{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:ZCLFFAIOJB66G5Z6TXUDUD3LFE","short_pith_number":"pith:ZCLFFAIO","schema_version":"1.0","canonical_sha256":"c89652810e487de3773e9de83a0f6b293fa47b0bd72feaf63a137db2c1ccaa0b","source":{"kind":"arxiv","id":"1102.2978","version":2},"attestation_state":"computed","paper":{"title":"A Sino-German 6cm polarization survey of the Galactic plane IV. The region from 60deg to 129deg longitude","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"H. Shi, J. L. Han, L. Xiao, O. Lochner, P. Reich, R. Wielebinski, W. Reich, X. H. Sun","submitted_at":"2011-02-15T06:40:14Z","abstract_excerpt":"Linear polarization of diffuse Galactic emission is a signature of magnetic fields in the interstellar medium of our Galaxy. Observations at high frequencies are less affected by Faraday depolarization than those at lower frequencies and are able to detect polarized emission from more distant Galactic regions. We attempt to perform a sensitive survey of the polarized emission from the Galactic disk at 6 cm wavelength. We made polarization observations of the Galactic plane using the Urumqi 25-m telescope at 6 cm covering the area of 60deg< l <129deg and |b|<5deg. Missing large-scale structures"},"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":"1102.2978","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2011-02-15T06:40:14Z","cross_cats_sorted":[],"title_canon_sha256":"08d32206f303da47a152157670c6e37e7db88dd049835142087f0448fa106275","abstract_canon_sha256":"ed4fb129ef58bb21b3fad12fda087022a51815a00e9370f1a331c95a8255d26e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:03:11.030641Z","signature_b64":"LzD9ozJwpbZBqfjQDY1nZ5uA1m/cLROdwI+OzrmLswHuxYQnl8CxntPloz928wyIvMmdOybOOcy14C+Ctf5qCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c89652810e487de3773e9de83a0f6b293fa47b0bd72feaf63a137db2c1ccaa0b","last_reissued_at":"2026-05-18T02:03:11.030099Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:03:11.030099Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Sino-German 6cm polarization survey of the Galactic plane IV. The region from 60deg to 129deg longitude","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"H. Shi, J. L. Han, L. Xiao, O. Lochner, P. Reich, R. Wielebinski, W. Reich, X. H. Sun","submitted_at":"2011-02-15T06:40:14Z","abstract_excerpt":"Linear polarization of diffuse Galactic emission is a signature of magnetic fields in the interstellar medium of our Galaxy. Observations at high frequencies are less affected by Faraday depolarization than those at lower frequencies and are able to detect polarized emission from more distant Galactic regions. We attempt to perform a sensitive survey of the polarized emission from the Galactic disk at 6 cm wavelength. We made polarization observations of the Galactic plane using the Urumqi 25-m telescope at 6 cm covering the area of 60deg< l <129deg and |b|<5deg. Missing large-scale structures"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1102.2978","kind":"arxiv","version":2},"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":"1102.2978","created_at":"2026-05-18T02:03:11.030168+00:00"},{"alias_kind":"arxiv_version","alias_value":"1102.2978v2","created_at":"2026-05-18T02:03:11.030168+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1102.2978","created_at":"2026-05-18T02:03:11.030168+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZCLFFAIOJB66","created_at":"2026-05-18T12:26:47.523578+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZCLFFAIOJB66G5Z6","created_at":"2026-05-18T12:26:47.523578+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZCLFFAIO","created_at":"2026-05-18T12:26:47.523578+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/ZCLFFAIOJB66G5Z6TXUDUD3LFE","json":"https://pith.science/pith/ZCLFFAIOJB66G5Z6TXUDUD3LFE.json","graph_json":"https://pith.science/api/pith-number/ZCLFFAIOJB66G5Z6TXUDUD3LFE/graph.json","events_json":"https://pith.science/api/pith-number/ZCLFFAIOJB66G5Z6TXUDUD3LFE/events.json","paper":"https://pith.science/paper/ZCLFFAIO"},"agent_actions":{"view_html":"https://pith.science/pith/ZCLFFAIOJB66G5Z6TXUDUD3LFE","download_json":"https://pith.science/pith/ZCLFFAIOJB66G5Z6TXUDUD3LFE.json","view_paper":"https://pith.science/paper/ZCLFFAIO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1102.2978&json=true","fetch_graph":"https://pith.science/api/pith-number/ZCLFFAIOJB66G5Z6TXUDUD3LFE/graph.json","fetch_events":"https://pith.science/api/pith-number/ZCLFFAIOJB66G5Z6TXUDUD3LFE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZCLFFAIOJB66G5Z6TXUDUD3LFE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZCLFFAIOJB66G5Z6TXUDUD3LFE/action/storage_attestation","attest_author":"https://pith.science/pith/ZCLFFAIOJB66G5Z6TXUDUD3LFE/action/author_attestation","sign_citation":"https://pith.science/pith/ZCLFFAIOJB66G5Z6TXUDUD3LFE/action/citation_signature","submit_replication":"https://pith.science/pith/ZCLFFAIOJB66G5Z6TXUDUD3LFE/action/replication_record"}},"created_at":"2026-05-18T02:03:11.030168+00:00","updated_at":"2026-05-18T02:03:11.030168+00:00"}