GROUP MEETING · 2026-07-24
XMM Proposal Agent · internal research system · static snapshot 2026-07-23
Then search for evidence that supports it; archive duplication and published work are often discovered only at the end.
Proposing, retrieving evidence, writing, and judging are mixed in one context, inviting attachment.
Count rate, background, pile-up, and systematics surface only late in the draft.
It must leave behind sources, evidence, rebuttals, unresolved gates, a feasibility chain, state transitions, and an owner for the next step.
The goal is not “generate more ideas,” but eliminate ideas unworthy of further investment faster and more honestly.
Narrative first; failure often arrives too late.
Evidence first; failure is retained as reusable knowledge.
pipeline/*.md defines what each role can and cannot do; roles change rarely.
Coverage matrix, TRUST_TABLE, idea ledger, decision log, and graveyard.
Per-cycle materials, critiques, rebuttals, calculations, and SHIFTS handoffs.
Downstream roles receive an artifact + handoff, not an upstream agent’s long context.
No qualifying new input → STAGNATION (record it and stop; do not idle-burn).
Create a versioned run from a proposal-ready idea.
ObsID-level archive, duplication, and instrument facts.
Model → rate → pile-up → background → exposure.
Write only within the scope already closed by evidence and feasibility.
Three heterogeneous reviewers; any poor dimension triggers revision / park.
A poor result on any axis blocks promotion; a high average cannot conceal one fatal weak axis.
Use roughly 20 years of XMM + Chandra archives to search for temporal changes in the diffuse M82 superwind, and connect them to the central engine.
On the surface: deep archive, multiple epochs, a writable story.
R0: NGC 891 is a canonical edge-on hot halo; archive coverage appeared to leave room for a new halo-offset observation.
R2: Proposed new XMM halo mapping.
R1/R4: Examined the literature and existing observations in depth.
Hodges-Kluck, Bregman & Li 2018 already carried out the same measurement: an in-depth XMM/Chandra decomposition of the NGC 891 hot halo.
Not a “similar paper,” but the same measurement already published.
Retain I038’s surviving fifth target cell, but use Chandra-defined masks, independent (not joint) fits, preregistered nested models, a model-selection threshold, and a net-count floor.
Question: In mirror-matched sectors, can the SE/NW thermal-pressure ratio be distinguished from 1?
Observation: A ~110 ks XMM SE offset, paired with the existing NW 0723220101 (109.5 ks).
Scientific value: Pressure P = nekT drives wind dynamics; symmetry versus asymmetry distinguishes whether disk–halo feedback is uniform or directionally injected.
LIGHT / MEDIUM shifts: M0/R0/R1/R2/R4/R5/R6-lite/L
Actual archive extraction, SAS/ESAS, R6-full, simulation, and σsys
.runtime/, the Virgo workspace, and the result inboxTAKE-HOME
Use archive facts, literature, and gates to separate opportunities from wishes.
Give an independent red-team responsibility for killing bad questions, and make each kill reason a reusable constraint.
Make even the strongest idea retain its blocking evidence; Elo ranking does not pass a min-gate.
Make HEAVY execution serve only questions that can genuinely unlock a state transition.
Canonical records: pipeline/ · shared/ideas/ · TRUST_TABLE · cycles/ · cognition-os/