{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2001:LTTI5WTQDKEMT2ZLG2M3NTKFK2","short_pith_number":"pith:LTTI5WTQ","schema_version":"1.0","canonical_sha256":"5ce68eda701a88c9eb2b3699b6cd4556ad3db87ce3d80f88e3ac228c4dcd5375","source":{"kind":"arxiv","id":"astro-ph/0101322","version":1},"attestation_state":"computed","paper":{"title":"A radio continuum survey of the southern sky at 1420 MHz. Observations and data reduction","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"(2) MPI fuer Radioastronomie, A.J. Sanz (1) ((1) Instituto Argentino de Radioastronomia, Argentina, Bonn, E.E. Hurrel (1), F. R. Colomb (1), Germany), J.A. Bava (1), J.C. Testori (1), J.J. Larrarte (1), P. Reich (2), W. Reich (2)","submitted_at":"2001-01-18T09:47:01Z","abstract_excerpt":"We describe the equipment, observational method and reduction procedure of an absolutely calibrated radio continuum survey of the South Celestial Hemisphere at a frequency of 1420 MHz. These observations cover the area 0h < R.A. < 24h for declinations less than -10 degree. The sensitivity is about 50 mK T_B (full beam brightness) and the angular resolution (HPBW) is 35.4', which matches the existing northern sky survey at the same frequency."},"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/0101322","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2001-01-18T09:47:01Z","cross_cats_sorted":[],"title_canon_sha256":"42791910f73d31498c257d36759a2a61981560f1f4f276b261cce5632f9d9fcb","abstract_canon_sha256":"17f751b642b3e6471341b14a64669572401f36428116b252dfd8ea743414fee0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:22:35.602527Z","signature_b64":"HUHixIuDyT5H05gTcGqk7cISXBKdNlEdGjNLr9p0SC9F1NMDLHHhmT9/urM29fH8kHSp0OzwvsvxQG6i0mbTAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5ce68eda701a88c9eb2b3699b6cd4556ad3db87ce3d80f88e3ac228c4dcd5375","last_reissued_at":"2026-07-04T16:22:35.602102Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:22:35.602102Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A radio continuum survey of the southern sky at 1420 MHz. Observations and data reduction","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"(2) MPI fuer Radioastronomie, A.J. Sanz (1) ((1) Instituto Argentino de Radioastronomia, Argentina, Bonn, E.E. Hurrel (1), F. R. Colomb (1), Germany), J.A. Bava (1), J.C. Testori (1), J.J. Larrarte (1), P. Reich (2), W. Reich (2)","submitted_at":"2001-01-18T09:47:01Z","abstract_excerpt":"We describe the equipment, observational method and reduction procedure of an absolutely calibrated radio continuum survey of the South Celestial Hemisphere at a frequency of 1420 MHz. These observations cover the area 0h < R.A. < 24h for declinations less than -10 degree. The sensitivity is about 50 mK T_B (full beam brightness) and the angular resolution (HPBW) is 35.4', which matches the existing northern sky survey at the same frequency."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0101322","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/0101322/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/0101322","created_at":"2026-07-04T16:22:35.602168+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0101322v1","created_at":"2026-07-04T16:22:35.602168+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0101322","created_at":"2026-07-04T16:22:35.602168+00:00"},{"alias_kind":"pith_short_12","alias_value":"LTTI5WTQDKEM","created_at":"2026-07-04T16:22:35.602168+00:00"},{"alias_kind":"pith_short_16","alias_value":"LTTI5WTQDKEMT2ZL","created_at":"2026-07-04T16:22:35.602168+00:00"},{"alias_kind":"pith_short_8","alias_value":"LTTI5WTQ","created_at":"2026-07-04T16:22:35.602168+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2601.19386","citing_title":"Constraints on Primordial Black Holes from Galactic Diffuse Synchrotron Emissions","ref_index":167,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LTTI5WTQDKEMT2ZLG2M3NTKFK2","json":"https://pith.science/pith/LTTI5WTQDKEMT2ZLG2M3NTKFK2.json","graph_json":"https://pith.science/api/pith-number/LTTI5WTQDKEMT2ZLG2M3NTKFK2/graph.json","events_json":"https://pith.science/api/pith-number/LTTI5WTQDKEMT2ZLG2M3NTKFK2/events.json","paper":"https://pith.science/paper/LTTI5WTQ"},"agent_actions":{"view_html":"https://pith.science/pith/LTTI5WTQDKEMT2ZLG2M3NTKFK2","download_json":"https://pith.science/pith/LTTI5WTQDKEMT2ZLG2M3NTKFK2.json","view_paper":"https://pith.science/paper/LTTI5WTQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0101322&json=true","fetch_graph":"https://pith.science/api/pith-number/LTTI5WTQDKEMT2ZLG2M3NTKFK2/graph.json","fetch_events":"https://pith.science/api/pith-number/LTTI5WTQDKEMT2ZLG2M3NTKFK2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LTTI5WTQDKEMT2ZLG2M3NTKFK2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LTTI5WTQDKEMT2ZLG2M3NTKFK2/action/storage_attestation","attest_author":"https://pith.science/pith/LTTI5WTQDKEMT2ZLG2M3NTKFK2/action/author_attestation","sign_citation":"https://pith.science/pith/LTTI5WTQDKEMT2ZLG2M3NTKFK2/action/citation_signature","submit_replication":"https://pith.science/pith/LTTI5WTQDKEMT2ZLG2M3NTKFK2/action/replication_record"}},"created_at":"2026-07-04T16:22:35.602168+00:00","updated_at":"2026-07-04T16:22:35.602168+00:00"}