Review the full set, then decide what comes next.
This Stage 1 evidence index retains candidates, controls, distance shells, out-of-volume physical references, and explicit rejects. Missing fields remain “Not yet assessed / —” as recorded; catalogue values are not promoted to conclusions.
Optical and available XMM / Chandra layers are included, with 5′ / 10′ / 15′ angular-radius circles defined by Astropy WCS. Legend: cyan dashed = D25 ellipse; white / yellow / coral = 5′ / 10′ / 15′ WCS circles. X-ray images are 30′ × 30′ cutouts; the HiPS2FITS request grid is width=height=300, giving 6.00 arcsec pix⁻¹; this is not server-side post-processing resampling. Display stretches are for morphology navigation only and must not be used to judge flux, exposure, spectral colour, or significance. Background and HiPS observation footprints / mosaic edges are retained for morphology and coverage diagnostics. Weak features near an edge are not standalone halo evidence. Some catalogue objects may lack public HiPS coverage.
Parameter-space screening
Select X / Y coordinates and use the three two-handle sliders at left, bottom, and right to form an intersection; the same subset drives the table below. Records missing any selected scalar are excluded from both the scatter plot and table.
Note: this is a sample-screening tool based on current metadata scalars, not a physical inference. Ranges are closed intervals; complete / circularised quality for the D25 ellipse is given in the object details and image metadata.
| Object | Distance | Geometry | Mass / SFR | X-ray archive | Environment | halo / wind / bubble | Radio structure | eDIG / Hα | HI / warp / lag | BH-mass evidence | AGN evidence | Sample role |
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