{
 "item": "H-6",
 "overlay_rule": "consistency overlay only; never enters any likelihood or prior",
 "source": "paper/h/g3/g3_map.json",
 "verdict_counts": {
  "BUILDABLE_PESSIMISTIC": 557,
  "BUILDABLE_OPTIMISTIC": 153,
  "NOT_BUILDABLE": 140,
  "LITERATURE_SILENT": 111
 },
 "bh25_favoured": {
  "m_range": [
   200000.0,
   300000.0
  ],
  "a_range": [
   1.5,
   2.2
  ],
  "note": "Banares-Hernandez et al. 2025 (arXiv:2408.00939, A&A 693, A104) favour an extended central mass of 2-3e5 Msun emulating a cluster of heavy stellar remnants, with a 3-sigma IMBH upper limit of 6e3 Msun. The 1.5-2.2 pc scale range is the restatement carried in the Paper H WU brief; it is not quoted in the paper's abstract and was not verified beyond it here."
 },
 "hpd90_regions": {
  "nolegprof_plummer_5200": {
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   "M_hi": 25118.864315095823,
   "a_hi": 0.012283531735409992,
   "n_cells": 49,
   "n_grid": 1891,
   "touches_a_lo": true,
   "extended_cells": 0
  },
  "nolegprof_plummer_5494": {
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  "nolegprof_abg_5494": {
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   "touches_a_lo": true,
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  }
 }
}