{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1999:HZUXZMKGDFN2UTI6IPPFA5DWLP","short_pith_number":"pith:HZUXZMKG","schema_version":"1.0","canonical_sha256":"3e697cb146195baa4d1e43de5074765be4495d2e51f4b260d83e68bc7d5c2d78","source":{"kind":"arxiv","id":"astro-ph/9906336","version":1},"attestation_state":"computed","paper":{"title":"A Radio Polarimetric Study of the Galactic Center Threads","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Cornelia C. Lang, & Luis Echevarria, Mark Morris","submitted_at":"1999-06-21T17:56:47Z","abstract_excerpt":"Multi-frequency, polarimetric VLA observations of the non-thermal filaments (NTF's), G0.08+0.15, and G359.96+0.09, also known as the Northern and Southern Threads are presented at 20, 6, 3.6 and 2 cm, with high enough spatial resolution to be resolved for the first time at 6 and 3.6 cm. The 20 cm image reveals a wealth of new detail in the radio sources lying within the inner 60 pc of the Galaxy. The Southern Thread has a prominent split along its length, similar to splitting at the ends of previously studied NTF's. With resolutions as fine as 2'', the 3.6 and 6 cm images reveal a high degree "},"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":"astro-ph/9906336","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"1999-06-21T17:56:47Z","cross_cats_sorted":[],"title_canon_sha256":"23531224376a938232fcda38e1e861d7dc80ae526418eaf86100ab010aa714a0","abstract_canon_sha256":"0038940c4cc8d91a9fc1545ee4b4725be0f88fd9961c284c065b2ec0bc6aebc8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:11:20.493208Z","signature_b64":"PIw1zEjqa3S/VcBasB0iAaVJR7IvlJAbMvr84qXZhFUBwq12vQ6vPHC6on/rGI5Vmzw1xvW1wv8QkhJ4RHb4Bg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3e697cb146195baa4d1e43de5074765be4495d2e51f4b260d83e68bc7d5c2d78","last_reissued_at":"2026-07-04T16:11:20.492734Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:11:20.492734Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Radio Polarimetric Study of the Galactic Center Threads","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Cornelia C. Lang, & Luis Echevarria, Mark Morris","submitted_at":"1999-06-21T17:56:47Z","abstract_excerpt":"Multi-frequency, polarimetric VLA observations of the non-thermal filaments (NTF's), G0.08+0.15, and G359.96+0.09, also known as the Northern and Southern Threads are presented at 20, 6, 3.6 and 2 cm, with high enough spatial resolution to be resolved for the first time at 6 and 3.6 cm. The 20 cm image reveals a wealth of new detail in the radio sources lying within the inner 60 pc of the Galaxy. The Southern Thread has a prominent split along its length, similar to splitting at the ends of previously studied NTF's. With resolutions as fine as 2'', the 3.6 and 6 cm images reveal a high degree "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/9906336","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/astro-ph/9906336/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":"astro-ph/9906336","created_at":"2026-07-04T16:11:20.492809+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/9906336v1","created_at":"2026-07-04T16:11:20.492809+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/9906336","created_at":"2026-07-04T16:11:20.492809+00:00"},{"alias_kind":"pith_short_12","alias_value":"HZUXZMKGDFN2","created_at":"2026-07-04T16:11:20.492809+00:00"},{"alias_kind":"pith_short_16","alias_value":"HZUXZMKGDFN2UTI6","created_at":"2026-07-04T16:11:20.492809+00:00"},{"alias_kind":"pith_short_8","alias_value":"HZUXZMKG","created_at":"2026-07-04T16:11:20.492809+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.03314","citing_title":"Exploring the Magnetic Field Structure of the Milky Way with Pulsars in the SKA Era","ref_index":78,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/HZUXZMKGDFN2UTI6IPPFA5DWLP","json":"https://pith.science/pith/HZUXZMKGDFN2UTI6IPPFA5DWLP.json","graph_json":"https://pith.science/api/pith-number/HZUXZMKGDFN2UTI6IPPFA5DWLP/graph.json","events_json":"https://pith.science/api/pith-number/HZUXZMKGDFN2UTI6IPPFA5DWLP/events.json","paper":"https://pith.science/paper/HZUXZMKG"},"agent_actions":{"view_html":"https://pith.science/pith/HZUXZMKGDFN2UTI6IPPFA5DWLP","download_json":"https://pith.science/pith/HZUXZMKGDFN2UTI6IPPFA5DWLP.json","view_paper":"https://pith.science/paper/HZUXZMKG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/9906336&json=true","fetch_graph":"https://pith.science/api/pith-number/HZUXZMKGDFN2UTI6IPPFA5DWLP/graph.json","fetch_events":"https://pith.science/api/pith-number/HZUXZMKGDFN2UTI6IPPFA5DWLP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HZUXZMKGDFN2UTI6IPPFA5DWLP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HZUXZMKGDFN2UTI6IPPFA5DWLP/action/storage_attestation","attest_author":"https://pith.science/pith/HZUXZMKGDFN2UTI6IPPFA5DWLP/action/author_attestation","sign_citation":"https://pith.science/pith/HZUXZMKGDFN2UTI6IPPFA5DWLP/action/citation_signature","submit_replication":"https://pith.science/pith/HZUXZMKGDFN2UTI6IPPFA5DWLP/action/replication_record"}},"created_at":"2026-07-04T16:11:20.492809+00:00","updated_at":"2026-07-04T16:11:20.492809+00:00"}