{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:23ASPPMND6UXVYLMINLILX4TH3","short_pith_number":"pith:23ASPPMN","schema_version":"1.0","canonical_sha256":"d6c127bd8d1fa97ae16c435685df933eca249723d2a3a2992deeb47fd29dadd1","source":{"kind":"arxiv","id":"1706.08896","version":2},"attestation_state":"computed","paper":{"title":"Scintillation based search for off-pulse radio emission from pulsars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","astro-ph.IM"],"primary_cat":"astro-ph.HE","authors_text":"Avinash A. Deshpande, Kumar Ravi","submitted_at":"2017-06-27T14:52:45Z","abstract_excerpt":"We propose a new method to detect off-pulse (unpulsed and/or continuous) emission from pulsars, using the intensity modulations associated with interstellar scintillation. Our technique involves obtaining the dynamic spectra, separately for on-pulse window and off-pulse region, with time and frequency resolutions to properly sample the intensity variations due to diffractive scintillation, and then estimating their mutual correlation as a measure of off-pulse emission, if any. We describe and illustrate the essential details of this technique with the help of simulations, as well as real data."},"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":"1706.08896","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-06-27T14:52:45Z","cross_cats_sorted":["astro-ph.GA","astro-ph.IM"],"title_canon_sha256":"2329bd7ed9cdbaf115e7dce6a648e94b4b7b9dd37ba87a057ccf78ed3541dee6","abstract_canon_sha256":"1f95d0fa6abe9256a88df068a66ad8cd654698b228ccaa3285741feb1ba05e9f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:15:21.832004Z","signature_b64":"oDEz2vgsRYAwbRRk3MDNUfDRAmWTQ52bAPbkGM/eoXbDx5cK13GP6LlfPHnEeODFXB1Zf33eBCT+GrzI9YZNDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d6c127bd8d1fa97ae16c435685df933eca249723d2a3a2992deeb47fd29dadd1","last_reissued_at":"2026-05-18T00:15:21.831266Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:15:21.831266Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Scintillation based search for off-pulse radio emission from pulsars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","astro-ph.IM"],"primary_cat":"astro-ph.HE","authors_text":"Avinash A. Deshpande, Kumar Ravi","submitted_at":"2017-06-27T14:52:45Z","abstract_excerpt":"We propose a new method to detect off-pulse (unpulsed and/or continuous) emission from pulsars, using the intensity modulations associated with interstellar scintillation. Our technique involves obtaining the dynamic spectra, separately for on-pulse window and off-pulse region, with time and frequency resolutions to properly sample the intensity variations due to diffractive scintillation, and then estimating their mutual correlation as a measure of off-pulse emission, if any. We describe and illustrate the essential details of this technique with the help of simulations, as well as real data."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1706.08896","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":"1706.08896","created_at":"2026-05-18T00:15:21.831447+00:00"},{"alias_kind":"arxiv_version","alias_value":"1706.08896v2","created_at":"2026-05-18T00:15:21.831447+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1706.08896","created_at":"2026-05-18T00:15:21.831447+00:00"},{"alias_kind":"pith_short_12","alias_value":"23ASPPMND6UX","created_at":"2026-05-18T12:30:55.937587+00:00"},{"alias_kind":"pith_short_16","alias_value":"23ASPPMND6UXVYLM","created_at":"2026-05-18T12:30:55.937587+00:00"},{"alias_kind":"pith_short_8","alias_value":"23ASPPMN","created_at":"2026-05-18T12:30:55.937587+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/23ASPPMND6UXVYLMINLILX4TH3","json":"https://pith.science/pith/23ASPPMND6UXVYLMINLILX4TH3.json","graph_json":"https://pith.science/api/pith-number/23ASPPMND6UXVYLMINLILX4TH3/graph.json","events_json":"https://pith.science/api/pith-number/23ASPPMND6UXVYLMINLILX4TH3/events.json","paper":"https://pith.science/paper/23ASPPMN"},"agent_actions":{"view_html":"https://pith.science/pith/23ASPPMND6UXVYLMINLILX4TH3","download_json":"https://pith.science/pith/23ASPPMND6UXVYLMINLILX4TH3.json","view_paper":"https://pith.science/paper/23ASPPMN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1706.08896&json=true","fetch_graph":"https://pith.science/api/pith-number/23ASPPMND6UXVYLMINLILX4TH3/graph.json","fetch_events":"https://pith.science/api/pith-number/23ASPPMND6UXVYLMINLILX4TH3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/23ASPPMND6UXVYLMINLILX4TH3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/23ASPPMND6UXVYLMINLILX4TH3/action/storage_attestation","attest_author":"https://pith.science/pith/23ASPPMND6UXVYLMINLILX4TH3/action/author_attestation","sign_citation":"https://pith.science/pith/23ASPPMND6UXVYLMINLILX4TH3/action/citation_signature","submit_replication":"https://pith.science/pith/23ASPPMND6UXVYLMINLILX4TH3/action/replication_record"}},"created_at":"2026-05-18T00:15:21.831447+00:00","updated_at":"2026-05-18T00:15:21.831447+00:00"}