§3 结果（论文体）§3 Results (paper style)
读前须知：单位与状态标签Before you read: units and status tags
距离 D = 19 Mpc，1 角分（′）= 5.53 kpc。面亮度单位 1 PW = 1e-7 个 XSPEC APEC 归一化每平方角分（0.3 keV 等离子体），对应 ∫ne nH dl = 1.49e15 cm⁻⁵。举例：一个 5 PW 的壁面亮度 ≈ 每平方角分 5e-7 个 apec 归一化。热压力 P = 2.3 n_H kT；举例：nH = 5.5e-5 cm⁻³、kT = 0.2 keV 时 P = 4.05e-14 dyn cm⁻²。状态标签（I021）：MEASURED = 直接测量（含场散误差）；INFERRED = 依赖模型；CONDITIONAL = 依赖明示假设；CANDIDATE = 非探测；WITHDRAWN = 不要引用。坐标架：+mnr = ENE（PA 75°），−mnr = WSW（PA 255°），盘方位角 PA 165°。
Distance D = 19 Mpc, 1 arcmin (′) = 5.53 kpc. Surface-brightness unit: 1 PW = 1e-7 XSPEC APEC norm per arcmin² of a 0.3 keV plasma, equivalent to ∫ne nH dl = 1.49e15 cm⁻⁵. Example: a wall brightness of 5 PW ≈ 5e-7 apec norm per arcmin². Thermal pressure P = 2.3 n_H kT; example: with nH = 5.5e-5 cm⁻³ and kT = 0.2 keV, P = 4.05e-14 dyn cm⁻². Status tags (I021): MEASURED = direct, with field-scatter errors; INFERRED = model-dependent; CONDITIONAL = rests on a stated assumption; CANDIDATE = not a detection; WITHDRAWN = do not cite. Frame: +mnr = ENE (PA 75°), −mnr = WSW (PA 255°), disk PA 165°.
来源Source: .agent/jobs/2026-10-15-S09-FACTS.md; I021_s09_paper_plan_v2.md
3.1 数据质量结果（科学的根基）Data-quality results the science rests on
五项数据质量结果决定了后续所有测量的口径（L1–L4）。MEASURED (1) 从 ODF 重新处理恢复了曝光，逐相机做了耀发 GTI 剔除，风区 PN/MOS 亮度比 1.07–1.12（L1）。(2) MOS1 CCD4 的软超出会制造一个假的 ~1 keV 成分，因此 MOS1 退出所有风区光谱（L2）。(3) MOS1 与 MOS2 都带一个随卷帘角变化的望远镜坐标架大尺度梯度（N−S 0.7–1.2 PW/′），PN 干净；因此 XMM 在 ≳5′ 的工作只用 PN，或给每台 MOS 加平面 nuisance 项（L2b）。(4) FXTDAS/CALDB v1.30 的 FXT 点源谱与 XMM 在 0.4–1 keV 一致到 0–10%（v1.20 最多低 37%）（L3）。(5) Chandra 目录中 19 个条目是弥漫气体而非点源，保留在图中（L4）。
Five data-quality results set the conventions of every later measurement (L1–L4). (1) Reprocessing from ODFs recovers the exposures; camera-level flare GTIs are applied; the wind-region PN/MOS brightness ratio is 1.07–1.12 (L1). (2) A soft excess on MOS1 CCD4 makes a false ~1 keV component, so MOS1 is excluded from all wind spectra (L2). (3) MOS1 and MOS2 both carry a roll-dependent, telescope-frame large-scale gradient (N−S 0.7–1.2 PW/′); PN is clean; XMM work beyond ≳5′ therefore uses PN only, or a plane nuisance per MOS camera (L2b). (4) FXTDAS/CALDB v1.30 FXT point-source spectra match XMM to 0–10% at 0.4–1 keV (v1.20 was up to 37% low) (L3). (5) 19 Chandra-catalogue entries are diffuse gas, not point sources, and stay in the maps (L4).
来源Source: cognition-os/experiments/E085_s09_xmm_ns_pointing_systematic.md; E083 handover; artifacts/s09_e085_xmm_ns/n3079_s09_e085_xmm_ns.png
3.2 ENE 轴上的背景星系团（L5）The background cluster on the ENE axis (L5)
MEASURED ENE 小轴上 h ≈ 4.3–6.5′（24–36 kpc）的拉长 X 射线条带不是风气体，而是红移 z = 0.593 的背景星系团 WH24 J100242.9+554158（M500 = 1.4e14 M⊙，13 个成员；SDSS 光谱 z = 0.59323/0.59357）。XMM 与 FXT 都看到它：形状延伸（XMM σ 44″ × 17.5″，PSF 5.5″，2ΔlnL = 64），谱上需要 kT ≈ 2.3 keV（z 0.593）的热成分（占 0.4–1.25 keV 超出的 57–84%）。它与小轴方向一致是巧合（chance ~0.2）。所有风分析都用 1.5′ 半径掩罩它（E090）。掩罩后，ENE 轴带亮度从无掩罩时的 4.5–9.3 PW（4.75–6.75′）降到 8.0/8.8 PW（3.75/4.25′）、7′ 以外 1–3 PW；"ENE 锥到 39 kpc 是填满的"这一旧结论是星系团造成的（已撤回）。
MEASURED The elongated X-ray strip on the ENE minor axis at h ≈ 4.3–6.5′ (24–36 kpc) is not wind gas. It is the hot gas of a background galaxy cluster at z = 0.593, WH24 J100242.9+554158 (M500 = 1.4e14 M⊙, 13 members; SDSS spectra z = 0.59323/0.59357). XMM and FXT both see it: extended shape (XMM σ 44″ × 17.5″ against a 5.5″ PSF, 2ΔlnL = 64), and the spectrum needs a hot component at kT ≈ 2.3 keV (z 0.593; 57–84% of the 0.4–1.25 keV excess). Its alignment with the minor axis is a coincidence (chance ~0.2). Every wind analysis masks it with a 1.5′ circle (E090). With the mask, the ENE axis strip falls from 4.5–9.3 PW (unmasked, 4.75–6.75′) to 8.0/8.8 PW at 3.75/4.25′ and 1–3 PW beyond 7′; the old "filled ENE cone to 39 kpc" was the cluster (withdrawn).
