NGC 3079 热风手册（S09）NGC 3079 hot-wind handbook (S09)

评审更正（2026-10-15，Claude）：本页写于红队核查之前，以下结论已更新，以此为准：（1）L7：墙测到约 55 kpc（39–55 kpc 的超出 B = 2.48 ± 0.43 PW，计入估计量系统误差后 3.8–4.8σ）；55–66 kpc 的延伸改为 CANDIDATE，计入估计量与掩膜系统误差后为 2.0–2.9σ；66 kpc 以外为上限 B < 0.75 PW（95%，仅统计误差）。（2）L9：锥形下缘在约 40 kpc 转为宽度近乎不变的上部结构（MEASURED）；三维“空心烟囱”改为 INFERRED（非轴对称“两片墙”模型同样好），转折高度 1σ 范围 26–43 kpc（联合图），“空心”仅约 2σ。（3）L13：计入晕密度 28% 误差后 P_wall/P_halo = 2.95 ± 0.84（kT_halo = 0.2 keV，∝ 0.2 keV/kT_halo）；“不随高度变化”依赖 z > 14 kpc 截断；最不利的假设组合仍给 1.41 > 1。（4）图 fig_wall_profile 的晕压参考线已改正（原画在 10 倍处）。下一版手册将把这些改动写入正文。

Review correction (2026-10-15, Claude): this page was written before the red-team checks. These updates override the text below: (1) L7: walls are detected to about 55 kpc (39-55 kpc excess B = 2.48 +- 0.43 PW, 3.8-4.8 sigma with the estimator systematic); the 55-66 kpc extension is now CANDIDATE, 2.0-2.9 sigma with the estimator and mask systematics; beyond 66 kpc there is a limit, B < 0.75 PW (95%, statistical only). (2) L9: the cone-like lower edge turns into a near-constant-width upper structure at about 40 kpc (MEASURED); the 3-D "hollow chimney" is now INFERRED (a non-axisymmetric two-sheet model fits as well); the break height is 26-43 kpc at 1 sigma (joint map); "hollow" is only about 2 sigma. (3) L13: with the 28% halo-density error, P_wall/P_halo = 2.95 +- 0.84 (kT_halo = 0.2 keV; scales as 0.2 keV/kT_halo); "flat with height" depends on the z > 14 kpc cut; the most hostile set of assumptions still gives 1.41 > 1. (4) The halo reference line in fig_wall_profile is corrected (it was drawn 10x too high). The next version will put these changes into the text.

来源：cognition-os/REDTEAM_QUEUE.md（RT-01、RT-02、RT-03、RT-06）；I021 L7、L9、L13 的 2026-10-15 注记

Source: cognition-os/REDTEAM_QUEUE.md (RT-01, RT-02, RT-03, RT-06); I021 L7, L9, L13 notes of 2026-10-15

项目一句话The project in one paragraph

NGC 3079 是一个侧向（edge-on）星暴星系（D = 19 Mpc，1′ = 5.53 kpc）。S09 阶段用 10 个重新处理的 XMM-Newton 指向、86 个 Einstein Probe FXT 指向和 Chandra 源普查研究它的热气体外流：沿径向抽取 0.3 keV 等离子体（APEC）面亮度图与分区光谱，测到一对 X 形双极风的"壁"到 ~66 kpc、WSW 锥在 36–41 kpc 处变成烟囱（chimney）、90 kpc 内无"帽"（cap）、壁相对测量到的热晕超压约 3 倍，且质量与能量远超现今星暴风所能供给 —— 一个更早、更强爆发期的遗迹。本页给出可发表结果的当前状态（截至 2026-10-15）。

NGC 3079 is an edge-on starburst galaxy (D = 19 Mpc, 1′ = 5.53 kpc). Stage S09 studies its hot-gas outflow with 10 reprocessed XMM-Newton pointings, 86 Einstein Probe FXT pointings and a Chandra source census: radial 0.3 keV plasma (APEC) surface-brightness maps and zoned spectra find the walls of an X-shaped bipolar wind to ~66 kpc, a WSW cone that becomes a chimney at 36–41 kpc, no cap within 90 kpc, walls over-pressured by about 3× against the measured hot halo, and mass and energy far beyond what the present starburst wind can supply — a relic of an earlier, stronger episode. This page gives the current state of the publishable results (as of 2026-10-15).

