# Stellar Gas Population Grouping Study **Date:** 2026-05-09 **Decision:** `ADMIT_POPULATION_GROUPING_SURFACE` **Claim boundary:** MaNGA stellar-gas population grouping only. A coarse DESI/MaNGA cell join now exists; object-level crossmatch remains `HOLD`. Proxy classes do not prove physical shock, AGN, or gas mechanism. ## Population Surface ```text rows seen, all DAP types: 43128 unique Plate-IFU count: 10782 selected population: 10782 preferred DAPTYPE: HYB10-MILESHC-MASTARSSP ``` ## Aggregate ```json { "bpt_proxy_classes": { "agn_liner_or_shock_proxy": 2740, "star_forming_proxy": 5029, "composite_proxy": 2883, "unclassified": 130 }, "shock_lier_proxy_classes": { "shock_lier_proxy": 4589, "partial_shock_proxy": 2458, "no_shock_proxy": 3735 }, "partial_or_full_shock_fraction": 0.653589, "gas_sigma_summary": { "count": 10609, "min": 0.384927, "max": 929.010071, "mean": 157.969176, "median": 77.881104, "p90": 420.896637 }, "stellar_sigma_summary": { "count": 10297, "min": 3.115719, "max": 765.25354, "mean": 118.838681, "median": 94.604462, "p90": 233.339722 } } ``` ## Redshift Bins | Bin | Count | Shock+Partial Fraction | Gas Sigma Median | Stellar Sigma Median | |---|---:|---:|---:|---:| | `z_002_004` | 4838 | 0.619678 | 55.327721 | 72.146851 | | `z_004_006` | 2415 | 0.57764 | 78.61245 | 101.009289 | | `z_008_plus` | 1250 | 0.896 | 284.684052 | 230.705811 | | `z_000_002` | 1241 | 0.635778 | 30.074999 | 52.191267 | | `z_006_008` | 1038 | 0.717726 | 157.058464 | 172.332016 | ## DESI-Ready Sky/Redshift Cells These are population cells for the existing coarse DESI/MaNGA cell join. They are not object-level DESI/MaNGA crossmatches and not DESI environment classes yet. | Cell | Count | Shock+Partial Fraction | Main BPT Counts | |---|---:|---:|---| | `ra03_north__z_002_004` | 1622 | 0.676326 | `{'star_forming_proxy': 811, 'agn_liner_or_shock_proxy': 342, 'composite_proxy': 437, 'unclassified': 32}` | | `ra02_north__z_002_004` | 1289 | 0.584174 | `{'agn_liner_or_shock_proxy': 222, 'composite_proxy': 286, 'star_forming_proxy': 781}` | | `ra04_north__z_002_004` | 960 | 0.60625 | `{'agn_liner_or_shock_proxy': 219, 'composite_proxy': 257, 'star_forming_proxy': 483, 'unclassified': 1}` | | `ra02_north__z_004_006` | 684 | 0.554094 | `{'composite_proxy': 188, 'star_forming_proxy': 319, 'agn_liner_or_shock_proxy': 174, 'unclassified': 3}` | | `ra03_north__z_004_006` | 531 | 0.572505 | `{'star_forming_proxy': 246, 'composite_proxy': 152, 'agn_liner_or_shock_proxy': 131, 'unclassified': 2}` | | `ra00_north__z_000_002` | 450 | 0.72 | `{'star_forming_proxy': 214, 'agn_liner_or_shock_proxy': 79, 'composite_proxy': 117, 'unclassified': 40}` | | `ra04_north__z_004_006` | 420 | 0.6 | `{'agn_liner_or_shock_proxy': 128, 'star_forming_proxy': 159, 'composite_proxy': 133}` | | `ra03_north__z_006_008` | 374 | 0.754011 | `{'star_forming_proxy': 83, 'agn_liner_or_shock_proxy': 164, 'composite_proxy': 127}` | | `ra02_north__z_008_plus` | 364 | 0.881868 | `{'agn_liner_or_shock_proxy': 163, 'composite_proxy': 143, 'star_forming_proxy': 58}` | | `ra03_north__z_008_plus` | 305 | 0.918033 | `{'composite_proxy': 130, 'star_forming_proxy': 43, 'agn_liner_or_shock_proxy': 129, 'unclassified': 3}` | | `ra03_north__z_000_002` | 279 | 0.670251 | `{'agn_liner_or_shock_proxy': 40, 'star_forming_proxy': 188, 'unclassified': 14, 'composite_proxy': 37}` | | `ra02_north__z_000_002` | 270 | 0.581481 | `{'star_forming_proxy': 210, 'composite_proxy': 30, 'agn_liner_or_shock_proxy': 28, 'unclassified': 2}` | ## What This Gives Us - A population baseline over unique MaNGA Plate-IFU rows. - Grouped shock/LIER and BPT proxy counts by redshift and sky cell. - DESI-ready cells now used by the coarse DESI/MaNGA cell join. - Residual target: cells whose local gas state diverges from later DESI environment priors. ## Receipt `shared-data/data/stellar_gas_observation/stellar_gas_population_grouping_study_receipt_*.json` ## Receipt Backlinks - Coarse cell join receipt: `shared-data/data/stellar_gas_observation/desi_epoviz_manga_population_cell_join_receipt.json` - Tiddler: `6-Documentation/tiddlywiki-local/wiki/tiddlers/Stellar Gas Population Grouping Study.tid`