来源Source: XMMLineMap cognition-os/experiments/E090_n3079_ene_axis_feature_background_cluster.md; artifacts/s09_web_v10/v10_data.json
3.3 形态：X 形双极风（L6）Morphology: an X-shaped bipolar wind (L6)
MEASURED 0.3 keV 面亮度图显示一对沿小轴的双极风，X 形，逐历元（2017-only、2018-only）与逐仪器（XMM、FXT、联合）都可复现；FXT 复现 XMM 形态到 ~6′（E076）。灰圈为已扣除的点源（40″ 掩罩），黄圈为星系团掩罩。最终图集（C1：全部用 PN 或 PN+FXT 联合图重建）尚未完成，是论文 I 图 1–4 的前置条件。
MEASURED The 0.3 keV surface-brightness maps show a bipolar pair of winds along the minor axis, X-shaped, reproduced per epoch (2017-only, 2018-only) and per instrument (XMM, FXT, joint); FXT reproduces the XMM morphology to ~6′ (E076). Grey circles mark the subtracted point sources (40″ masks), the yellow circle the cluster mask. The final map set (C1: everything rebuilt on PN or the PN+FXT joint map) is not yet done and gates Paper I figures 1–4.
来源Source: artifacts/s09_web_v10/map_jointpn.png, map_xmmpn.png; E083 handover (L6, E076)
3.4 壁的延伸：测到 ~55 kpc，55–66 kpc 为候选（L7）Wall extent: measured to ~55 kpc, 55–66 kpc a candidate (L7)
MEASURED (39–55 kpc) CANDIDATE (55–66 kpc) 用分区剖面（壁楔 θ 15–45° 减去同半径外侧 θ > 52.5°）测壁超出 B。联合 PN+FXT（星系团掩罩后）：39–55 kpc B = 2.48 ± 0.43 PW；把 E084 的 0.3–0.5 PW 估计器系统学加进误差后为 4.8–3.8σ。55–66 kpc B = 2.09 ± 0.67 PW：加入估计器系统学为 2.9–2.5σ（RT-01），再加 RT-06 的 0.47–0.59 PW 掩罩系统学为 2.0–2.4σ（保守），随所含系统学不同在 2.0–2.9σ —— 候选，非探测。66 kpc 以外无探测（12–16′ 为 −0.26 ± 0.61），95% 上限 B < 0.75 PW（仅统计）。FXT 单独 3.3σ、XMM PN 单独 1.6σ，符号一致（联合值在 55–66 kpc 约 75% 由 FXT 加权，与 FXT 单独不独立）；MOS 单独为负（−0.64 ± 1.13、−2.07 ± 1.92）——正是 MOS 梯度曾把 v9 XMM 壁压低的原因。同统计量旋转零假设（29 条非相邻轴）：观测 B 超过全部对照，p ≤ 0.033。FXT 60′ 壁发射率可追到 70–80 kpc（WSW，误差大）。
MEASURED (39–55 kpc) CANDIDATE (55–66 kpc) The wall excess B is measured from zone profiles (wall wedge θ 15–45° minus the same-radius outside θ > 52.5°). Joint PN+FXT (cluster masked): B = 2.48 ± 0.43 PW at 39–55 kpc; 4.8–3.8σ once the E084 0.3–0.5 PW estimator systematic is added in quadrature. At 55–66 kpc B = 2.09 ± 0.67 PW: 2.9–2.5σ with the estimator systematic (RT-01), and 2.0–2.4σ (conservative) once the RT-06 0.47–0.59 PW mask systematic is added — 2.0–2.9σ depending on the systematics included, a candidate, not a detection. Beyond 66 kpc there is no detection (12–16′: −0.26 ± 0.61), with a 95% limit B < 0.75 PW (stat only). FXT alone gives 3.3σ and XMM PN alone 1.6σ, same sign (the joint value at 55–66 kpc is ~75% FXT-weighted, so it is not independent of FXT alone); MOS alone is negative (−0.64 ± 1.13, −2.07 ± 1.92) — the MOS gradient is what had pulled the v9 XMM walls down. A same-statistic rotated null over 29 non-adjacent axes: the observed B exceeds all controls, p ≤ 0.033. The FXT 60′ wall emissivity is traceable to 70–80 kpc (WSW, large errors).
