{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:BO6CRVODEQRCO5LGHZ7YQW26QJ","short_pith_number":"pith:BO6CRVOD","schema_version":"1.0","canonical_sha256":"0bbc28d5c324222775663e7f885b5e82585cbd303c9c40a0e6f0b7dde1d426d8","source":{"kind":"arxiv","id":"1009.1622","version":1},"attestation_state":"computed","paper":{"title":"Modules for Experiments in Stellar Astrophysics (MESA)","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.SR","authors_text":"Aaron Dotter, Bill Paxton, Falk Herwig, Frank Timmes, Lars Bildsten, Pierre Lesaffre","submitted_at":"2010-09-08T20:00:05Z","abstract_excerpt":"Stellar physics and evolution calculations enable a broad range of research in astrophysics. Modules for Experiments in Stellar Astrophysics (MESA) is a suite of open source libraries for a wide range of applications in computational stellar astrophysics. A newly designed 1-D stellar evolution module, MESA star, combines many of the numerical and physics modules for simulations of a wide range of stellar evolution scenarios ranging from very-low mass to massive stars, including advanced evolutionary phases. MESA star solves the fully coupled structure and composition equations simultaneously. "},"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":"1009.1622","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2010-09-08T20:00:05Z","cross_cats_sorted":["astro-ph.IM"],"title_canon_sha256":"e4c1edacc11a04ed95800ae4a0c79eba1bd49e8c75ff89d2121142b3b7d736fc","abstract_canon_sha256":"db595c160f1efc9fabf5f80b93b1f68de94451865475c3213149bc3ff830ede6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:33:06.890061Z","signature_b64":"UY5yOWv7A/4qirvXCStkuio+ZxKzxUv6+b+wm/TVqkt7D5RUPv1Ee83pnnngM00Ge966daALMCJ0AMjDUH/wCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0bbc28d5c324222775663e7f885b5e82585cbd303c9c40a0e6f0b7dde1d426d8","last_reissued_at":"2026-05-18T04:33:06.889475Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:33:06.889475Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Modules for Experiments in Stellar Astrophysics (MESA)","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"astro-ph.SR","authors_text":"Aaron Dotter, Bill Paxton, Falk Herwig, Frank Timmes, Lars Bildsten, Pierre Lesaffre","submitted_at":"2010-09-08T20:00:05Z","abstract_excerpt":"Stellar physics and evolution calculations enable a broad range of research in astrophysics. Modules for Experiments in Stellar Astrophysics (MESA) is a suite of open source libraries for a wide range of applications in computational stellar astrophysics. A newly designed 1-D stellar evolution module, MESA star, combines many of the numerical and physics modules for simulations of a wide range of stellar evolution scenarios ranging from very-low mass to massive stars, including advanced evolutionary phases. MESA star solves the fully coupled structure and composition equations simultaneously. "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1009.1622","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":"1009.1622","created_at":"2026-05-18T04:33:06.889545+00:00"},{"alias_kind":"arxiv_version","alias_value":"1009.1622v1","created_at":"2026-05-18T04:33:06.889545+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1009.1622","created_at":"2026-05-18T04:33:06.889545+00:00"},{"alias_kind":"pith_short_12","alias_value":"BO6CRVODEQRC","created_at":"2026-05-18T12:26:05.355336+00:00"},{"alias_kind":"pith_short_16","alias_value":"BO6CRVODEQRCO5LG","created_at":"2026-05-18T12:26:05.355336+00:00"},{"alias_kind":"pith_short_8","alias_value":"BO6CRVOD","created_at":"2026-05-18T12:26:05.355336+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":11,"internal_anchor_count":7,"sample":[{"citing_arxiv_id":"2605.23209","citing_title":"TESS Observations of Stochastic Low-frequency Variability in Extreme Helium Stars","ref_index":278,"is_internal_anchor":true},{"citing_arxiv_id":"2602.15119","citing_title":"Detection horizon for the neutrino burst from the stellar helium flash","ref_index":34,"is_internal_anchor":true},{"citing_arxiv_id":"2605.21062","citing_title":"Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models","ref_index":1,"is_internal_anchor":true},{"citing_arxiv_id":"2605.19000","citing_title":"Exoplanets in ancient stellar populations: occurrence constraints and hot-Jupiter candidates in the Galactic halo","ref_index":68,"is_internal_anchor":true},{"citing_arxiv_id":"2605.17005","citing_title":"Red novae, their progenitors, and remnants","ref_index":123,"is_internal_anchor":true},{"citing_arxiv_id":"2510.06741","citing_title":"Diagnosing the Properties and Evolutionary Fates of Black Hole and Wolf-Rayet X-ray Binaries as Potential Gravitational Wave Sources for the LIGO-Virgo-KAGRA Network","ref_index":25,"is_internal_anchor":true},{"citing_arxiv_id":"2510.17955","citing_title":"Sub-Snowline Formation of Gas-Giant Planets in Binary Systems","ref_index":22,"is_internal_anchor":true},{"citing_arxiv_id":"2604.02413","citing_title":"The Black Hole Mass Gap as a New Probe of Millicharged Particles","ref_index":82,"is_internal_anchor":false},{"citing_arxiv_id":"2604.26004","citing_title":"Revisiting Turner Window Axions: The Untapped Potential of NaI Dark Matter Detectors","ref_index":36,"is_internal_anchor":false},{"citing_arxiv_id":"2604.23503","citing_title":"Hyperaccreting Neutron Stars inside Massive Envelopes: The Implausibility of Thorne-\\.Zytkow Objects","ref_index":48,"is_internal_anchor":false},{"citing_arxiv_id":"2604.21650","citing_title":"Modeling of the magnetic stellar wind braking of the ssrAp 33 Lib (HD137949)","ref_index":54,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/BO6CRVODEQRCO5LGHZ7YQW26QJ","json":"https://pith.science/pith/BO6CRVODEQRCO5LGHZ7YQW26QJ.json","graph_json":"https://pith.science/api/pith-number/BO6CRVODEQRCO5LGHZ7YQW26QJ/graph.json","events_json":"https://pith.science/api/pith-number/BO6CRVODEQRCO5LGHZ7YQW26QJ/events.json","paper":"https://pith.science/paper/BO6CRVOD"},"agent_actions":{"view_html":"https://pith.science/pith/BO6CRVODEQRCO5LGHZ7YQW26QJ","download_json":"https://pith.science/pith/BO6CRVODEQRCO5LGHZ7YQW26QJ.json","view_paper":"https://pith.science/paper/BO6CRVOD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1009.1622&json=true","fetch_graph":"https://pith.science/api/pith-number/BO6CRVODEQRCO5LGHZ7YQW26QJ/graph.json","fetch_events":"https://pith.science/api/pith-number/BO6CRVODEQRCO5LGHZ7YQW26QJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BO6CRVODEQRCO5LGHZ7YQW26QJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BO6CRVODEQRCO5LGHZ7YQW26QJ/action/storage_attestation","attest_author":"https://pith.science/pith/BO6CRVODEQRCO5LGHZ7YQW26QJ/action/author_attestation","sign_citation":"https://pith.science/pith/BO6CRVODEQRCO5LGHZ7YQW26QJ/action/citation_signature","submit_replication":"https://pith.science/pith/BO6CRVODEQRCO5LGHZ7YQW26QJ/action/replication_record"}},"created_at":"2026-05-18T04:33:06.889545+00:00","updated_at":"2026-05-18T04:33:06.889545+00:00"}