来源Source: cognition-os/insights/I021_s09_paper_plan_v2.md; .agent/jobs/2026-10-15-S09-FACTS.md

骨架图Skeleton

来源Source: I021_s09_paper_plan_v2.md (papers, checks C1–C12)

目标表（O1–O4）Objectives (O1–O4)

目标Objective	状态与当前最佳数字（含来源）Status and best current number (with source)	趋势Trend
O1 论文 I：热外流到 66 kpc —— 壁、烟囱、无帽、超压遗迹Paper I: the hot outflow to 66 kpc — walls, a chimney, no cap, an over-pressured relic `L1–L10, L12–L14, L17; gates C1, C3–C5, C7, C9–C10 open; C2 done 2026-10-15`	`MEASURED` 壁到 66 kpc（联合 PN+FXT：39–55 kpc B = 2.48 ± 0.43 PW，5.8σ；55–66 kpc 2.09 ± 0.67，3.1σ；55–66 kpc 为合并径向 bin，非端点）。超压 WSW 2.95 ± 0.16（3-d 半径）→ C2 重标定后 2.87。Walls to 66 kpc (joint PN+FXT: B = 2.48 ± 0.43 PW at 39–55 kpc, 5.8σ; 2.09 ± 0.67 at 55–66 kpc, 3.1σ; the 55–66 kpc bin is pooled, not an endpoint). Over-pressure WSW 2.95 ± 0.16 (3-d radius) → 2.87 after the C2 rescaling. 来源Source: `cognition-os/artifacts/s09_e086_l7_l8_pn/redo_l7_l8.json; .agent/jobs/2026-10-15-c2-outer-spectra-pn-fxt/REPORT.hermes.md Table 3`	↗ C2 完成后更稳↗ firmer after C2
O2 论文 II：径向 O/Fe（与 Liu et al. 2026 团队）Paper II: radial O/Fe (with the Liu et al. 2026 team) `L11; gates C2 done, C5, C6`	`MEASURED (relative)` 1T O/Fe：17–28 kpc 壁 8.26 → C2 PN+FXT 6.81（太阳仍被排除，dC(1) +5.4）；pooled 28–61 kpc 4.87 → 6.33。合并似然区间未校准（每 ON 区重复计一次 BG，e079_fit.py:220）。1T O/Fe: walls 17–28 kpc 8.26 → 6.81 with C2 PN+FXT (solar still rejected, dC(1) +5.4); pooled 28–61 kpc walls 4.87 → 6.33. Pooled-likelihood intervals are uncalibrated (BG counted once per ON region, e079_fit.py:220). 来源Source: `REPORT.hermes.md Table 2; session 2026-10-15.md (R1 astra)`	→ 待 C5/C6→ awaiting C5/C6
O3 物理解释（遗迹弱激波、能量来源、化学）Physical interpretation (relic weak shock, energy source, chemistry) `L15, L16; P1/P2/P4/L1/L2/A1 (2026-10-15)`	`INFERRED` 弱激波 Mach ~1.5–1.6（由 q 推定，非测量）。A1 审计：100 Myr 情景每瓣 E0 = 3.40–4.94e57 erg、注入功率 1.08–1.57e42 erg/s（两瓣为 SN 功率的 2.7–3.9×）；7–9e41 是对整个泡龄（151–176 Myr）的平均功率。全部能量 ∝ P_halo(47 kpc)/4.1e-14。Weak shock Mach ~1.5–1.6 (inferred from q, not measured). A1 audit: for the 100 Myr episode E0 = 3.40–4.94e57 erg per lobe and injection power 1.08–1.57e42 erg/s (2.7–3.9× the SN power for two lobes); 7–9e41 is the power averaged over the full 151–176 Myr bubble age. All energies scale as P_halo(47 kpc)/4.1e-14. 来源Source: `.agent/jobs/2026-10-15-e098a-energy-audit/REPORT.sol.md; E098 record`	→ 讨论级→ discussion level
O4 技术短文：EP-FXT 软弥漫辐射（可选）Technical note: EP-FXT soft diffuse emission (optional) `L2, L2b, L3, E084-B; gate C10`	`OPTIONAL` FXTDAS/CALDB v1.30 点源谱与 XMM 一致到 0–10%（0.4–1 keV）；MOS 卷帘梯度与 MOS1 CCD4 软超出已表征。非首篇 EP-FXT 弥漫辐射文章（Tang et al. 2026, Abell 1795）。FXTDAS/CALDB v1.30 point-source spectra match XMM to 0–10% at 0.4–1 keV; the MOS roll-dependent gradient and the MOS1 CCD4 soft excess are characterised. Not the first EP-FXT diffuse paper (Tang et al. 2026, Abell 1795). 来源Source: `I021 (technical note); E084; S09 E085`	→ 可选→ optional