红队 R1/RT-01/RT-06 措辞（已采纳）：55–66 kpc 是一个合并径向 bin 的显著性，不是一个带误差的端点；外延的"终点"需要 C3 的端到端注入-回收与系统学标定。本手册写"壁测到 ~55 kpc；55–66 kpc 合并 bin 内候选（2.0–2.9σ）"，不写"壁终于 66 kpc ± …"。掩罩放大到 60–70″ 只在 5–21 楔形源周围时 B 降到 1.2–1.5 PW（一条可能的 PSF 翼路径，未证实，RT-06 待定项）。
Red-team R1/RT-01/RT-06 wording (adopted): the 55–66 kpc value is the significance of a pooled radial bin, not an endpoint with an error bar; the outer reach needs the C3 end-to-end injection-recovery and systematics calibration. This handbook says "walls measured to ~55 kpc; a candidate in the pooled 55–66 kpc bin (2.0–2.9σ)", not "the walls end at 66 kpc ± …". Enlarging the masks to 60–70″ only around the 5–21 wedge sources lowers B to 1.2–1.5 PW (a possible PSF-wing route, not demonstrated; an RT-06 undecided item).
来源Source: cognition-os/experiments/E086_s09_l7_l8_pn_only.md; artifacts/s09_e086_l7_l8_pn/redo_l7_l8.json; R1 redteam REPORT.sol.md (rank 1)
3.5 45–90 kpc 无帽（L8）No cap at 45–90 kpc (L8)
MEASURED 用切圆模板与自由半径扫描（远点 ≥ 45 kpc，34 个旋转空假设，全局 p）搜"帽"。30° 帽扇区（避开壁）内无任何模板显著（p ≥ 0.24，两侧与折叠均如此）。60° 扇区内唯一显著的边（PN 联合，p < 0.03，远点 69 kpc）位于壁楔角内 —— 是壁的顶端，不是帽。95% 帽缘上限（联合 PN+FXT 折叠，60° 扇区）：50–70 kpc K95 ≈ 1.4 PW，70–90 kpc ≈ 2.1 PW（PW，0.3 keV 等离子体口径）；FXT 60′ 折叠到 110 kpc 为 0.9–2.0 PW。0.7–2 keV 硬带（FXT 60′）无热帽探测；在测得的晕密度下，软强击波帽会在软带上限边缘（边缘排除），热（1 keV）帽允许（E093）。红队 R1 措辞（已采纳）：这些是模板依赖的上限，"无帽"应写作"在所述模板与灵敏度内无需帽"，不排除闭式/热泡。
MEASURED A cap search uses tangent-circle templates and a free-radius scan (far point ≥ 45 kpc, 34 rotated nulls, global p). No template is significant in the 30° cap sector (clear of the walls; p ≥ 0.24 on both sides and in the fold). The only significant edge in the 60° sector (PN joint, p < 0.03, far point 69 kpc) lies inside the wall wedge — it is the top of the walls, not a cap. 95% cap-rim limits (joint PN+FXT fold, 60° sector): K95 ≈ 1.4 PW at 50–70 kpc and ≈ 2.1 PW at 70–90 kpc (PW, the 0.3 keV plasma-unit convention); the FXT 60′ fold gives 0.9–2.0 PW to 110 kpc. No hot cap is detected at 0.7–2 keV (FXT 60′); at the measured halo density a soft strong-shock cap would sit at the soft fold limit (marginally excluded) and a hot (1 keV) cap is allowed (E093). Red-team R1 wording (adopted): these are template-dependent limits; "no cap" should read "no cap required within the stated templates and sensitivities", which does not exclude a closed or hot bubble.
