{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:S2EYOMFRKPGPUMIQXDFFRLTXVA","short_pith_number":"pith:S2EYOMFR","schema_version":"1.0","canonical_sha256":"96898730b153ccfa3110b8ca58ae77a811fdd805f4cd0396c1e84becb6343d8c","source":{"kind":"arxiv","id":"2006.00528","version":5},"attestation_state":"computed","paper":{"title":"The First Light Curve Solutions and Period Study of BQ Ari","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Aky\\\"uz, A. Boudesh, A. Poro, A. Sojoudizadeh, A. Solmaz, E. Lashgari, E. M. Esmer, F. Alicavus, F. Davoudi, J. Rahimi, M. Ghanbarzadehchaleshtori, M. Teke\\c{s}, N. Aksaker, O. Basturk, S. Khakpash, S. Modarres, Y. Alada\\u{g}","submitted_at":"2020-05-31T14:09:06Z","abstract_excerpt":"The first analysis of the photometric observation in BVR filters of a W UMa type binary system BQ Ari was performed. Light curve analysis was performed using Wilson-Devinney (W-D) code combined with a Monte Carlo (MC) simulation to determine its photometric and geometric elements and their uncertainties. These results show that BQ Ari is a contact binary system with a photometric mass ratio q=0.548\\pm0.019, a fillout factor f=24\\pm0.8 percent, and an orbital inclination of i=85.09\\pm0.45. We used the parallax from Gaia EDR3 for calculating the absolute parameters of the binary system. This stu"},"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":"2006.00528","kind":"arxiv","version":5},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2020-05-31T14:09:06Z","cross_cats_sorted":[],"title_canon_sha256":"8df84f8146e7447f2ac7d355fb569b12132055b0db1739a1b035c249bd647036","abstract_canon_sha256":"3b499c8bad1459b501dcb253293a607101c4c0be68ee4c5bd99b148e2e5f1907"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:28:09.558078Z","signature_b64":"lkS8P2wcjWg9sgm2vPptO50zP5CBJWo2mkuFOLjLL7cH6BAPVW/wmAvJv89SDPDc3KAjFc6ADFJ6FnrA8N4RCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"96898730b153ccfa3110b8ca58ae77a811fdd805f4cd0396c1e84becb6343d8c","last_reissued_at":"2026-07-05T03:28:09.557560Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:28:09.557560Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The First Light Curve Solutions and Period Study of BQ Ari","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"A. Aky\\\"uz, A. Boudesh, A. Poro, A. Sojoudizadeh, A. Solmaz, E. Lashgari, E. M. Esmer, F. Alicavus, F. Davoudi, J. Rahimi, M. Ghanbarzadehchaleshtori, M. Teke\\c{s}, N. Aksaker, O. Basturk, S. Khakpash, S. Modarres, Y. Alada\\u{g}","submitted_at":"2020-05-31T14:09:06Z","abstract_excerpt":"The first analysis of the photometric observation in BVR filters of a W UMa type binary system BQ Ari was performed. Light curve analysis was performed using Wilson-Devinney (W-D) code combined with a Monte Carlo (MC) simulation to determine its photometric and geometric elements and their uncertainties. These results show that BQ Ari is a contact binary system with a photometric mass ratio q=0.548\\pm0.019, a fillout factor f=24\\pm0.8 percent, and an orbital inclination of i=85.09\\pm0.45. We used the parallax from Gaia EDR3 for calculating the absolute parameters of the binary system. This stu"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2006.00528","kind":"arxiv","version":5},"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/2006.00528/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":"2006.00528","created_at":"2026-07-05T03:28:09.557615+00:00"},{"alias_kind":"arxiv_version","alias_value":"2006.00528v5","created_at":"2026-07-05T03:28:09.557615+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2006.00528","created_at":"2026-07-05T03:28:09.557615+00:00"},{"alias_kind":"pith_short_12","alias_value":"S2EYOMFRKPGP","created_at":"2026-07-05T03:28:09.557615+00:00"},{"alias_kind":"pith_short_16","alias_value":"S2EYOMFRKPGPUMIQ","created_at":"2026-07-05T03:28:09.557615+00:00"},{"alias_kind":"pith_short_8","alias_value":"S2EYOMFR","created_at":"2026-07-05T03:28:09.557615+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/S2EYOMFRKPGPUMIQXDFFRLTXVA","json":"https://pith.science/pith/S2EYOMFRKPGPUMIQXDFFRLTXVA.json","graph_json":"https://pith.science/api/pith-number/S2EYOMFRKPGPUMIQXDFFRLTXVA/graph.json","events_json":"https://pith.science/api/pith-number/S2EYOMFRKPGPUMIQXDFFRLTXVA/events.json","paper":"https://pith.science/paper/S2EYOMFR"},"agent_actions":{"view_html":"https://pith.science/pith/S2EYOMFRKPGPUMIQXDFFRLTXVA","download_json":"https://pith.science/pith/S2EYOMFRKPGPUMIQXDFFRLTXVA.json","view_paper":"https://pith.science/paper/S2EYOMFR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2006.00528&json=true","fetch_graph":"https://pith.science/api/pith-number/S2EYOMFRKPGPUMIQXDFFRLTXVA/graph.json","fetch_events":"https://pith.science/api/pith-number/S2EYOMFRKPGPUMIQXDFFRLTXVA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/S2EYOMFRKPGPUMIQXDFFRLTXVA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/S2EYOMFRKPGPUMIQXDFFRLTXVA/action/storage_attestation","attest_author":"https://pith.science/pith/S2EYOMFRKPGPUMIQXDFFRLTXVA/action/author_attestation","sign_citation":"https://pith.science/pith/S2EYOMFRKPGPUMIQXDFFRLTXVA/action/citation_signature","submit_replication":"https://pith.science/pith/S2EYOMFRKPGPUMIQXDFFRLTXVA/action/replication_record"}},"created_at":"2026-07-05T03:28:09.557615+00:00","updated_at":"2026-07-05T03:28:09.557615+00:00"}