{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:KA75EPIU2FVUUPRN3QP4ICOR5H","short_pith_number":"pith:KA75EPIU","schema_version":"1.0","canonical_sha256":"503fd23d14d16b4a3e2ddc1fc409d1e9f4202589f4419ddaeb378bd4cb2f4dcd","source":{"kind":"arxiv","id":"1807.02568","version":1},"attestation_state":"computed","paper":{"title":"Interrelated Main-Sequence Mass-Luminosity, Mass-Radius and Mass-Effective Temperature Relations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"E. Soydugan, F. Alicavus, F. Soydugan, G. Aslan, H. Bakis, I. Steer, M. Alpsoy, S. Bilir, V. Bakis, Z. Eker","submitted_at":"2018-07-06T21:05:47Z","abstract_excerpt":"Absolute parameters of 509 main-sequence stars selected from the components of detached-eclipsing spectroscopic binaries in the Solar neighbourhood are used to study mass-luminosity, mass-radius and mass-effective temperature relations (MLR, MRR and MTR). The MLR function is found better if expressed by a six-piece classical MLR ($L \\propto M^{\\alpha}$) rather than a fifth or a sixth degree polynomial within the mass range of $0.179\\leq M/M_{\\odot}\\leq 31$. The break points separating the mass-ranges with classical MLR do not appear to us to be arbitrary. Instead, the data indicate abrupt chan"},"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":"1807.02568","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2018-07-06T21:05:47Z","cross_cats_sorted":[],"title_canon_sha256":"d1aad72e9346b58c7b4010c2db1edf68b626f8e19f7c0f505147e7dea918870b","abstract_canon_sha256":"97b80ae18cf03673a37d7525f12cdd7abf343a9226a323bd547f124dc6cb61cc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:08:38.311787Z","signature_b64":"JPwnlRIHesOWafZbyrA1v73io1pa746hGB9ReE0HHNHfv2Y9ERtYYrOh2S8B8zQ2o4VrTtgSBwMjj3DPdsAMDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"503fd23d14d16b4a3e2ddc1fc409d1e9f4202589f4419ddaeb378bd4cb2f4dcd","last_reissued_at":"2026-05-18T00:08:38.311141Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:08:38.311141Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Interrelated Main-Sequence Mass-Luminosity, Mass-Radius and Mass-Effective Temperature Relations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"E. Soydugan, F. Alicavus, F. Soydugan, G. Aslan, H. Bakis, I. Steer, M. Alpsoy, S. Bilir, V. Bakis, Z. Eker","submitted_at":"2018-07-06T21:05:47Z","abstract_excerpt":"Absolute parameters of 509 main-sequence stars selected from the components of detached-eclipsing spectroscopic binaries in the Solar neighbourhood are used to study mass-luminosity, mass-radius and mass-effective temperature relations (MLR, MRR and MTR). The MLR function is found better if expressed by a six-piece classical MLR ($L \\propto M^{\\alpha}$) rather than a fifth or a sixth degree polynomial within the mass range of $0.179\\leq M/M_{\\odot}\\leq 31$. The break points separating the mass-ranges with classical MLR do not appear to us to be arbitrary. Instead, the data indicate abrupt chan"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1807.02568","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":""},"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":"1807.02568","created_at":"2026-05-18T00:08:38.311230+00:00"},{"alias_kind":"arxiv_version","alias_value":"1807.02568v1","created_at":"2026-05-18T00:08:38.311230+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1807.02568","created_at":"2026-05-18T00:08:38.311230+00:00"},{"alias_kind":"pith_short_12","alias_value":"KA75EPIU2FVU","created_at":"2026-05-18T12:32:33.847187+00:00"},{"alias_kind":"pith_short_16","alias_value":"KA75EPIU2FVUUPRN","created_at":"2026-05-18T12:32:33.847187+00:00"},{"alias_kind":"pith_short_8","alias_value":"KA75EPIU","created_at":"2026-05-18T12:32:33.847187+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.19402","citing_title":"IZ Tel and UW Vir: Southern oscillating eclipsing Algol systems with active mass transfer","ref_index":86,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/KA75EPIU2FVUUPRN3QP4ICOR5H","json":"https://pith.science/pith/KA75EPIU2FVUUPRN3QP4ICOR5H.json","graph_json":"https://pith.science/api/pith-number/KA75EPIU2FVUUPRN3QP4ICOR5H/graph.json","events_json":"https://pith.science/api/pith-number/KA75EPIU2FVUUPRN3QP4ICOR5H/events.json","paper":"https://pith.science/paper/KA75EPIU"},"agent_actions":{"view_html":"https://pith.science/pith/KA75EPIU2FVUUPRN3QP4ICOR5H","download_json":"https://pith.science/pith/KA75EPIU2FVUUPRN3QP4ICOR5H.json","view_paper":"https://pith.science/paper/KA75EPIU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1807.02568&json=true","fetch_graph":"https://pith.science/api/pith-number/KA75EPIU2FVUUPRN3QP4ICOR5H/graph.json","fetch_events":"https://pith.science/api/pith-number/KA75EPIU2FVUUPRN3QP4ICOR5H/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KA75EPIU2FVUUPRN3QP4ICOR5H/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KA75EPIU2FVUUPRN3QP4ICOR5H/action/storage_attestation","attest_author":"https://pith.science/pith/KA75EPIU2FVUUPRN3QP4ICOR5H/action/author_attestation","sign_citation":"https://pith.science/pith/KA75EPIU2FVUUPRN3QP4ICOR5H/action/citation_signature","submit_replication":"https://pith.science/pith/KA75EPIU2FVUUPRN3QP4ICOR5H/action/replication_record"}},"created_at":"2026-05-18T00:08:38.311230+00:00","updated_at":"2026-05-18T00:08:38.311230+00:00"}