未决问题表Open problems

问题Problem	为何重要Why it matters	最佳假设Best hypothesis	下一步检验Next test	负责Owner	状态Status
合并 on-off 似然把 BG 每 ON 区计一次Pooled on-off likelihood counts BG once per ON region	pooled kT/O/Fe 区间（E096 §d、C2 pooled）未校准pooled kT/O/Fe intervals (E096 §d, C2 pooled) are uncalibrated	复合似然，偏差方向未知composite likelihood, bias direction unknown	在引擎副本中改为每相机一个共享 BG 项并重拟 E096 pooled O/Fefix one shared BG term per camera in an engine copy and refit the E096 pooled O/Fe	`e079_fit.py:220; session 2026-10-15 NEXT`	`OPEN`
E098a 注入功率 vs 平均功率措辞E098a injection vs mean power wording	L15 的能量叙事；页 v10 面板 P 数字错误the L15 energy narrative; page v10 panel P numbers are wrong	A1 已给出正确措辞（未应用到记录）A1 supplies the correct wording (not yet applied to the record)	修 E098 行 61 与 I021 L15fix E098 line 61 and I021 L15	`A1 · REPORT.sol.md`	`OPEN`
WWLM 谱区受 MCG 9-17-9 影响WWLM spectral region exposed to MCG 9-17-9	28–39 kpc WSW 壁 kT/O/Fe（该区 18–30% 像素在伴星系 1.5–2′ 内）the 28–39 kpc WSW wall kT/O/Fe (18–30% of its pixels lie within 1.5–2′ of the companion)	P5：L7 与烟囱边缘不受影响；+1.4–1.7 PW 超出仅 ~2σ_nullP5: L7 and the chimney edge are unaffected; the +1.4–1.7 PW excess is only ~2σ_null	用 2′ MCG 掩罩重拟 WWLMrefit WWLM with a 2′ MCG mask	`P5 (REPORT.sonnet.md); C2 follow-up`	`OPEN`
红队 RT-01 / RT-02 在跑Red teams RT-01 / RT-02 running	L7 端点、L13 压力误差的独立复核independent re-checks of the L7 endpoint and the L13 pressure error	——	等待报告await the reports	`.agent/jobs/2026-10-15-redteam-rt01-l7-extent, -rt02-l13-pressure`	待定Pending
最终图集（C1）与端点系统学（C3）Final map set (C1) and extent systematics (C3)	论文 I 图 1–4 的口径统一；PSF 翼、FXT 渐晕、CXB 方差one consistent set for Paper I figures 1–4; PSF wings, FXT vignetting, CXB variance	PN+FXT 联合图为基准the PN+FXT joint map is the baseline	按 I021 C1/C3 重建rebuild per I021 C1/C3	`I021 C1, C3`	`OPEN`
晕锚（C7）：FXT 公共模渐晕未测Halo anchor (C7): common-mode FXT vignetting untested	L13–L17 全部随 P_halo(47 kpc) 缩放L13–L17 all scale with P_halo(47 kpc)	两台 FXT 模块一致、PN-only XMM 独立排除平衡晕both FXT modules agree; PN-only XMM excludes the balance halo independently	FXT 空白场/团场检验（只读）an FXT blank/cluster-field test (read-only)	`I021 C7; E084`	`OPEN`
L21 轴候选（PN 55–66 kpc）L21 axis candidate (PN 55–66 kpc)	PN C = +2.8 ± 1.0，FXT +0.6 ± 0.8，仪器间 ~2σ 不一致PN C = +2.8 ± 1.0, FXT +0.6 ± 0.8, a ~2σ instrument disagreement	候选，未确认candidate, unconfirmed	PN N/S 组、FXT A/B、一个谱检验（C12）PN N/S groups, FXT A/B, a spectral test (C12)	`E086; I021 C12`	`CANDIDATE`

