Astrophotography diagnosis of IC1396_0724: Backfocus error and tracking drift

Raw300s25 juil. 2026

The Doc examined this image of IC1396_0724 (raw, 300s). Estimated overall technical quality: 6/10. 2 defects found: Backfocus error (severity 3/5), Tracking drift (severity 2/5).

Annotated image
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Info

Cible
IC1396_0724
Date
25 juil. 2026, 21:44
Lune
Croissant décroissant 12.4% (12° d'alt., 102.3° de la cible)
Site
Bortle 2 · rural typique (VIIRS)
Position
21h40m36s · +58°16'59"

Excellent conditions: a Bortle 2 sky is ideal for a faint, extended target like IC 1396, and the Moon (waning crescent at 12.4%, only 12 degrees above the horizon and 102 degrees from the target) has no significant impact. The very dark background of this sub confirms it: no lunar gradient to worry about, and the dark nebulosity already stands out on a single 300 s exposure. You can stack many subs with no light-pollution or Moon limitation, giving a very favorable SNR on the faint structures of this region.

- the Doc

Setup

Type d'image
Brut
Télescope
EQMod Mount
Caméra
ZWO ASI585MM Pro
Exposition
300s
Phase de lune
Gibbeuse croissante (86 %)
FOV
1.70°

Setup consistent with the target: at 375 mm focal length the 1.70 degree field frames a portion of IC 1396 well, and the 1.60 arcsec/px sampling is comfortable, neither over- nor under-sampled for typical seeing. Central FWHM of 1.88 px (about 3.0 arcsec) is decent. The item to address is optical: the FWHM rise in the corners reveals a backfocus/spacing to adjust to exploit the full field. On settings, gain 252 is fairly high and the 300 s sub gives a background e_margin of 2.02, low but NORMAL here (mono, possibly narrow band, under a very dark sky). Offset 15 with no dark clipping and sensor at -14C are healthy.

- the Doc

The diagnosis in detail

This sub is well made. Under a Bortle 2 sky with no lunar interference, the dark nebulosity and dusty cirrus of IC 1396 are already readable on a single 300 s exposure, structurally matching the DSS reference: these are real signal, not artifacts. The background is clean, with no visible banding or walking noise, and the histogram (sufficient offset, no clipping) confirms healthy settings at -14C.

The only real job is star shape, measured by the aberration inspector. The center is tight (FWHM 1.88 px, elong 1.15) but FWHM rises symmetrically toward all four corners (ratio 1.87, elong 1.54-1.55 at TR and R with oval, stretched stars): this is the signature of an incorrect backfocus / field curvature, to be fixed at the optical spacing level. Added to this is a subtler component: central elongation slightly exceeds the field floor with a consistent PA everywhere (spread 13.7 degrees), i.e. a small tracking drift present down to the center.

As a priority, set the backfocus: it is what most penalizes the full-field rendering. The tracking drift is minor over 300 s and will partly smooth out during stacking, but it warrants a check of polar alignment and guiding.

Priority actions

  1. Set the backfocus precisely (thin spacers to the corrector's nominal value) to even out corner FWHM
  2. Check polar alignment and refine guiding calibration to reduce the directional drift
  3. Stack a large number of subs: the Bortle 2, Moon-free sky allows an excellent SNR on IC 1396's faint structures