来源Source: cognition-os/experiments/E086_s09_l7_l8_pn_only.md (L8 tables); XMMLineMap E087, E093; n3079_e087_cap_circles.png
3.6 三维几何（3-D geometry）：WSW 锥→近等宽结构；ENE 张开（L9）3-D geometry: WSW cone → near-constant width; ENE flares (L9)
MEASURED (edge shape) INFERRED (3-D hollow chimney)（mock 标定；轴对称模型族内）对每 0.5′ 横向 bin、1′ 高度 bin（14–80 kpc）用精确 Abel 投影拟合轴对称壳+内部模型。WSW：半张角 44–46° 的厚壁锥（壁厚分数 f 0.45–0.6）在 ~40 kpc 处变为近等宽结构；锥形在 Δχ² +10.4（FXT 60′）/ +8.2（联合 PN）上更差，填充双锥被拒绝（Δχ² +14.8 / +18.6）。转折高度较宽：联合 dχ² ≤ 1 区间为 26–43 kpc（最佳 38.7–41.5 kpc）。"空心"是 ~2σ 上限（η = 1 代价 Δχ² 3.2–3.9；无显著边缘增亮）。ENE：~45° 锥，~40 kpc 以上缓慢张开；其填充不受约束（mock P 0.07–0.13）。Kompaneets 剧烈失宠（WSW Δχ² +28.6：底部太宽）。PN+FXT 联合图复核（S09 E087）：WSW 46° 锥 → 36 kpc 近烟囱，与 FXT 60′ 同形；ENE 不变。红队 RT-03（已采纳）：39 kpc 以上一个非轴对称的"双片"（two-sheet）模型拟合得同样好（Δχ² −0.96 FXT / +0.53 联合），6–8° 倾角与 HPD 尺度 PSF 不能解释边缘形状；因此"边缘形状锥→近等宽"是 MEASURED，"3-D 空心烟囱"是 INFERRED（轴对称 imposed）。
MEASURED (edge shape) INFERRED (3-D hollow chimney) (mock-calibrated; within axisymmetric families) Transverse profiles (0.5′ bins, 1′ height bins, 14–80 kpc) are fitted with axisymmetric shell + interior models projected by an exact Abel integral. WSW: a thick-walled cone of half-opening 44–46° (fractional thickness f 0.45–0.6) turns into a near-constant-width structure at ~40 kpc; the cone is worse by Δχ² +10.4 (FXT 60′) / +8.2 (joint PN), and a filled bicone is rejected (Δχ² +14.8 / +18.6). The break height is broad: the joint dχ² ≤ 1 interval is 26–43 kpc (best 38.7–41.5 kpc). "Hollow" is a ~2σ limit (η = 1 costs Δχ² 3.2–3.9; no significant limb). ENE: a ~45° cone flaring slowly above ~40 kpc; its fill is not constrained (mock P 0.07–0.13). Kompaneets blow-out is strongly disfavoured (WSW Δχ² +28.6: its base is too wide). The PN+FXT joint map recheck (S09 E087) gives the same WSW form (46° cone → near-chimney at 36 kpc), in the same shape as FXT 60′; ENE is unchanged. Red-team RT-03 (adopted): above 39 kpc a non-axisymmetric two-sheet model fits as well (Δχ² −0.96 FXT / +0.53 joint), and a 6–8° inclination and HPD-scale PSF do not explain the edge shape; so "edge shape cone → near-constant width" is MEASURED, while the "3-D hollow chimney" is INFERRED (axisymmetry imposed).
来源Source: XMMLineMap E094_n3079_wind_3d_geometry.md; E097; S09 E087_s09_joint_products_pn.md; R1 redteam (rank 7)
3.7 温度 kT(z)（L10）与 C2 复核Temperatures kT(z) (L10) and the C2 recheck
MEASURED 1T on-off APEC 谱拟合（Z 固定 0.3）：8–28 kpc kT 0.25–0.31 keV；41–61 kpc 壁 0.19–0.22 keV；每个高度上壁与内部共享一个 kT（E095，dC ≤ 2）。C2 复核（2026-10-15，去 MOS2）：归档门（WWALL:BG，MOS2+PN+FXT）精确复现 kT = 0.187298 keV；PN+FXT 重拟后 WSW 壁 41–61 kpc 0.187 → 0.182 keV、ENE 0.218 → 0.237 keV；所有相机对移动 ≤ 0.036 keV（≤ 1.3 倍归档半宽）；PN-only 更噪（最大移动 +2.53 半宽）。结论 L10 不变。
MEASURED 1T on-off APEC spectral fits (Z fixed at 0.3): kT 0.25–0.31 keV at 8–28 kpc; walls 0.19–0.22 keV at 41–61 kpc; wall and interior share one kT at each height (E095, dC ≤ 2). C2 recheck (2026-10-15, MOS2 removed): the archived gate (WWALL:BG, MOS2+PN+FXT) reproduces kT = 0.187298 keV exactly; with PN+FXT the WSW wall at 41–61 kpc moves 0.187 → 0.182 keV and the ENE wall 0.218 → 0.237 keV; every camera pair moves by ≤ 0.036 keV (≤ 1.3 archived half-widths); PN-only is noisier (largest move +2.53 half-widths). L10 stands.
