{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:YAZG7OPFBIY23YEVCDKE4SMDJC","short_pith_number":"pith:YAZG7OPF","schema_version":"1.0","canonical_sha256":"c0326fb9e50a31ade09510d44e498348b253805f5d187b7ca963c6730c9de1ac","source":{"kind":"arxiv","id":"1905.03741","version":1},"attestation_state":"computed","paper":{"title":"New composite supernova remnant toward HESS J1844-030?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Alberto Petriella","submitted_at":"2019-05-09T16:34:51Z","abstract_excerpt":"AIMS: HESS J1844-030 is a newly confirmed TeV source in the direction of the X-ray pulsar wind nebula (PWN) candidate G29.4+0.1 and the complex radio source G29.37+0.1, which is likely formed by the superposition of a background radio galaxy and a Galactic supernova remnant (SNR). We investigate the possible connection between the SNR, the PWN G29.4+0.1, and HESS J1844-030 to shed light on the astrophysical origin of the TeV emission. METHODS: We performed an imaging and spectral study of the X-ray emission from the PWN G29.4+0.1 using archival observations obtained with the Chandra and XMM-Ne"},"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":"1905.03741","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2019-05-09T16:34:51Z","cross_cats_sorted":[],"title_canon_sha256":"7c7ea5cb774ed2c8377ac5f339fd97b6a255ab45f9e909dce0a7783bc2f0937f","abstract_canon_sha256":"0053d3d060d9295d0ac9bcdfbc2424d10b5f50376722c64acc9bbe7682e328d1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:43:02.148564Z","signature_b64":"I225/BZvy7GYUouQlzhP+JrAMIAL9TAJdXhqo+ssVF3mfoYzqJV0RKSI0iKqQB0p8OqkKOE0J6umAHezspFEAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c0326fb9e50a31ade09510d44e498348b253805f5d187b7ca963c6730c9de1ac","last_reissued_at":"2026-05-17T23:43:02.147858Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:43:02.147858Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"New composite supernova remnant toward HESS J1844-030?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Alberto Petriella","submitted_at":"2019-05-09T16:34:51Z","abstract_excerpt":"AIMS: HESS J1844-030 is a newly confirmed TeV source in the direction of the X-ray pulsar wind nebula (PWN) candidate G29.4+0.1 and the complex radio source G29.37+0.1, which is likely formed by the superposition of a background radio galaxy and a Galactic supernova remnant (SNR). We investigate the possible connection between the SNR, the PWN G29.4+0.1, and HESS J1844-030 to shed light on the astrophysical origin of the TeV emission. METHODS: We performed an imaging and spectral study of the X-ray emission from the PWN G29.4+0.1 using archival observations obtained with the Chandra and XMM-Ne"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1905.03741","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":"1905.03741","created_at":"2026-05-17T23:43:02.147981+00:00"},{"alias_kind":"arxiv_version","alias_value":"1905.03741v1","created_at":"2026-05-17T23:43:02.147981+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1905.03741","created_at":"2026-05-17T23:43:02.147981+00:00"},{"alias_kind":"pith_short_12","alias_value":"YAZG7OPFBIY2","created_at":"2026-05-18T12:33:33.725879+00:00"},{"alias_kind":"pith_short_16","alias_value":"YAZG7OPFBIY23YEV","created_at":"2026-05-18T12:33:33.725879+00:00"},{"alias_kind":"pith_short_8","alias_value":"YAZG7OPF","created_at":"2026-05-18T12:33:33.725879+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/YAZG7OPFBIY23YEVCDKE4SMDJC","json":"https://pith.science/pith/YAZG7OPFBIY23YEVCDKE4SMDJC.json","graph_json":"https://pith.science/api/pith-number/YAZG7OPFBIY23YEVCDKE4SMDJC/graph.json","events_json":"https://pith.science/api/pith-number/YAZG7OPFBIY23YEVCDKE4SMDJC/events.json","paper":"https://pith.science/paper/YAZG7OPF"},"agent_actions":{"view_html":"https://pith.science/pith/YAZG7OPFBIY23YEVCDKE4SMDJC","download_json":"https://pith.science/pith/YAZG7OPFBIY23YEVCDKE4SMDJC.json","view_paper":"https://pith.science/paper/YAZG7OPF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1905.03741&json=true","fetch_graph":"https://pith.science/api/pith-number/YAZG7OPFBIY23YEVCDKE4SMDJC/graph.json","fetch_events":"https://pith.science/api/pith-number/YAZG7OPFBIY23YEVCDKE4SMDJC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YAZG7OPFBIY23YEVCDKE4SMDJC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YAZG7OPFBIY23YEVCDKE4SMDJC/action/storage_attestation","attest_author":"https://pith.science/pith/YAZG7OPFBIY23YEVCDKE4SMDJC/action/author_attestation","sign_citation":"https://pith.science/pith/YAZG7OPFBIY23YEVCDKE4SMDJC/action/citation_signature","submit_replication":"https://pith.science/pith/YAZG7OPFBIY23YEVCDKE4SMDJC/action/replication_record"}},"created_at":"2026-05-17T23:43:02.147981+00:00","updated_at":"2026-05-17T23:43:02.147981+00:00"}