{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:7WBJI7R2GMGOHBLKAXORPJKUID","short_pith_number":"pith:7WBJI7R2","schema_version":"1.0","canonical_sha256":"fd82947e3a330ce3856a05dd17a55440e6ca2351cb9a2ec26897686ea636ada7","source":{"kind":"arxiv","id":"2006.08757","version":3},"attestation_state":"computed","paper":{"title":"Gamma-ray emission revealed at the western edge of SNR G344.7-0.1","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Vendrasco, D. Castro, J. Eagle, M. Ajello, S. Marchesi","submitted_at":"2020-06-15T20:50:03Z","abstract_excerpt":"We report on the investigation of a very high energy (VHE), Galactic gamma-ray source recently discovered at >50GeV using the Large Area Telescope (LAT) on board the Fermi Gamma-Ray Space Telescope. This object, 2FHL J1703.4-4145, displays a very hard >50GeV spectrum with a photon index ~1.2 in the 2FHL catalog and, as such, is one of the most extreme sources in the 2FHL sub-sample of Galactic objects. A detailed analysis of the available multi-wavelength data shows that this source is located on the western edge of the supernova remnant (SNR) G344.7--0.1, along with extended TeV source, HESS "},"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":"2006.08757","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2020-06-15T20:50:03Z","cross_cats_sorted":[],"title_canon_sha256":"72e87e99e2e77becbe6b6ef05a7e6d9813851c2ad0c3c1cab50d0d134a014f6e","abstract_canon_sha256":"cc5b0e4cce92dd43804985c0dfacb4c804c2dd3f4ecde257430785fd5f347ecd"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:55:56.449015Z","signature_b64":"GIJkTd43X5aWblWSXe4G73xvUu7+gT/7znHa1Gp+r4uNV/XWo20+xcA2sWJaGW6UnBxtUZA1Tv+KhQdNKT2DAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fd82947e3a330ce3856a05dd17a55440e6ca2351cb9a2ec26897686ea636ada7","last_reissued_at":"2026-07-05T01:55:56.448541Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:55:56.448541Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gamma-ray emission revealed at the western edge of SNR G344.7-0.1","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Vendrasco, D. Castro, J. Eagle, M. Ajello, S. Marchesi","submitted_at":"2020-06-15T20:50:03Z","abstract_excerpt":"We report on the investigation of a very high energy (VHE), Galactic gamma-ray source recently discovered at >50GeV using the Large Area Telescope (LAT) on board the Fermi Gamma-Ray Space Telescope. This object, 2FHL J1703.4-4145, displays a very hard >50GeV spectrum with a photon index ~1.2 in the 2FHL catalog and, as such, is one of the most extreme sources in the 2FHL sub-sample of Galactic objects. A detailed analysis of the available multi-wavelength data shows that this source is located on the western edge of the supernova remnant (SNR) G344.7--0.1, along with extended TeV source, HESS "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2006.08757","kind":"arxiv","version":3},"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/2006.08757/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":"2006.08757","created_at":"2026-07-05T01:55:56.448595+00:00"},{"alias_kind":"arxiv_version","alias_value":"2006.08757v3","created_at":"2026-07-05T01:55:56.448595+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2006.08757","created_at":"2026-07-05T01:55:56.448595+00:00"},{"alias_kind":"pith_short_12","alias_value":"7WBJI7R2GMGO","created_at":"2026-07-05T01:55:56.448595+00:00"},{"alias_kind":"pith_short_16","alias_value":"7WBJI7R2GMGOHBLK","created_at":"2026-07-05T01:55:56.448595+00:00"},{"alias_kind":"pith_short_8","alias_value":"7WBJI7R2","created_at":"2026-07-05T01:55:56.448595+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/7WBJI7R2GMGOHBLKAXORPJKUID","json":"https://pith.science/pith/7WBJI7R2GMGOHBLKAXORPJKUID.json","graph_json":"https://pith.science/api/pith-number/7WBJI7R2GMGOHBLKAXORPJKUID/graph.json","events_json":"https://pith.science/api/pith-number/7WBJI7R2GMGOHBLKAXORPJKUID/events.json","paper":"https://pith.science/paper/7WBJI7R2"},"agent_actions":{"view_html":"https://pith.science/pith/7WBJI7R2GMGOHBLKAXORPJKUID","download_json":"https://pith.science/pith/7WBJI7R2GMGOHBLKAXORPJKUID.json","view_paper":"https://pith.science/paper/7WBJI7R2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2006.08757&json=true","fetch_graph":"https://pith.science/api/pith-number/7WBJI7R2GMGOHBLKAXORPJKUID/graph.json","fetch_events":"https://pith.science/api/pith-number/7WBJI7R2GMGOHBLKAXORPJKUID/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7WBJI7R2GMGOHBLKAXORPJKUID/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7WBJI7R2GMGOHBLKAXORPJKUID/action/storage_attestation","attest_author":"https://pith.science/pith/7WBJI7R2GMGOHBLKAXORPJKUID/action/author_attestation","sign_citation":"https://pith.science/pith/7WBJI7R2GMGOHBLKAXORPJKUID/action/citation_signature","submit_replication":"https://pith.science/pith/7WBJI7R2GMGOHBLKAXORPJKUID/action/replication_record"}},"created_at":"2026-07-05T01:55:56.448595+00:00","updated_at":"2026-07-05T01:55:56.448595+00:00"}