| 相机对（regspec）Pair (regspec) | 归档 kT (keV)Archived kT (keV) | C2 PN+FXT | D (keV) |
|---|---|---|---|
WWALL:BG (e092) | 0.187 (0.150–0.226) | 0.182 (0.146–0.215) | −0.005 |
EWALL:BG (e092) | 0.218 (0.192–0.246) | 0.237 (0.211–0.268) | +0.019 |
WWLL:BG (e095) | 0.247 (0.231–0.265) | 0.248 (0.230–0.270) | +0.001 |
EWLL:BG (e095) | 0.239 (0.217–0.265) | 0.252 (0.220–0.288) | +0.013 |
来源Source: .agent/jobs/2026-10-15-c2-outer-spectra-pn-fxt/REPORT.hermes.md Table 1; out_hermes/kT/*.npy; XMMLineMap E092, E095
3.8 O/Fe：归档对 C2，与 Liu et al. 2026 比较（L11）O/Fe: archived against C2, and the Liu et al. 2026 comparison (L11)
MEASURED（相对值）CONDITIONAL（绝对值）1T 轮廓似然 O/Fe（a_O/a_Fe，Asplund 2009 太阳标度）：C2 PN+FXT 使最佳值下降 10–45% —— 壁 17–28 kpc 8.26 → 6.81（dC(O/Fe=1) +8.9 → +5.4）、内部 17–28 kpc 7.47 → 5.88（+11.7 → +6.6）、壁 41–61 kpc 11.2 → 6.6；pooled 壁 28–61 kpc 4.87 → 6.33（上升）。所有区间与归档重叠；上界仍触格点边 20。太阳（O/Fe = 1）仍被排除的：pooled 17–28 kpc 壁与内部、pooled 41–61 kpc 内部（dC +5.4/+6.6/+12.4）；单区 17–28 kpc 与 28–61 kpc 壁不再排除太阳。合并似然注意：pooled 拟合对每个 ON 区重复计一次 BG 谱（e079_fit.py:220，R1 astra 发现、Claude 确认），profile-dC 区间未校准；单区拟合不受影响。与 Liu et al. 2026（arXiv:2609.37646）比较：其 RGS 核心区 O/Fe = 0.47（mCIE+CX，Lodders 2009 标度，与 Asplund 2009 数字比相同，×1.00），EPIC-MOS 1T 为 3.5（1–2′）、5.1（2–3′）、4.1（NE+SW 扇区）—— 绝对 1T 值偏高的直接证据；两者标度换算（Lodders→Asplund）尚未做（C6）。
MEASURED (relative) CONDITIONAL (absolute) 1T profile-likelihood O/Fe (a_O/a_Fe, Asplund 2009 solar scale): C2 PN+FXT lowers the best values by 10–45% — walls 17–28 kpc 8.26 → 6.81 (dC(O/Fe=1) +8.9 → +5.4), interior 17–28 kpc 7.47 → 5.88 (+11.7 → +6.6), walls 41–61 kpc 11.2 → 6.6; pooled walls 28–61 kpc rise 4.87 → 6.33. Every interval overlaps the archive; upper bounds still hit the grid edge at 20. Solar (O/Fe = 1) remains rejected for the pooled 17–28 kpc walls and interior and the pooled 41–61 kpc interior (dC +5.4/+6.6/+12.4); the single 17–28 kpc regions and the 28–61 kpc walls no longer reject solar. Pooled-likelihood caveat: pooled fits count the BG spectrum once per ON region (e079_fit.py:220, found by R1 astra, confirmed by Claude), so their profile-dC intervals are uncalibrated; single-region fits are unaffected. Comparison with Liu et al. 2026 (arXiv:2609.37646): their RGS nucleus O/Fe = 0.47 (mCIE+CX, Lodders 2009 scale, numerically identical ratio to Asplund 2009, ×1.00), EPIC-MOS 1T 3.5 (1–2′), 5.1 (2–3′), 4.1 (NE+SW sectors) — direct evidence that absolute 1T values are biased high; the Lodders→Asplund conversion is not yet done (C6).
| 谱区（高度）Spec (height) | 归档 O/FeArchived O/Fe | C2（PN+FXT）C2 (PN+FXT) | dC(1) 归档→C2archived→C2 |
|---|---|---|---|
EWLL+WWLL:BG (walls 17–28) | 8.26 (4.09–20.0) | 6.81 (3.20–20.0 EDGE) | +8.9 → +5.4 |
EAXL+WAXL:BG (interior 17–28) | 7.47 (4.18–17.87) | 5.88 (3.19–12.95) | +11.7 → +6.6 |
EWLM+WWLM:BG (walls 28–39) | 3.07 (1.23–10.79) | 3.96 (1.29–15.76) | +1.5 → +1.5 |
EWALL+WWALL:BG (walls 41–61) | 11.23 (1.60–20.0) | 6.55 (1.05–20.0 EDGE) | +1.5 → +1.0 |
EWLM+WWLM+EWALL+WWALL:BG (walls 28–61 pooled) | 4.87 (2.03–20.0) | 6.33 (2.34–20.0 EDGE) | +3.4 → +3.6 |
来源Source: REPORT.hermes.md Table 2; out_hermes/ofe/*.npy; XMMLineMap E096 §d; P1 REPORT.sonnet.md (Lodders/Asplund ×1.00)
3.9 晕剖面与 47 kpc 密度（L12）—— 上限，非探测The halo profile and the density at 47 kpc (L12) — an upper limit, not a detection
LIMIT（2026-10-15 RT-05 分诊；原 MEASURED，模型依赖）沿主轴（PA 165/345 ±30° 扇区，1′ 环）的面亮度梯度给出中心热晕：晕未被探测到 —— FXT 60′ 振幅仅 1.63σ，PN 单独为 −0.33σ。引用上限：47 kpc 处 n_H < 0.9–1.4e-4 cm⁻³（2σ，随 FXT 径向标定与发射率转换而变）；最佳值 5.8–6.7e-5 不是探测。原 2σ 上限 8.6e-5 在 FXT 公共模径向残差（仍被 PN/FXT 斜率 −0.15 ± 0.24 PW/arcmin、最大 +0.34 在 2σ 内允许）下升至 1.43e-4 —— 恰为平衡密度。发射率转换：0.2 keV（非 0.3 keV）使 n_H ×1.16–1.17（最佳 6.7e-5、上限 1.0e-4、0.2 keV 处 P 4.9e-14）；Z 0.1–1 使 n_H ×1.73–0.68（C5 已知告警，现已量化）。β 0.2 / r_c 64′（350 kpc）给 1.43e-4 但不可信（次要；r_c ≤ 8′、β ≥ 0.35 时 8.9e-5）。PN-only XMM 独立给出 2σ ≤ 5.1–12.1e-5。能把壁压平衡掉的晕（nH ≈ 1.4e-4）预测 S(8′)−S(22′) = 4.1–5.3 PW，而 FXT 60′ 实测 −0.1 ± 1.4 PW —— 在两侧情形中被排除，但公共模残差路径（RT-08，在跑）仍待测。
