are not the limiting factor here, total integration time is.

- the Doc

Setup

Type d'image
Traitée
Exposition
35x300s
Phase de lune
Dernier croissant (30%)

The optical train's sampling is appropriate for the target: with a central FWHM of 3.1 px and an elongation floor of 1.04, stars are tight and well resolved, with no penalizing oversampling. The field covers SH2-119 generously, the target fits entirely in frame with comfortable margins, a good focal length choice. The weak point of the setup is field correction: FWHM climbs from 3.1 px at center to 4.5 px in the bottom-left corner, meaning a corrector poorly spaced or slightly short for the image circle in use. On the acquisition side, 35 subs of 300 s give under three hours, which is light for a nebulosity of this surface faintness, whatever the gear.

- the Doc

The diagnosis in detail

The diagnosis comes down to two threads that do not intersect. The first is purely optical: the aberration inspector shows a clean center (elong 1.09 against a field floor of 1.04, FWHM 3.11 px) and degradation rising with radius across all four corners, corner/center ratio 1.209. That is the classic signature of uncompensated field curvature, so a backfocus outside tolerance rather than a tracking fault, which would have elongated the central stars too. The bottom-left corner stands out (elong 1.56, FWHM 4.48 px): not asymmetric enough to call it true tilt, but it suggests that on top of the spacing, the optical train has slight mechanical play on one side. The order of attack is therefore spacing first, clamping only afterwards.

The second thread is a photon budget problem. The measured background-to-black-point margin (e_margin 1.73) and the positive Bowley skew say the sky background is barely lifted off the black point, and the result shows in the background grain, particularly in the right half where the faint nebulosity sinks into noise. With under three hours on such a diffuse target, no processing will recover what was never captured: smoothing would only erase the very extensions you are trying to show.

The rest is cosmetic. A few bright star cores are clipped, a limited loss of nuance easily avoided with a set of short complementary exposures. Overall the image is already very presentable, and the two improvement levers are clear and independent of one another.

Priority actions

  1. Double the integration at minimum, aim for 8 to 10 hours on SH2-119 to lift the faint extensions out of the noise
  2. Measure and correct the corrector backfocus spacing in 0.5 to 1 mm steps until the corner/center FWHM ratio drops below 1.15
  3. Check clamping and play in the optical train, particularly on the bottom-left side of the field, which degrades more than the other corners
  4. Add a short series of 10 to 30 s exposures to rebuild the bright star cores in HDR
  5. Dither systematically between subs to improve background smoothing at rejection