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Installation & Setup

6
  • System Requirements & Download
  • Installing Astro PM on Windows
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Astro PM App Guide

34
  • App Overview & Navigation
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Astro PM NINA Guide

10
  • Installing the NINA Plugin
  • Connecting NINA to Astro PM
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  • Building Your Sequence
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Astro PM Phone Guide

7
  • Installing the Phone App
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Single Image Analysis Tools

One sub, examined properly, can tell you whether your focus plane is tilted, your optics are collimated, your flats are keeping up with vignetting, and whether that donut in the corner is dust on the sensor or the filter. The Image Analysis panel is that examination.

Loading & Star Detection #

Open Image loads a FITS/XISF/TIFF (dimensions, file type, and bit depth shown). Choose a Fit Model – Gaussian (fast) or Moffat4 (more faithful to real star profiles; adds a Min R² fit-quality slider, default 0.60, to discard poor fits) – and run Star Detection. Results: HFR, HFD, FWHM, star count, eccentricity, mean ADU, plus image scale and field of view derived from the plate solve or the header’s focal length and pixel size.

Every deeper analysis builds on this step; an Auto-run checkbox runs the entire suite the moment detection finishes.

The Eight Analyses #

AnalysisWhat it measuresWhat the result means
Star DetectionHFR, FWHM, count, eccentricityoverall frame quality baseline
Eccentricitystar elongation across the frameguiding, wind, flexure issues
TiltHFR compared across a 3×3 zone gridfocus-plane tilt severity (%) and its direction – which corner is worst
PSF (Select Region)interactive point-spread function viewer3D intensity surface, directional radial profiles, HFR/FWHM rings for any star you select
Collimationeccentricity patterns and optical-center shifthow far the optical center sits from the geometric center
Vignettingbrightness in five concentric ringsedge falloff % plus horizontal/vertical profiles
Dust / Reflectionscircular dark and bright artifactseach found artifact circled and labeled, with an estimated distance from the sensor – which tells you which surface to clean
Exposurebackground statistics and saturationclipped stars, saturated area, background level vs. ideal

Each analysis paints its evidence onto the image: the tilt zone grid, vignetting rings, dust circles, PSF rings – you see the diagnosis, not just a number. Status dots track each analysis (gray = not run, green = done).

The Results Dashboard #

The dashboard column collects everything with progress-bar visualizations: star quality (HFR, FWHM, eccentricity, count), frame quality (tilt %, curvature, vignetting %, collimation shift, artifact count), and exposure (mean ADU, airmass when present). Hover any metric for the exact definition – e.g. tilt is (worst zone – best zone) / median HFR × 100.

Viewer & Annotation Tools #

The image viewer offers zoom (+/-, Fit, 1:1, mouse wheel; 10-500%), drag-to-pan, and a live cursor readout of pixel coordinates – plus RA/Dec once plate-solved. A Draw annotation mode lets you mark the image freehand in six colors (Yellow, Cyan, Lime, Red, Orange, White), with a clear button and label counter – handy for documenting an issue before posting it to a forum or sending it to us.

Metadata & External Tools #

The right column lists everything the header knows: filter, coordinates, date, exposure, gain/offset, binning, sensor temperature, airmass, focal length and ratio, pixel size, focus position, rotation. Below it, external integrations (configured in Settings):

  • Plate Solve with ASTAP – local solve; fills RA/Dec, rotation, and plate scale, and reports ASTAP’s own HFD/FWHM/star count for comparison.
  • Open in ASTAP – launches the full ASTAP GUI with the image.
  • Open CCD Inspector – hands the image to CCD Inspector if you use it.
Tip: Monthly ritual worth having: run the full suite on one good sub per rig. Tilt, collimation, and dust drift slowly – the dashboard catches them before they cost you a season’s data.
Updated on July 12, 2026
SubInspectorImage Annotator
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