LIMIT (2026-10-15 RT-05 triage; was MEASURED, model-dependent) The major-axis brightness gradient (sectors within ±30° of PA 165/345, 1′ rings) gives the centred hot halo: the halo is not detected — the FXT 60′ amplitude is only 1.63σ and PN alone is −0.33σ. Quote the limit: at 47 kpc n_H < 0.9–1.4e-4 cm⁻³ (2σ, depending on the FXT radial calibration and the emissivity conversion); the best value 5.8–6.7e-5 is not a detection. The former 2σ upper 8.6e-5 rises to 1.43e-4 — the balance density — under an FXT common-mode radial residual still allowed at 2σ by the PN/FXT slope (−0.15 ± 0.24 PW/arcmin, max +0.34). Emissivity conversion: 0.2 keV (not 0.3 keV) multiplies n_H by 1.16–1.17 (best 6.7e-5, upper 1.0e-4, P 4.9e-14 at 0.2 keV); Z 0.1–1 multiplies n_H by 1.73–0.68 (a known C5 caveat, now quantified). β 0.2 / r_c 64′ (350 kpc) gives 1.43e-4 but is implausible (minor; r_c ≤ 8′, β ≥ 0.35 gives 8.9e-5). PN-only XMM independently gives 2σ ≤ 5.1–12.1e-5. A halo dense enough to balance the walls (nH ≈ 1.4e-4) predicts S(8′)−S(22′) = 4.1–5.3 PW against the measured FXT 60′ value of −0.1 ± 1.4 PW — excluded in the two-sided cases, but the common-mode residual route (RT-08, running) is still untested.
来源Source: I021 L12 (RT-05 triage 2026-10-15); REDTEAM_QUEUE.md RT-05; cognition-os/experiments/E084_s09_halo_limit_robustness.md; XMMLineMap E091; P2 REPORT.sol.md
3.10 壁超压 P_wall/P_halo（L13）与 C2 重标定 —— 条件于 FXT 径向标定Wall over-pressure P_wall/P_halo (L13) and the C2 rescaling — conditional on the FXT radial calibration
CONDITIONAL（2026-10-15 RT-05 后果；原 MEASURED 由 L12）壁压力 P_wall = 2.3 nH_wall kT（nH_wall 由发射率、固定波段转换；kT 由 §3.7 表）。在壁的三维半径（3-d radius）r = √(z² + w_c²) 处对局部晕比较：在最佳拟合晕处 WSW P_wall/P_halo = 2.95 ± 0.84（1σ；含 28% 晕水平误差 E091，kT_halo 取 0.2 keV；q ∝ 0.2 keV/kT_halo）—— ± 0.16 只是壁归一化误差。ENE 依图与壁厚模型族为 2.6–3.6。"随高度持平"依赖 e098a 的 z > 14 kpc 截断：纳入 13.8 kpc bin 后 q = 3.49、斜率 −0.30 ± 0.07。RT-05 后果（Claude 算术，未重跑）：q ∝ 1/P_halo；用一致的 0.2 keV 发射率（n_H ×1.16）时 q 2.95 → ~2.55；若 FXT 公共模 2σ 上限（1.43e-4）替换 8.6e-5，最不利叠加从 1.41 降到 ~0.85 —— 在所有 2σ 系统学下超压并无保证。条件："在最佳拟合晕处超压"；状态 CONDITIONAL 于 FXT 径向标定。联合 PN 图独立分支：WSW 2.7（< 38 kpc）/ 2.3（> 38 kpc），与 FXT 60′ 一致。C2 重标定（固定密度）：kT_new/kT_old = 0.97（WSW 41–61 kpc）与 1.09（ENE），故 WSW 2.95 → 2.87、ENE 2.6 → 2.83。38–40 kpc 处无压力跳变。P2 静力学范围：16 个 HSE 晕模型给出 WSW 平均 q = 2.16–3.78（永不接近 1），但斜率 −0.45 到 +0.60 —— "随高度持平"在模型族间脆弱。
CONDITIONAL (2026-10-15 RT-05 consequence; was MEASURED from L12) The wall pressure is P_wall = 2.3 nH_wall kT (nH_wall from the emissivity at a fixed band conversion; kT from the §3.7 table). Compared against the local halo at the wall's 3-d radius r = √(z² + w_c²): at the best-fit halo WSW P_wall/P_halo = 2.95 ± 0.84 (1σ; including the 28% halo-level error from E091, with kT_halo at 0.2 keV; q ∝ 0.2 keV/kT_halo) — ±0.16 is the wall-normalisation error only. ENE is 2.6–3.6 depending on the map and wall-thickness family. "Flat with height" depends on the e098a z > 14 kpc cut: including the 13.8 kpc bin gives q = 3.49 and slope −0.30 ± 0.07. RT-05 consequence (Claude arithmetic, not re-run): q scales as 1/P_halo; with a consistent 0.2 keV emissivity (n_H ×1.16) q goes 2.95 → ~2.55; if the FXT common-mode 2σ upper (1.43e-4) replaces 8.6e-5, the hostile stack drops from 1.41 to ~0.85 — over-pressure is not guaranteed under all 2σ systematics. Conditional wording: "over-pressured at the best-fit halo"; status CONDITIONAL on the FXT radial calibration. The independent joint-PN branch gives WSW 2.7 (below 38 kpc) / 2.3 (above 38 kpc), consistent with FXT 60′. C2 rescaling (fixed density): kT_new/kT_old = 0.97 (WSW 41–61 kpc) and 1.09 (ENE), so WSW 2.95 → 2.87 and ENE 2.6 → 2.83. No pressure jump at 38–40 kpc. P2 hydrostatic range: 16 HSE halo models give a WSW mean q = 2.16–3.78 (never near 1), but slopes from −0.45 to +0.60 — "flat with height" is fragile across model families.
