{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:3KYFHT3L7EDHQKMJKIOVZAQGSJ","short_pith_number":"pith:3KYFHT3L","schema_version":"1.0","canonical_sha256":"dab053cf6bf906782989521d5c82069270cf1e4112c921eb6730f100255bcda4","source":{"kind":"arxiv","id":"2402.06449","version":1},"attestation_state":"computed","paper":{"title":"The EBLM project -- XIII. The absolute dynamical masses of the circumbinary planet host TOI-1338/BEBOP-1","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"A. H.M.J. Triaud, D. Sebastian, D. V. Martin, L. Sairam, M. B. Nielsen, M. Brogi, M. R. Standing, P. F.L. Maxted, T. A. Baycroft","submitted_at":"2024-02-09T14:51:25Z","abstract_excerpt":"High-contrast eclipsing binaries with low mass M-dwarf secondaries are precise benchmark stars to build empirical mass-radius relationships for fully convective low-mass ($\\rm M_{*} < 0.35\\,M_{\\rm sun}$) dwarf stars. The contributed light of the M-dwarf in such binaries is usually much less than one~per~cent at optical wavelengths. This enables the detection of circumbinary planets from precise radial velocity measurements. High-resolution cross-correlation techniques are typically used to detect exoplanet atmospheres. One key aspect of these techniques is the post-processing, which includes t"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"2402.06449","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2024-02-09T14:51:25Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"26b121610e2bf6b56af9d12e842e692f007aaa69a7ff03decabe3834094a130c","abstract_canon_sha256":"6f87a8b57622e4b53d029f1ceb68e08b62f1c95dda9abacbfa71dbbea83d344a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:43:24.671741Z","signature_b64":"p1Ua9zdVo4ntwe9cpzp4CIqL3u5hggYYMaqLhQPl0Ll9xdqe0WhM+LibZF88M/sb1tjaJYfFPpT5gBBRWVluAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"dab053cf6bf906782989521d5c82069270cf1e4112c921eb6730f100255bcda4","last_reissued_at":"2026-07-05T07:43:24.671354Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:43:24.671354Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The EBLM project -- XIII. The absolute dynamical masses of the circumbinary planet host TOI-1338/BEBOP-1","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.EP","authors_text":"A. H.M.J. Triaud, D. Sebastian, D. V. Martin, L. Sairam, M. B. Nielsen, M. Brogi, M. R. Standing, P. F.L. Maxted, T. A. Baycroft","submitted_at":"2024-02-09T14:51:25Z","abstract_excerpt":"High-contrast eclipsing binaries with low mass M-dwarf secondaries are precise benchmark stars to build empirical mass-radius relationships for fully convective low-mass ($\\rm M_{*} < 0.35\\,M_{\\rm sun}$) dwarf stars. The contributed light of the M-dwarf in such binaries is usually much less than one~per~cent at optical wavelengths. This enables the detection of circumbinary planets from precise radial velocity measurements. High-resolution cross-correlation techniques are typically used to detect exoplanet atmospheres. One key aspect of these techniques is the post-processing, which includes t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2402.06449","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2402.06449/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"2402.06449","created_at":"2026-07-05T07:43:24.671417+00:00"},{"alias_kind":"arxiv_version","alias_value":"2402.06449v1","created_at":"2026-07-05T07:43:24.671417+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2402.06449","created_at":"2026-07-05T07:43:24.671417+00:00"},{"alias_kind":"pith_short_12","alias_value":"3KYFHT3L7EDH","created_at":"2026-07-05T07:43:24.671417+00:00"},{"alias_kind":"pith_short_16","alias_value":"3KYFHT3L7EDHQKMJ","created_at":"2026-07-05T07:43:24.671417+00:00"},{"alias_kind":"pith_short_8","alias_value":"3KYFHT3L","created_at":"2026-07-05T07:43:24.671417+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/3KYFHT3L7EDHQKMJKIOVZAQGSJ","json":"https://pith.science/pith/3KYFHT3L7EDHQKMJKIOVZAQGSJ.json","graph_json":"https://pith.science/api/pith-number/3KYFHT3L7EDHQKMJKIOVZAQGSJ/graph.json","events_json":"https://pith.science/api/pith-number/3KYFHT3L7EDHQKMJKIOVZAQGSJ/events.json","paper":"https://pith.science/paper/3KYFHT3L"},"agent_actions":{"view_html":"https://pith.science/pith/3KYFHT3L7EDHQKMJKIOVZAQGSJ","download_json":"https://pith.science/pith/3KYFHT3L7EDHQKMJKIOVZAQGSJ.json","view_paper":"https://pith.science/paper/3KYFHT3L","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2402.06449&json=true","fetch_graph":"https://pith.science/api/pith-number/3KYFHT3L7EDHQKMJKIOVZAQGSJ/graph.json","fetch_events":"https://pith.science/api/pith-number/3KYFHT3L7EDHQKMJKIOVZAQGSJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3KYFHT3L7EDHQKMJKIOVZAQGSJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3KYFHT3L7EDHQKMJKIOVZAQGSJ/action/storage_attestation","attest_author":"https://pith.science/pith/3KYFHT3L7EDHQKMJKIOVZAQGSJ/action/author_attestation","sign_citation":"https://pith.science/pith/3KYFHT3L7EDHQKMJKIOVZAQGSJ/action/citation_signature","submit_replication":"https://pith.science/pith/3KYFHT3L7EDHQKMJKIOVZAQGSJ/action/replication_record"}},"created_at":"2026-07-05T07:43:24.671417+00:00","updated_at":"2026-07-05T07:43:24.671417+00:00"}