{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:ZCLYEEUAJLUY4KX5UUFMGLZCVY","short_pith_number":"pith:ZCLYEEUA","schema_version":"1.0","canonical_sha256":"c8978212804ae98e2afda50ac32f22ae12d7baf8d5391a0e5cc6730570e42787","source":{"kind":"arxiv","id":"2407.01285","version":1},"attestation_state":"computed","paper":{"title":"Search for rotating radio transients in monitoring data for three years","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A.V. Chernosov, D.V. Pervoukhin, E.A. Brylyakova, G.E. Tyul'basheva, I.L. Ovchinnikov, M.A. Kitaeva, S.A. Tyul'bashev","submitted_at":"2024-07-01T13:39:33Z","abstract_excerpt":"The search for rotating radio transients (RRAT) was done at a frequency of 111 MHz, in daily observations carried out on the radio telescope, a Large Phased Array (LPA) at declinations -9o < decj < +42o. 19 new RRATs were discovered for dispersion measures (DM) from 2.5 to 72.6 pc cm^{-3}. Estimates of the periods were obtained for three RRATs. Two of them (J0408+28; J0440+35) are located at distances of 134 and 136 pc from Sun and are among the closest of all known RRATs."},"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":"2407.01285","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2024-07-01T13:39:33Z","cross_cats_sorted":[],"title_canon_sha256":"9687f942b5b3d20358a68bc06fb5018851432efcee0b3c7622c8a58b0c4198e3","abstract_canon_sha256":"bd0790870bf150e11e357020f32696d1e286ad3bd41e415e5c22285835a580d2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:38:45.723659Z","signature_b64":"93gDmPZJsrbX0nD59+mWzIukR4dJUz0ud+X6JZtQTQltqeEWDgZka0t0XMXTbbSmJKjPVmRgel9nCgv1EC35Cw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c8978212804ae98e2afda50ac32f22ae12d7baf8d5391a0e5cc6730570e42787","last_reissued_at":"2026-07-05T08:38:45.723166Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:38:45.723166Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Search for rotating radio transients in monitoring data for three years","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A.V. Chernosov, D.V. Pervoukhin, E.A. Brylyakova, G.E. Tyul'basheva, I.L. Ovchinnikov, M.A. Kitaeva, S.A. Tyul'bashev","submitted_at":"2024-07-01T13:39:33Z","abstract_excerpt":"The search for rotating radio transients (RRAT) was done at a frequency of 111 MHz, in daily observations carried out on the radio telescope, a Large Phased Array (LPA) at declinations -9o < decj < +42o. 19 new RRATs were discovered for dispersion measures (DM) from 2.5 to 72.6 pc cm^{-3}. Estimates of the periods were obtained for three RRATs. Two of them (J0408+28; J0440+35) are located at distances of 134 and 136 pc from Sun and are among the closest of all known RRATs."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2407.01285","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/2407.01285/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":"2407.01285","created_at":"2026-07-05T08:38:45.723221+00:00"},{"alias_kind":"arxiv_version","alias_value":"2407.01285v1","created_at":"2026-07-05T08:38:45.723221+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2407.01285","created_at":"2026-07-05T08:38:45.723221+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZCLYEEUAJLUY","created_at":"2026-07-05T08:38:45.723221+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZCLYEEUAJLUY4KX5","created_at":"2026-07-05T08:38:45.723221+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZCLYEEUA","created_at":"2026-07-05T08:38:45.723221+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2509.03001","citing_title":"Low-frequency observations of low-mass binary systems with neutron star candidates","ref_index":63,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/ZCLYEEUAJLUY4KX5UUFMGLZCVY","json":"https://pith.science/pith/ZCLYEEUAJLUY4KX5UUFMGLZCVY.json","graph_json":"https://pith.science/api/pith-number/ZCLYEEUAJLUY4KX5UUFMGLZCVY/graph.json","events_json":"https://pith.science/api/pith-number/ZCLYEEUAJLUY4KX5UUFMGLZCVY/events.json","paper":"https://pith.science/paper/ZCLYEEUA"},"agent_actions":{"view_html":"https://pith.science/pith/ZCLYEEUAJLUY4KX5UUFMGLZCVY","download_json":"https://pith.science/pith/ZCLYEEUAJLUY4KX5UUFMGLZCVY.json","view_paper":"https://pith.science/paper/ZCLYEEUA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2407.01285&json=true","fetch_graph":"https://pith.science/api/pith-number/ZCLYEEUAJLUY4KX5UUFMGLZCVY/graph.json","fetch_events":"https://pith.science/api/pith-number/ZCLYEEUAJLUY4KX5UUFMGLZCVY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZCLYEEUAJLUY4KX5UUFMGLZCVY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZCLYEEUAJLUY4KX5UUFMGLZCVY/action/storage_attestation","attest_author":"https://pith.science/pith/ZCLYEEUAJLUY4KX5UUFMGLZCVY/action/author_attestation","sign_citation":"https://pith.science/pith/ZCLYEEUAJLUY4KX5UUFMGLZCVY/action/citation_signature","submit_replication":"https://pith.science/pith/ZCLYEEUAJLUY4KX5UUFMGLZCVY/action/replication_record"}},"created_at":"2026-07-05T08:38:45.723221+00:00","updated_at":"2026-07-05T08:38:45.723221+00:00"}