{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:TOL76WDKNF56RGELH4772EMEYR","short_pith_number":"pith:TOL76WDK","schema_version":"1.0","canonical_sha256":"9b97ff586a697be8988b3f3ffd1184c47f0e3c58f456d585bf426303f2c4f480","source":{"kind":"arxiv","id":"2310.10341","version":1},"attestation_state":"computed","paper":{"title":"GMRT observations of the radio trail from CXOU J163802.6-471358","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.GA","authors_text":"D. A. Green, S. Roy","submitted_at":"2023-10-16T12:28:34Z","abstract_excerpt":"The X-ray source CXOU J163802.6-471358is thought to be a pulsar wind nebula (PWN), as it shows an extended, $\\approx 40$ arcsec trail from a compact source. Here we present GMRT observations of this source at 330 and 1390 MHz, which reveal a remarkable linear radio trail $\\approx 90$ arcsec in extent. Although the radio trail points back to the supernova remnant (SNR) G338.1+0.4, $\\approx 50$ arcmin from ,CXOU J163802.6-471358 associating it with this remnant would require a very large velocity for the pulsar. There are no known galactic SNRs close to the PWN and radio trail. No pulsar has yet"},"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":"2310.10341","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2023-10-16T12:28:34Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"c7c59926e77c4c625bb05d7c01fd548522c657cb6b11549e2ab33f743042a453","abstract_canon_sha256":"03dbcc81926a40e5e062a7f5d548dd62bec62cac1da55fff448dcd98f58b4407"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:01:18.990088Z","signature_b64":"UTqfw4Grf46p4UKwr2qEpE+5LhkQtc8PVa2jQHObrptBViF8KIHdecFAG3irGDHtowuXHgE99L2JEeRp9R0gCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9b97ff586a697be8988b3f3ffd1184c47f0e3c58f456d585bf426303f2c4f480","last_reissued_at":"2026-07-05T07:01:18.989691Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:01:18.989691Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"GMRT observations of the radio trail from CXOU J163802.6-471358","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.GA","authors_text":"D. A. Green, S. Roy","submitted_at":"2023-10-16T12:28:34Z","abstract_excerpt":"The X-ray source CXOU J163802.6-471358is thought to be a pulsar wind nebula (PWN), as it shows an extended, $\\approx 40$ arcsec trail from a compact source. Here we present GMRT observations of this source at 330 and 1390 MHz, which reveal a remarkable linear radio trail $\\approx 90$ arcsec in extent. Although the radio trail points back to the supernova remnant (SNR) G338.1+0.4, $\\approx 50$ arcmin from ,CXOU J163802.6-471358 associating it with this remnant would require a very large velocity for the pulsar. There are no known galactic SNRs close to the PWN and radio trail. No pulsar has yet"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2310.10341","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/2310.10341/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":"2310.10341","created_at":"2026-07-05T07:01:18.989752+00:00"},{"alias_kind":"arxiv_version","alias_value":"2310.10341v1","created_at":"2026-07-05T07:01:18.989752+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2310.10341","created_at":"2026-07-05T07:01:18.989752+00:00"},{"alias_kind":"pith_short_12","alias_value":"TOL76WDKNF56","created_at":"2026-07-05T07:01:18.989752+00:00"},{"alias_kind":"pith_short_16","alias_value":"TOL76WDKNF56RGEL","created_at":"2026-07-05T07:01:18.989752+00:00"},{"alias_kind":"pith_short_8","alias_value":"TOL76WDK","created_at":"2026-07-05T07:01:18.989752+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/TOL76WDKNF56RGELH4772EMEYR","json":"https://pith.science/pith/TOL76WDKNF56RGELH4772EMEYR.json","graph_json":"https://pith.science/api/pith-number/TOL76WDKNF56RGELH4772EMEYR/graph.json","events_json":"https://pith.science/api/pith-number/TOL76WDKNF56RGELH4772EMEYR/events.json","paper":"https://pith.science/paper/TOL76WDK"},"agent_actions":{"view_html":"https://pith.science/pith/TOL76WDKNF56RGELH4772EMEYR","download_json":"https://pith.science/pith/TOL76WDKNF56RGELH4772EMEYR.json","view_paper":"https://pith.science/paper/TOL76WDK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2310.10341&json=true","fetch_graph":"https://pith.science/api/pith-number/TOL76WDKNF56RGELH4772EMEYR/graph.json","fetch_events":"https://pith.science/api/pith-number/TOL76WDKNF56RGELH4772EMEYR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TOL76WDKNF56RGELH4772EMEYR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TOL76WDKNF56RGELH4772EMEYR/action/storage_attestation","attest_author":"https://pith.science/pith/TOL76WDKNF56RGELH4772EMEYR/action/author_attestation","sign_citation":"https://pith.science/pith/TOL76WDKNF56RGELH4772EMEYR/action/citation_signature","submit_replication":"https://pith.science/pith/TOL76WDKNF56RGELH4772EMEYR/action/replication_record"}},"created_at":"2026-07-05T07:01:18.989752+00:00","updated_at":"2026-07-05T07:01:18.989752+00:00"}