{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:2GRFAVPWJFAEYPHVW2UR53HNLR","short_pith_number":"pith:2GRFAVPW","schema_version":"1.0","canonical_sha256":"d1a25055f649404c3cf5b6a91eeced5c528c63ab1621d90bda0a5f721d0e2890","source":{"kind":"arxiv","id":"1011.6425","version":1},"attestation_state":"computed","paper":{"title":"A Sino-German 6 cm polarization survey of the Galactic plane III. The region from 10 degree to 60 degree longitude","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"2), C. Wang (1), J. L. Han (1), P. M\\\"uller (2) ((1) NAOC (2) MPIfR), P. Reich (2), R. Wielebinski (2), W. Reich (2), X. H. Sun (1","submitted_at":"2010-11-30T00:51:39Z","abstract_excerpt":"(Abridged) We have conducted a total intensity and polarization survey of the Galactic plane at 6 cm using the Urumqi 25 m telescope for the Galactic longitude range of 10 deg<l<60 deg and the Galactic latitude range of |b|<5 deg. Missing absolute zero levels of Stokes U and Q maps were restored by extrapolating the WMAP five-year K-band polarization data. For total intensities we recovered missing large-scale components by referring to the Effelsberg 11 cm survey. Total intensity and polarization maps are presented with an angular resolution of 9.5 arcmin and a sensitivity of 1 mK and 0.5 mK "},"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":"1011.6425","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2010-11-30T00:51:39Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"1cc1a492893daf1d603c0163c7eab9d32db76aa14fa6e86c7f75d71b2536f22d","abstract_canon_sha256":"cc9f4382e434e771bd17f8154c531307ad8a040c1b8fa471a1cf161df3d900e0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:04:37.507242Z","signature_b64":"ue8gONBXvQc6zYi/juq4C2GwPdcgC1OYcHDGmoF2nbLF/wnANc3uvXfWjWgtjy/HBKUi/6esDMjPxpv3G7uXAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d1a25055f649404c3cf5b6a91eeced5c528c63ab1621d90bda0a5f721d0e2890","last_reissued_at":"2026-05-18T02:04:37.506520Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:04:37.506520Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Sino-German 6 cm polarization survey of the Galactic plane III. The region from 10 degree to 60 degree longitude","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.GA","authors_text":"2), C. Wang (1), J. L. Han (1), P. M\\\"uller (2) ((1) NAOC (2) MPIfR), P. Reich (2), R. Wielebinski (2), W. Reich (2), X. H. Sun (1","submitted_at":"2010-11-30T00:51:39Z","abstract_excerpt":"(Abridged) We have conducted a total intensity and polarization survey of the Galactic plane at 6 cm using the Urumqi 25 m telescope for the Galactic longitude range of 10 deg<l<60 deg and the Galactic latitude range of |b|<5 deg. Missing absolute zero levels of Stokes U and Q maps were restored by extrapolating the WMAP five-year K-band polarization data. For total intensities we recovered missing large-scale components by referring to the Effelsberg 11 cm survey. Total intensity and polarization maps are presented with an angular resolution of 9.5 arcmin and a sensitivity of 1 mK and 0.5 mK "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1011.6425","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":"1011.6425","created_at":"2026-05-18T02:04:37.506653+00:00"},{"alias_kind":"arxiv_version","alias_value":"1011.6425v1","created_at":"2026-05-18T02:04:37.506653+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1011.6425","created_at":"2026-05-18T02:04:37.506653+00:00"},{"alias_kind":"pith_short_12","alias_value":"2GRFAVPWJFAE","created_at":"2026-05-18T12:26:03.138858+00:00"},{"alias_kind":"pith_short_16","alias_value":"2GRFAVPWJFAEYPHV","created_at":"2026-05-18T12:26:03.138858+00:00"},{"alias_kind":"pith_short_8","alias_value":"2GRFAVPW","created_at":"2026-05-18T12:26:03.138858+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/2GRFAVPWJFAEYPHVW2UR53HNLR","json":"https://pith.science/pith/2GRFAVPWJFAEYPHVW2UR53HNLR.json","graph_json":"https://pith.science/api/pith-number/2GRFAVPWJFAEYPHVW2UR53HNLR/graph.json","events_json":"https://pith.science/api/pith-number/2GRFAVPWJFAEYPHVW2UR53HNLR/events.json","paper":"https://pith.science/paper/2GRFAVPW"},"agent_actions":{"view_html":"https://pith.science/pith/2GRFAVPWJFAEYPHVW2UR53HNLR","download_json":"https://pith.science/pith/2GRFAVPWJFAEYPHVW2UR53HNLR.json","view_paper":"https://pith.science/paper/2GRFAVPW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1011.6425&json=true","fetch_graph":"https://pith.science/api/pith-number/2GRFAVPWJFAEYPHVW2UR53HNLR/graph.json","fetch_events":"https://pith.science/api/pith-number/2GRFAVPWJFAEYPHVW2UR53HNLR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2GRFAVPWJFAEYPHVW2UR53HNLR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2GRFAVPWJFAEYPHVW2UR53HNLR/action/storage_attestation","attest_author":"https://pith.science/pith/2GRFAVPWJFAEYPHVW2UR53HNLR/action/author_attestation","sign_citation":"https://pith.science/pith/2GRFAVPWJFAEYPHVW2UR53HNLR/action/citation_signature","submit_replication":"https://pith.science/pith/2GRFAVPWJFAEYPHVW2UR53HNLR/action/replication_record"}},"created_at":"2026-05-18T02:04:37.506653+00:00","updated_at":"2026-05-18T02:04:37.506653+00:00"}