{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:27XRV4FBTGHH52PVGL7OH3XL5J","short_pith_number":"pith:27XRV4FB","schema_version":"1.0","canonical_sha256":"d7ef1af0a1998e7ee9f532fee3eeebea7cd151859295acdb25e72c63f8fb419f","source":{"kind":"arxiv","id":"1211.6550","version":2},"attestation_state":"computed","paper":{"title":"A study of the performance of the transit detection tool DST in space-based surveys. Application of the CoRoT pipeline to Kepler data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Erikson, H. Rauer, J. Cabrera, S. Kirste, Sz. Csizmadia","submitted_at":"2012-11-28T09:16:28Z","abstract_excerpt":"Context. Transit detection algorithms are mathematical tools used for detecting planets in the photometric data of transit surveys. In this work we study their application to space-based surveys. Aims: Space missions are exploring the parameter space of the transit surveys where classical algorithms do not perform optimally, either because of the challenging signal-to-noise ratio of the signal or its non-periodic characteristics. We have developed an algorithm addressing these challenges for the mission CoRoT. Here we extend the application to the data from the space mission Kepler. We aim at "},"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":"1211.6550","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.EP","submitted_at":"2012-11-28T09:16:28Z","cross_cats_sorted":[],"title_canon_sha256":"af75daed65c0bdab440c404cdc654720daa5869168b5dc84fd51e68993261d71","abstract_canon_sha256":"14d7bfe585f527a2d54607892f4f32410fbec87c45231c8882c704ac9f4bd661"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:39:14.298879Z","signature_b64":"Kc/NNcT0GRtkta/PAah4m10OoTQT/SFnZDqqZmqfkIgwPH/snoeFpggIn9r1xNa4hteD4gLWiYsF0xXjbT9QDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d7ef1af0a1998e7ee9f532fee3eeebea7cd151859295acdb25e72c63f8fb419f","last_reissued_at":"2026-05-18T03:39:14.298172Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:39:14.298172Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A study of the performance of the transit detection tool DST in space-based surveys. Application of the CoRoT pipeline to Kepler data","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.EP","authors_text":"A. Erikson, H. Rauer, J. Cabrera, S. Kirste, Sz. Csizmadia","submitted_at":"2012-11-28T09:16:28Z","abstract_excerpt":"Context. Transit detection algorithms are mathematical tools used for detecting planets in the photometric data of transit surveys. In this work we study their application to space-based surveys. Aims: Space missions are exploring the parameter space of the transit surveys where classical algorithms do not perform optimally, either because of the challenging signal-to-noise ratio of the signal or its non-periodic characteristics. We have developed an algorithm addressing these challenges for the mission CoRoT. Here we extend the application to the data from the space mission Kepler. We aim at "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1211.6550","kind":"arxiv","version":2},"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":"1211.6550","created_at":"2026-05-18T03:39:14.298275+00:00"},{"alias_kind":"arxiv_version","alias_value":"1211.6550v2","created_at":"2026-05-18T03:39:14.298275+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1211.6550","created_at":"2026-05-18T03:39:14.298275+00:00"},{"alias_kind":"pith_short_12","alias_value":"27XRV4FBTGHH","created_at":"2026-05-18T12:26:50.516681+00:00"},{"alias_kind":"pith_short_16","alias_value":"27XRV4FBTGHH52PV","created_at":"2026-05-18T12:26:50.516681+00:00"},{"alias_kind":"pith_short_8","alias_value":"27XRV4FB","created_at":"2026-05-18T12:26:50.516681+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/27XRV4FBTGHH52PVGL7OH3XL5J","json":"https://pith.science/pith/27XRV4FBTGHH52PVGL7OH3XL5J.json","graph_json":"https://pith.science/api/pith-number/27XRV4FBTGHH52PVGL7OH3XL5J/graph.json","events_json":"https://pith.science/api/pith-number/27XRV4FBTGHH52PVGL7OH3XL5J/events.json","paper":"https://pith.science/paper/27XRV4FB"},"agent_actions":{"view_html":"https://pith.science/pith/27XRV4FBTGHH52PVGL7OH3XL5J","download_json":"https://pith.science/pith/27XRV4FBTGHH52PVGL7OH3XL5J.json","view_paper":"https://pith.science/paper/27XRV4FB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1211.6550&json=true","fetch_graph":"https://pith.science/api/pith-number/27XRV4FBTGHH52PVGL7OH3XL5J/graph.json","fetch_events":"https://pith.science/api/pith-number/27XRV4FBTGHH52PVGL7OH3XL5J/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/27XRV4FBTGHH52PVGL7OH3XL5J/action/timestamp_anchor","attest_storage":"https://pith.science/pith/27XRV4FBTGHH52PVGL7OH3XL5J/action/storage_attestation","attest_author":"https://pith.science/pith/27XRV4FBTGHH52PVGL7OH3XL5J/action/author_attestation","sign_citation":"https://pith.science/pith/27XRV4FBTGHH52PVGL7OH3XL5J/action/citation_signature","submit_replication":"https://pith.science/pith/27XRV4FBTGHH52PVGL7OH3XL5J/action/replication_record"}},"created_at":"2026-05-18T03:39:14.298275+00:00","updated_at":"2026-05-18T03:39:14.298275+00:00"}