{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:CKKTZT5X7MF46FYORNSAYSWJME","short_pith_number":"pith:CKKTZT5X","schema_version":"1.0","canonical_sha256":"12953ccfb7fb0bcf170e8b640c4ac9611ccd01297bab563a073f34794dd492b4","source":{"kind":"arxiv","id":"2209.14059","version":1},"attestation_state":"computed","paper":{"title":"Interstellar scintillation and polarization of PSR B0656+14 in the Monogem Ring","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"Daniel R. Stinebring, Di Li, Jianping Yuan, Jumei Yao, Michael Kramer, Na Wang, Pei Wang, Richard N. Manchester, Weiwei Zhu, William A. Coles, Yi Feng","submitted_at":"2022-09-24T03:34:50Z","abstract_excerpt":"High sensitivity interstellar scintillation and polarization observations of PSR~B0656+14 made at three epochs over a year using the Five-hundred-meter Aperture Spherical radio Telescope (FAST) show that the scattering is dominated by two different compact regions. We identify the one nearer to the pulsar with the shell of the Monogem Ring, thereby confirming the association. The other is probably associated with the Local Bubble. We find that the observed position angles of the pulsar spin axis and the space velocity are significantly different, with a separation of $19\\fdg3\\pm$0\\fdg8, incons"},"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":"2209.14059","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2022-09-24T03:34:50Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"488dfc3e09410964e39ab9a641dcf1dc3b8307783bfc2127bc08c1094d78106e","abstract_canon_sha256":"d66b85ac24964376f4a3e39b105e4904aaee53566b12f5d0dfcb7c16cf6f637c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:16:24.365612Z","signature_b64":"lVZJj/QpPqqycYYvo4en6Q3ID1Yo9tkPSy8HiYYwj0/6BDCB6oVeSPVG6n1/S5/XeVZzjJpdSptipAA40dSJDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"12953ccfb7fb0bcf170e8b640c4ac9611ccd01297bab563a073f34794dd492b4","last_reissued_at":"2026-07-05T05:16:24.365127Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:16:24.365127Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Interstellar scintillation and polarization of PSR B0656+14 in the Monogem Ring","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"Daniel R. Stinebring, Di Li, Jianping Yuan, Jumei Yao, Michael Kramer, Na Wang, Pei Wang, Richard N. Manchester, Weiwei Zhu, William A. Coles, Yi Feng","submitted_at":"2022-09-24T03:34:50Z","abstract_excerpt":"High sensitivity interstellar scintillation and polarization observations of PSR~B0656+14 made at three epochs over a year using the Five-hundred-meter Aperture Spherical radio Telescope (FAST) show that the scattering is dominated by two different compact regions. We identify the one nearer to the pulsar with the shell of the Monogem Ring, thereby confirming the association. The other is probably associated with the Local Bubble. We find that the observed position angles of the pulsar spin axis and the space velocity are significantly different, with a separation of $19\\fdg3\\pm$0\\fdg8, incons"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2209.14059","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/2209.14059/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":"2209.14059","created_at":"2026-07-05T05:16:24.365204+00:00"},{"alias_kind":"arxiv_version","alias_value":"2209.14059v1","created_at":"2026-07-05T05:16:24.365204+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2209.14059","created_at":"2026-07-05T05:16:24.365204+00:00"},{"alias_kind":"pith_short_12","alias_value":"CKKTZT5X7MF4","created_at":"2026-07-05T05:16:24.365204+00:00"},{"alias_kind":"pith_short_16","alias_value":"CKKTZT5X7MF46FYO","created_at":"2026-07-05T05:16:24.365204+00:00"},{"alias_kind":"pith_short_8","alias_value":"CKKTZT5X","created_at":"2026-07-05T05:16:24.365204+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2310.16594","citing_title":"Constraining the slow-diffusion zone size and electron injection spectral index for the Geminga pulsar halo","ref_index":34,"is_internal_anchor":false},{"citing_arxiv_id":"2508.13667","citing_title":"PHECT: A lightweight computation tool for pulsar halo emission","ref_index":45,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CKKTZT5X7MF46FYORNSAYSWJME","json":"https://pith.science/pith/CKKTZT5X7MF46FYORNSAYSWJME.json","graph_json":"https://pith.science/api/pith-number/CKKTZT5X7MF46FYORNSAYSWJME/graph.json","events_json":"https://pith.science/api/pith-number/CKKTZT5X7MF46FYORNSAYSWJME/events.json","paper":"https://pith.science/paper/CKKTZT5X"},"agent_actions":{"view_html":"https://pith.science/pith/CKKTZT5X7MF46FYORNSAYSWJME","download_json":"https://pith.science/pith/CKKTZT5X7MF46FYORNSAYSWJME.json","view_paper":"https://pith.science/paper/CKKTZT5X","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2209.14059&json=true","fetch_graph":"https://pith.science/api/pith-number/CKKTZT5X7MF46FYORNSAYSWJME/graph.json","fetch_events":"https://pith.science/api/pith-number/CKKTZT5X7MF46FYORNSAYSWJME/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CKKTZT5X7MF46FYORNSAYSWJME/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CKKTZT5X7MF46FYORNSAYSWJME/action/storage_attestation","attest_author":"https://pith.science/pith/CKKTZT5X7MF46FYORNSAYSWJME/action/author_attestation","sign_citation":"https://pith.science/pith/CKKTZT5X7MF46FYORNSAYSWJME/action/citation_signature","submit_replication":"https://pith.science/pith/CKKTZT5X7MF46FYORNSAYSWJME/action/replication_record"}},"created_at":"2026-07-05T05:16:24.365204+00:00","updated_at":"2026-07-05T05:16:24.365204+00:00"}