{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:7OSZJISLUA5UU3UBIZCJ2A4H7E","short_pith_number":"pith:7OSZJISL","schema_version":"1.0","canonical_sha256":"fba594a24ba03b4a6e8146449d0387f93ec984fe505984972f688b9bb6e8effa","source":{"kind":"arxiv","id":"2010.09397","version":1},"attestation_state":"computed","paper":{"title":"Search for Off-pulse emission in Long Period Pulsars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Dipanjan Mitra, George I. Melikidze, Rahul Basu","submitted_at":"2020-10-19T11:33:36Z","abstract_excerpt":"We have revisited the problem of off-pulse emission in pulsars, where detailed search for the presence of low level radio emission outside the pulse window is carried out. The presence of off-pulse emission was earlier reported in two long period pulsars, PSR B0525+21 and B2046-16 at frequencies below 1 GHz using the Giant Meterwave Radio Telescope (GMRT). However, subsequent studies did not detect off-pulse emission from these pulsars at higher radio frequencies (> 1 GHz). We have carefully inspected the analysis scheme used in the earlier detections and found an anomaly with data editing rou"},"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":"2010.09397","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2020-10-19T11:33:36Z","cross_cats_sorted":[],"title_canon_sha256":"3e2c2b40ea03ae80b1403f5f020f02590e6c931fb6e45d914fe869fa887a0706","abstract_canon_sha256":"3d43a29d10cd48b79fe0354f8a66c9eef46ac0df546ea16207827c1599f06142"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:59:51.371985Z","signature_b64":"wgVkqFWGtbxVJNos9x1+0WOL8irXw7E+3sCGM3sfpskUylPaRG+QFzdr1NaLfiJFvbcTHbV7jVAeVCQ+vItqAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fba594a24ba03b4a6e8146449d0387f93ec984fe505984972f688b9bb6e8effa","last_reissued_at":"2026-07-05T01:59:51.371498Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:59:51.371498Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Search for Off-pulse emission in Long Period Pulsars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Dipanjan Mitra, George I. Melikidze, Rahul Basu","submitted_at":"2020-10-19T11:33:36Z","abstract_excerpt":"We have revisited the problem of off-pulse emission in pulsars, where detailed search for the presence of low level radio emission outside the pulse window is carried out. The presence of off-pulse emission was earlier reported in two long period pulsars, PSR B0525+21 and B2046-16 at frequencies below 1 GHz using the Giant Meterwave Radio Telescope (GMRT). However, subsequent studies did not detect off-pulse emission from these pulsars at higher radio frequencies (> 1 GHz). We have carefully inspected the analysis scheme used in the earlier detections and found an anomaly with data editing rou"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2010.09397","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/2010.09397/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":"2010.09397","created_at":"2026-07-05T01:59:51.371554+00:00"},{"alias_kind":"arxiv_version","alias_value":"2010.09397v1","created_at":"2026-07-05T01:59:51.371554+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2010.09397","created_at":"2026-07-05T01:59:51.371554+00:00"},{"alias_kind":"pith_short_12","alias_value":"7OSZJISLUA5U","created_at":"2026-07-05T01:59:51.371554+00:00"},{"alias_kind":"pith_short_16","alias_value":"7OSZJISLUA5UU3UB","created_at":"2026-07-05T01:59:51.371554+00:00"},{"alias_kind":"pith_short_8","alias_value":"7OSZJISL","created_at":"2026-07-05T01:59:51.371554+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/7OSZJISLUA5UU3UBIZCJ2A4H7E","json":"https://pith.science/pith/7OSZJISLUA5UU3UBIZCJ2A4H7E.json","graph_json":"https://pith.science/api/pith-number/7OSZJISLUA5UU3UBIZCJ2A4H7E/graph.json","events_json":"https://pith.science/api/pith-number/7OSZJISLUA5UU3UBIZCJ2A4H7E/events.json","paper":"https://pith.science/paper/7OSZJISL"},"agent_actions":{"view_html":"https://pith.science/pith/7OSZJISLUA5UU3UBIZCJ2A4H7E","download_json":"https://pith.science/pith/7OSZJISLUA5UU3UBIZCJ2A4H7E.json","view_paper":"https://pith.science/paper/7OSZJISL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2010.09397&json=true","fetch_graph":"https://pith.science/api/pith-number/7OSZJISLUA5UU3UBIZCJ2A4H7E/graph.json","fetch_events":"https://pith.science/api/pith-number/7OSZJISLUA5UU3UBIZCJ2A4H7E/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7OSZJISLUA5UU3UBIZCJ2A4H7E/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7OSZJISLUA5UU3UBIZCJ2A4H7E/action/storage_attestation","attest_author":"https://pith.science/pith/7OSZJISLUA5UU3UBIZCJ2A4H7E/action/author_attestation","sign_citation":"https://pith.science/pith/7OSZJISLUA5UU3UBIZCJ2A4H7E/action/citation_signature","submit_replication":"https://pith.science/pith/7OSZJISLUA5UU3UBIZCJ2A4H7E/action/replication_record"}},"created_at":"2026-07-05T01:59:51.371554+00:00","updated_at":"2026-07-05T01:59:51.371554+00:00"}