{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:HQVKHSDE6XJA63YASDQPQGWTKQ","short_pith_number":"pith:HQVKHSDE","schema_version":"1.0","canonical_sha256":"3c2aa3c864f5d20f6f0090e0f81ad354087e4e7d45cd45d263c7f00ca81216a2","source":{"kind":"arxiv","id":"1108.0401","version":1},"attestation_state":"computed","paper":{"title":"Deep Radio Continuum Imaging of the Dwarf Irregular Galaxy IC10: Tracing Star Formation and Magnetic Fields","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"(2) NRAO, (3) Lowell Observatory), Deirdre A. Hunter (3) ((1) University of Hertfordshire, Elias Brinks (1), Michael Rupen (2), Urvashi Rau (2), Volker Heesen (1)","submitted_at":"2011-08-01T19:35:38Z","abstract_excerpt":"We exploit the vastly increased sensitivity of the Expanded Very Large Array (EVLA) to study the radio continuum and polarization properties of the post-starburst, dwarf irregular galaxy IC10 at 6 cm, at a linear resolution of ~50 pc. We find close agreement between radio continuum and Halpha emission, from the brightest HII regions to the weaker emission in the disk. A quantitative analysis shows a strictly linear correlation, where the thermal component contributes 50% to the total radio emission, the remainder being due to a non-thermal component with a surprisingly steep radio spectral ind"},"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":"1108.0401","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2011-08-01T19:35:38Z","cross_cats_sorted":[],"title_canon_sha256":"6e5912539d0ec74a558833a9311f4f41b66dfc8d4f261da798411ba6ec5153d8","abstract_canon_sha256":"7c1c71f76a915855db947efd111e1ea7026c5f33cbfd47563a066d9d086a1a97"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:01:04.725304Z","signature_b64":"a7tpBV3+gLHmg7I+oBaYTB9PEhjuSHNZNZjq1oIq4i1kjdRb4ZVRJciO3X+VLSDrOYYmO9vwlqmacU8Cn3B4Bg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3c2aa3c864f5d20f6f0090e0f81ad354087e4e7d45cd45d263c7f00ca81216a2","last_reissued_at":"2026-05-18T02:01:04.724571Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:01:04.724571Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Deep Radio Continuum Imaging of the Dwarf Irregular Galaxy IC10: Tracing Star Formation and Magnetic Fields","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"(2) NRAO, (3) Lowell Observatory), Deirdre A. Hunter (3) ((1) University of Hertfordshire, Elias Brinks (1), Michael Rupen (2), Urvashi Rau (2), Volker Heesen (1)","submitted_at":"2011-08-01T19:35:38Z","abstract_excerpt":"We exploit the vastly increased sensitivity of the Expanded Very Large Array (EVLA) to study the radio continuum and polarization properties of the post-starburst, dwarf irregular galaxy IC10 at 6 cm, at a linear resolution of ~50 pc. We find close agreement between radio continuum and Halpha emission, from the brightest HII regions to the weaker emission in the disk. A quantitative analysis shows a strictly linear correlation, where the thermal component contributes 50% to the total radio emission, the remainder being due to a non-thermal component with a surprisingly steep radio spectral ind"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1108.0401","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":"1108.0401","created_at":"2026-05-18T02:01:04.724696+00:00"},{"alias_kind":"arxiv_version","alias_value":"1108.0401v1","created_at":"2026-05-18T02:01:04.724696+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1108.0401","created_at":"2026-05-18T02:01:04.724696+00:00"},{"alias_kind":"pith_short_12","alias_value":"HQVKHSDE6XJA","created_at":"2026-05-18T12:26:30.835961+00:00"},{"alias_kind":"pith_short_16","alias_value":"HQVKHSDE6XJA63YA","created_at":"2026-05-18T12:26:30.835961+00:00"},{"alias_kind":"pith_short_8","alias_value":"HQVKHSDE","created_at":"2026-05-18T12:26:30.835961+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/HQVKHSDE6XJA63YASDQPQGWTKQ","json":"https://pith.science/pith/HQVKHSDE6XJA63YASDQPQGWTKQ.json","graph_json":"https://pith.science/api/pith-number/HQVKHSDE6XJA63YASDQPQGWTKQ/graph.json","events_json":"https://pith.science/api/pith-number/HQVKHSDE6XJA63YASDQPQGWTKQ/events.json","paper":"https://pith.science/paper/HQVKHSDE"},"agent_actions":{"view_html":"https://pith.science/pith/HQVKHSDE6XJA63YASDQPQGWTKQ","download_json":"https://pith.science/pith/HQVKHSDE6XJA63YASDQPQGWTKQ.json","view_paper":"https://pith.science/paper/HQVKHSDE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1108.0401&json=true","fetch_graph":"https://pith.science/api/pith-number/HQVKHSDE6XJA63YASDQPQGWTKQ/graph.json","fetch_events":"https://pith.science/api/pith-number/HQVKHSDE6XJA63YASDQPQGWTKQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HQVKHSDE6XJA63YASDQPQGWTKQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HQVKHSDE6XJA63YASDQPQGWTKQ/action/storage_attestation","attest_author":"https://pith.science/pith/HQVKHSDE6XJA63YASDQPQGWTKQ/action/author_attestation","sign_citation":"https://pith.science/pith/HQVKHSDE6XJA63YASDQPQGWTKQ/action/citation_signature","submit_replication":"https://pith.science/pith/HQVKHSDE6XJA63YASDQPQGWTKQ/action/replication_record"}},"created_at":"2026-05-18T02:01:04.724696+00:00","updated_at":"2026-05-18T02:01:04.724696+00:00"}