未来 1–4 周计划（按 I021 与 session 2026-10-15）Plan for the next 1–4 weeks (per I021 and session 2026-10-15)

C2 已完成（2026-10-15）。把 PN+FXT 的 kT 与 O/Fe 更新到页 v10 面板 D/P，并采用 A1 的能量措辞。C2 is done (2026-10-15). Update page v10 panels D/P with the PN+FXT kT and O/Fe, and adopt the A1 energy wording.
修 E098 行 61 措辞与 I021 L15（按 A1）；改正页 v10 面板 P 数字。Fix the E098 line-61 wording and I021 L15 (per A1); correct the page v10 panel P numbers.
用 2′ MCG 9-17-9 掩罩重拟 WWLM（C2 后续）。Refit WWLM with a 2′ MCG 9-17-9 mask (C2 follow-up).
在引擎副本中修复合并 on-off 似然（每相机一个共享 BG 项），并重拟 E096 pooled O/Fe 作比较；在此之前 L11 pooled 区间保持 PROVISIONAL/未校准。Fix the pooled on-off likelihood in an engine copy (one shared BG term per camera) and refit the E096 pooled O/Fe once for comparison; until then L11 pooled intervals stay PROVISIONAL/uncalibrated.
C1 + C3（图集与端点系统学），然后 C5、C7；C10 文献刷新后起草论文 I。C1 + C3 (map set and extent systematics), then C5, C7; draft Paper I after the C10 literature refresh.
C6 为论文 II（与 Liu et al. 团队，D2 之后）。C6 for Paper II (with the Liu et al. team, after D2).

本次更新What's new

日期Date	变更Change
2026-10-15	手册初建（H-N309-001）：§3 结果、§4 讨论、L1–L21 台账、§1/§2 占位。吸收 2026-10-15 的 C2（无 MOS2 外区谱）、P1 氧预算、P2 晕静力学、P4 NGC 3073、P5 MCG 9-17-9、A1 能量审计、R1 红队、L1 AGN vs 星暴、L2 混合层与 FUV 的结果。First handbook build (H-N309-001): §3 Results, §4 Discussion, the L1–L21 ledger, §1/§2 placeholders. It folds in the 2026-10-15 results: C2 (outer spectra without MOS2), P1 oxygen budget, P2 halo hydrostatics, P4 NGC 3073, P5 MCG 9-17-9, the A1 energy audit, the R1 red team, L1 AGN vs starburst, L2 mixing layers vs FUV.

日期Date

变更Change

2026-10-15

手册初建（H-N309-001）：§3 结果、§4 讨论、L1–L21 台账、§1/§2 占位。吸收 2026-10-15 的 C2（无 MOS2 外区谱）、P1 氧预算、P2 晕静力学、P4 NGC 3073、P5 MCG 9-17-9、A1 能量审计、R1 红队、L1 AGN vs 星暴、L2 混合层与 FUV 的结果。First handbook build (H-N309-001): §3 Results, §4 Discussion, the L1–L21 ledger, §1/§2 placeholders. It folds in the 2026-10-15 results: C2 (outer spectra without MOS2), P1 oxygen budget, P2 halo hydrostatics, P4 NGC 3073, P5 MCG 9-17-9, the A1 energy audit, the R1 red team, L1 AGN vs starburst, L2 mixing layers vs FUV.

数据截至Data as of: 2026-10-15T08:04Z （C2 报告完成；session 2026-10-15.md 最新条目 06:25Z）(C2 report complete; newest session 2026-10-15.md entry 06:25Z)