来源Source: XMMLineMap E096 §a, E098a; REPORT.hermes.md Table 3; P2 REPORT.sol.md (HSE grid); artifacts/s09_e087_joint_pn/PN/e096_wall_profile.json
3.11 质量与能量收支（L14、L17；L16 条件性）Mass and energy budgets (L14, L17; L16 conditional)
INFERRED（填充因子 f = 1；2026-10-15 RT-07 分诊后措辞）可见的现今风（HK2020 的 X 射线可见高纬成分：到 ~21.5 kpc 的箱，Ṁ < 0.19 M⊙/yr、L_kin < 1.35e40 erg/s、v 475–570 km/s；不是总风 —— 隐藏的快脊柱未被约束）在流动时间内供给 WSW 壁热能的 1/7–1/14（稳健能量亏缺 ×6.9–14；FXT ENE 38–80 kpc 的 ×34 用了窗口受限的几何，E096）。壁质量可以是被扫积的晕气体（壁/扫积比 1.8–2.2；体积填充 f_v 0.22–0.29 时相等），故质量亏缺条件于"喷出物"假设。WSW 壁 14–38 kpc 质量 2.5–3.7e8 M⊙、热能 3–4e56 erg；38–80 kpc 质量 5.2–6.4e8 M⊙、E_th 5e56 erg；ENE 相近。星暴机械功率（~8e41 erg/s）可在 30–40 Myr 内供上能量。INFERRED L17：L_X(0.5–2 keV, 14–80 kpc) ≈ 2e39 erg/s ≈ SN 功率的 0.25%（快照比值）。CONDITIONAL L16：光滑壁（热支撑）把 47 kpc 总晕压限制在 ≲ 3 P_X；类似 NGC 4594 的隐藏热相（f_X = 5e-3）需要 f_w ≤ 0.04。标度：质量与能量 ∝ √(f_v) √(L0/L) √(Λ0/Λ)（能量还 × kT）；全部能量 ∝ P_halo(47 kpc)/4.1e-14。
INFERRED (filling factor f = 1; wording after the 2026-10-15 RT-07 triage) The visible present wind (HK2020's X-ray-visible high-latitude component: boxes to ~21.5 kpc, Ṁ < 0.19 M⊙/yr, L_kin < 1.35e40 erg/s, v 475–570 km/s; not the total wind — a hidden fast spine is not bounded) supplies 1/7–1/14 of the WSW wall thermal energy over the flow time (robust energy deficit ×6.9–14; the ×34 for the FXT ENE 38–80 kpc uses window-limited geometry, E096). The wall mass can be swept-up halo gas (wall/swept 1.8–2.2; equal at volume filling f_v 0.22–0.29), so the mass deficit is conditional on ejecta. WSW walls 14–38 kpc: mass 2.5–3.7e8 M⊙, thermal energy 3–4e56 erg; 38–80 kpc: 5.2–6.4e8 M⊙, E_th 5e56 erg; ENE similar. The starburst mechanical power (~8e41 erg/s) would supply the energy in 30–40 Myr. INFERRED L17: L_X(0.5–2 keV, 14–80 kpc) ≈ 2e39 erg/s ≈ 0.25% of the SN power (a snapshot ratio). CONDITIONAL L16: smooth, thermally supported walls limit the total halo pressure at 47 kpc to ≲ 3 P_X; an NGC 4594-like hidden hot phase (f_X = 5e-3) needs f_w ≤ 0.04. Scalings: mass and energy ∝ √(f_v) √(L0/L) √(Λ0/Λ) (energy also × kT); all energies ∝ P_halo(47 kpc)/4.1e-14.
