{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:BFQRCSF2LCZRXA4243FWPSAW6B","short_pith_number":"pith:BFQRCSF2","schema_version":"1.0","canonical_sha256":"09611148ba58b31b839ae6cb67c816f06fca1795af74752306cd34ff9d66145c","source":{"kind":"arxiv","id":"1010.1758","version":1},"attestation_state":"computed","paper":{"title":"The G292.0+1.8 pulsar wind nebula in the mid-infrared","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A.A. Danilenko, D.A. Zyuzin, S.V. Zharikov, Yu.A. Shibanov","submitted_at":"2010-10-08T18:38:25Z","abstract_excerpt":"G292.0+1.8 is a Cas A-like supernova remnant that contains the young pulsar PSR J1124-5916 powering a compact torus-like pulsar wind nebula visible in X-rays. A likely counterpart to the nebula has been detected in the optical VRI bands. To confirm the counterpart candidate nature, we examined archival mid-infrared data obtained with the Spitzer Space Telescope. Broad-band images taken at 4.5, 8, 24, and 70 microns were analyzed and compared with available optical and X-ray data. The extended counterpart candidate is firmly detected in the 4.5 and 8 micron bands. It is brighter and more extend"},"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":"1010.1758","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2010-10-08T18:38:25Z","cross_cats_sorted":[],"title_canon_sha256":"c837e23113f589e6e4a94181776a58434a7a218c8fa94e81fe7cade7872c450f","abstract_canon_sha256":"78f5ec88e024578115c8becd6f199a19edd6def3026e3d99d5d048c960f9192b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:39:39.717388Z","signature_b64":"CYGH0hWZKtnOufUajDupcbokQgM0bwF8q8+YjJ8Kd6Pr5iJyi/1a3aAo33EY9GO5DejfEZDR3+I23F0VPP9FDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"09611148ba58b31b839ae6cb67c816f06fca1795af74752306cd34ff9d66145c","last_reissued_at":"2026-05-18T04:39:39.716891Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:39:39.716891Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The G292.0+1.8 pulsar wind nebula in the mid-infrared","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A.A. Danilenko, D.A. Zyuzin, S.V. Zharikov, Yu.A. Shibanov","submitted_at":"2010-10-08T18:38:25Z","abstract_excerpt":"G292.0+1.8 is a Cas A-like supernova remnant that contains the young pulsar PSR J1124-5916 powering a compact torus-like pulsar wind nebula visible in X-rays. A likely counterpart to the nebula has been detected in the optical VRI bands. To confirm the counterpart candidate nature, we examined archival mid-infrared data obtained with the Spitzer Space Telescope. Broad-band images taken at 4.5, 8, 24, and 70 microns were analyzed and compared with available optical and X-ray data. The extended counterpart candidate is firmly detected in the 4.5 and 8 micron bands. It is brighter and more extend"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1010.1758","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":""},"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":"1010.1758","created_at":"2026-05-18T04:39:39.716973+00:00"},{"alias_kind":"arxiv_version","alias_value":"1010.1758v1","created_at":"2026-05-18T04:39:39.716973+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1010.1758","created_at":"2026-05-18T04:39:39.716973+00:00"},{"alias_kind":"pith_short_12","alias_value":"BFQRCSF2LCZR","created_at":"2026-05-18T12:26:05.355336+00:00"},{"alias_kind":"pith_short_16","alias_value":"BFQRCSF2LCZRXA42","created_at":"2026-05-18T12:26:05.355336+00:00"},{"alias_kind":"pith_short_8","alias_value":"BFQRCSF2","created_at":"2026-05-18T12:26:05.355336+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/BFQRCSF2LCZRXA4243FWPSAW6B","json":"https://pith.science/pith/BFQRCSF2LCZRXA4243FWPSAW6B.json","graph_json":"https://pith.science/api/pith-number/BFQRCSF2LCZRXA4243FWPSAW6B/graph.json","events_json":"https://pith.science/api/pith-number/BFQRCSF2LCZRXA4243FWPSAW6B/events.json","paper":"https://pith.science/paper/BFQRCSF2"},"agent_actions":{"view_html":"https://pith.science/pith/BFQRCSF2LCZRXA4243FWPSAW6B","download_json":"https://pith.science/pith/BFQRCSF2LCZRXA4243FWPSAW6B.json","view_paper":"https://pith.science/paper/BFQRCSF2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1010.1758&json=true","fetch_graph":"https://pith.science/api/pith-number/BFQRCSF2LCZRXA4243FWPSAW6B/graph.json","fetch_events":"https://pith.science/api/pith-number/BFQRCSF2LCZRXA4243FWPSAW6B/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BFQRCSF2LCZRXA4243FWPSAW6B/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BFQRCSF2LCZRXA4243FWPSAW6B/action/storage_attestation","attest_author":"https://pith.science/pith/BFQRCSF2LCZRXA4243FWPSAW6B/action/author_attestation","sign_citation":"https://pith.science/pith/BFQRCSF2LCZRXA4243FWPSAW6B/action/citation_signature","submit_replication":"https://pith.science/pith/BFQRCSF2LCZRXA4243FWPSAW6B/action/replication_record"}},"created_at":"2026-05-18T04:39:39.716973+00:00","updated_at":"2026-05-18T04:39:39.716973+00:00"}