Astrophotography diagnosis of Pléiades: Light pollution gradient, clipped stars and 1 other

Processed360x20s

The Doc examined this image of Pléiades (processed, 360x20s). Estimated overall technical quality: 6/10. 3 defects found: Light pollution gradient (severity 3/5), Clipped stars (severity 3/5), Background chroma noise (severity 2/5).

Annotated image
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Info

Cible
Pléiades
Position
3h46m60s · +24°07'12"

Lunar conditions were ideal: a 3% waxing crescent, so no moon contribution to the sky background. The measured gradient therefore comes entirely from local light pollution or a low altitude above the horizon. The Pleiades are a broadband target, very sensitive to sky background: this is the right lunar window for them, but shoot them as high as possible and point away from the light source. The reported seeing of 5 is mediocre, which partly explains the rather puffy bright stars.

- the Doc

Setup

Type d'image
Traitée
Télescope
Seestar s50
Monture
AZimutale
Exposition
360x20s
Phase de lune
Premier croissant (3 %)
Seeing
5
FOV
1.50°

The Seestar s50 fits well here: a 1.50 degree field frames the main cluster with the Merope and Maia nebulosity, even though the Pleiades spill slightly beyond the frame, which remains an acceptable composition. 360 subs of 20s, so 2 hours of signal, are enough to pull out the reflection nebulosity, but 20s subs on magnitude 3 stars inevitably saturate the cores: that is a structural limit of the instrument on this target. An extra set of short exposures blended in HDR is the only real remedy. The alt-az mount holds up fine at this sub length, no tracking defect visible.

- the Doc

The diagnosis in detail

The diagnosis comes down to two independent points, one in acquisition, one in processing. On acquisition, the sky background carries a clear linear gradient, measured at 63% amplitude oriented at 274 degrees, with a plane fitting at R2=0.96 and dominating any radial component by a factor of 39. So this is not vignetting: it is a light ramp of external origin, and with the Moon at 3% ruled out, it points to ground light pollution or a target shot too low. This gradient was clearly not removed before stretching, which bakes it into the final image and also pulls the background color toward brown-red along the left edge.

On processing, the stretch was pushed hard enough to flatten the cores of the main Pleiades into white plateaus, which costs the blue signature of those giants. The same excess contributes to bloating the star discs, an effect amplified by mediocre seeing. Finally, with a background-to-black-point margin of only 1.55, the image is not truly sky-limited and chroma noise remains visible in the dark areas.

Nothing structural: stars are round out to the corners, the Seestar calibration holds, and the file is entirely recoverable by reprocessing from the master.

Priority actions

  1. Remove the gradient on the linear image with GraXpert or DBE before any stretch, then neutralize the background
  2. Redo the stretch with a star mask to preserve the blue tint of the Pleiades cores
  3. Add a set of short exposures for an HDR blend of the bright stars
  4. Apply targeted chroma noise reduction on the sky background only
  5. Shoot the target higher above the horizon and away from the light pollution source