| WSW 壁WSW walls | 14–38 kpc | 38–80 kpc |
|---|---|---|
| 质量（f = 1）Mass (f = 1) | 2.5–3.7e8 M⊙ | 5.2–6.4e8 M⊙ |
| E_th | 3–4e56 erg | 5e56 erg |
| 可见现今风供给质量需时Time for the visible present wind to supply the mass | 1.4–2.0 Gyr | 2.8–3.4 Gyr |
| ……供给能量需时（能量亏缺 ×6.9–14）…to supply the energy (deficit ×6.9–14) | 0.7–1.0 Gyr | 1.1–1.3 Gyr |
| 500 km/s 流动时间Flow time at 500 km/s | 74 Myr | 156 Myr |
来源Source: I021 L14/L17 (RT-07 triage 2026-10-15); REDTEAM_QUEUE.md RT-07; XMMLineMap E096 §b; E098a; S09 FACTS (budgets); HK2020 = Hodges-Kluck et al. 2020, ApJ 903, 35
3.12 候选与非探测（L18–L21），伴星系效应与撤回清单Candidates and non-detections (L18–L21), companion effects, and the withdrawn list
MEASURED / INFERREDL18 前向激波鞘：forward-shock sheath: 既未探测也未被排除。双成分上限为预测的 1.36–10×；SHE 孔径被冷的（0.14–0.21 keV）壁裙气体主导；WSW 14–28 kpc 软超出不具全局显著性（p 0.27–0.45）。检验需约 2× 灵敏度。Neither detected nor excluded. Two-component bounds are 1.36–10× the prediction; the SHE aperture is dominated by cool (0.14–0.21 keV) wall-skirt gas; the WSW 14–28 kpc soft excess is not globally significant (p 0.27–0.45). A test needs about 2× more sensitivity.MEASUREDL19： WSW 14–28 kpc 软超出不具全局显著性（相关噪声下全局 p 0.27–0.45）。The WSW 14–28 kpc soft excess is not globally significant (global p 0.27–0.45 with correlated noise).CANDIDATEL20： FXT 宽场小轴超出到 ~110 kpc 与 92–107 kpc 的三个 blob —— 仅候选，需 C4 的全局空假设重做。The FXT wide-field minor-axis excess to ~110 kpc and three blobs at 92–107 kpc — candidates only; the global nulls must be redone (C4).CANDIDATEL21： PN-only XMM 在 55–66 kpc 轴上 C = +2.8 ± 1.0，FXT +0.6 ± 0.8（仪器间 ~2σ 不一致）；通过 C12 检验前不入论文。PN-only XMM shows axis emission at 55–66 kpc, C = +2.8 ± 1.0, against FXT +0.6 ± 0.8 (a ~2σ instrument disagreement); it stays out of the paper until the C12 checks pass.MEASURED伴星系 MCG 9-17-9（P5）：The companion MCG 9-17-9 (P5): 位置 (maj, mnr) = (−3.83′, −5.36′)，r 6.59′（36.5 kpc），距 WSW 轴 35.5°；是物理伴星（Δv 173–192 km/s，33 kpc HI 桥）。其点源已被扣除（XMM #5，40″ 掩罩）。L7 壁超出 B（7–10′）随 1/1.5/2′ 掩罩变化 −0.03/+0.10/−0.05 PW；烟囱边缘（z 6–7′）不动（w 6.10′ → 6.10/6.20/6.20′）。但 E095/E096 的 WWLM 谱区（WSW 壁 28–39 kpc）有 5%/18%/29% 像素在它 1′/1.5′/2′ 内；其周围 1–3′ 有 +1.4–1.7 PW 的微弱超出（~2σ_null）—— WWLM 的 kT/O/Fe 条件性暴露，需 2′ 掩罩重拟（C2 后续）。Position (maj, mnr) = (−3.83′, −5.36′), r 6.59′ (36.5 kpc), 35.5° from the WSW axis; a physical companion (Δv 173–192 km/s, a 33 kpc HI bridge). Its point source is subtracted (XMM #5, 40″ mask). The L7 wall excess B (7–10′) changes by −0.03/+0.10/−0.05 PW for 1/1.5/2′ masks; the chimney edge (z 6–7′) does not move (w 6.10′ → 6.10/6.20/6.20′). But 5%/18%/29% of the WWLM spectral region (WSW wall 28–39 kpc, E095/E096) lies within 1′/1.5′/2′ of it, and a faint +1.4–1.7 PW excess at 1–3′ sits at ~2σ_null — the WWLM kT/O/Fe are conditionally exposed and need a 2′-mask refit (C2 follow-up).WITHDRAWN撤回清单（不要引用）：Withdrawn list (do not cite): 壁到 60–70 kpc（E077/I029 旧表述）；ENE 填满锥到 39 kpc（是星系团）；E095 "epoch 按高度分裂"；E096 用高度 z 处晕算的超压；E098b 鞘排除；E098b-d 的 OUT:BG 温度诊断（孔径重叠）；I030 的 "filled cone to ~39 kpc"。walls to 60–70 kpc (the old E077/I029 wording); the filled ENE cone to 39 kpc (the cluster); E095's "epochs split in height"; E096's over-pressure at height z; the E098b sheath exclusion; the OUT:BG temperature diagnostics of E098b-d (overlapping apertures); I030's "filled cone to ~39 kpc".
来源Source: I021 (L18–L21, withdrawn list); XMMLineMap E098c–e, E098d; E086 (L21); P5 REPORT.sonnet.md