{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:JYYB6XJ2OISIQO5FIV7FCPOHTZ","short_pith_number":"pith:JYYB6XJ2","schema_version":"1.0","canonical_sha256":"4e301f5d3a7224883ba5457e513dc79e6a313a330d23eb29c56a783f5458d5d1","source":{"kind":"arxiv","id":"1203.4636","version":2},"attestation_state":"computed","paper":{"title":"A search for AGN in the most extreme UV-selected starbursts using the European VLBI Network","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Basu-Zych, A. Lobanov, A. Ptak, D. Schiminovich, G. Kauffmann, R. Alexandroff, R. A. Overzier, S. Bourke, T. Heckman, Z. Paragi","submitted_at":"2012-03-21T02:28:13Z","abstract_excerpt":"We have used the European VLBI Network (EVN) to observe a sample of Lyman Break Analogs (LBAs), nearby (z < 0.3) galaxies with properties similar to the more distant Lyman Break Galaxies (LBGs). The study of LBGs may help define the feed-back relationship between black holes (BHs) and their host galaxies. Previous VLA observations have shown that the kpc-scale radio emission from LBAs is dominated by starbursts. The main targets of this VLBI experiment were selected because they possessed emission-line properties between starbursts and Type 2 (obscured) AGN. Eight targets (three star-forming L"},"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":"1203.4636","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2012-03-21T02:28:13Z","cross_cats_sorted":[],"title_canon_sha256":"3335a635518ef34e6149f33858f78bd192c4ee92e3ed1f4b134f0375f620d094","abstract_canon_sha256":"1e408b84b80f7e0967d6d52ff5cf6125b74e2a9d1a502e19a35b248c8da5dc55"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:58:05.167949Z","signature_b64":"F59cFdyiEiCs8k9+zASADaLBqeWzRK4CChS8VhMd43FJp9UayFTNosN4nAHNJLJ9A9E3eDXVh/QebUdkQM+sBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4e301f5d3a7224883ba5457e513dc79e6a313a330d23eb29c56a783f5458d5d1","last_reissued_at":"2026-05-18T01:58:05.167349Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:58:05.167349Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A search for AGN in the most extreme UV-selected starbursts using the European VLBI Network","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Basu-Zych, A. Lobanov, A. Ptak, D. Schiminovich, G. Kauffmann, R. Alexandroff, R. A. Overzier, S. Bourke, T. Heckman, Z. Paragi","submitted_at":"2012-03-21T02:28:13Z","abstract_excerpt":"We have used the European VLBI Network (EVN) to observe a sample of Lyman Break Analogs (LBAs), nearby (z < 0.3) galaxies with properties similar to the more distant Lyman Break Galaxies (LBGs). The study of LBGs may help define the feed-back relationship between black holes (BHs) and their host galaxies. Previous VLA observations have shown that the kpc-scale radio emission from LBAs is dominated by starbursts. The main targets of this VLBI experiment were selected because they possessed emission-line properties between starbursts and Type 2 (obscured) AGN. Eight targets (three star-forming L"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1203.4636","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":"1203.4636","created_at":"2026-05-18T01:58:05.167432+00:00"},{"alias_kind":"arxiv_version","alias_value":"1203.4636v2","created_at":"2026-05-18T01:58:05.167432+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1203.4636","created_at":"2026-05-18T01:58:05.167432+00:00"},{"alias_kind":"pith_short_12","alias_value":"JYYB6XJ2OISI","created_at":"2026-05-18T12:27:11.947152+00:00"},{"alias_kind":"pith_short_16","alias_value":"JYYB6XJ2OISIQO5F","created_at":"2026-05-18T12:27:11.947152+00:00"},{"alias_kind":"pith_short_8","alias_value":"JYYB6XJ2","created_at":"2026-05-18T12:27:11.947152+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/JYYB6XJ2OISIQO5FIV7FCPOHTZ","json":"https://pith.science/pith/JYYB6XJ2OISIQO5FIV7FCPOHTZ.json","graph_json":"https://pith.science/api/pith-number/JYYB6XJ2OISIQO5FIV7FCPOHTZ/graph.json","events_json":"https://pith.science/api/pith-number/JYYB6XJ2OISIQO5FIV7FCPOHTZ/events.json","paper":"https://pith.science/paper/JYYB6XJ2"},"agent_actions":{"view_html":"https://pith.science/pith/JYYB6XJ2OISIQO5FIV7FCPOHTZ","download_json":"https://pith.science/pith/JYYB6XJ2OISIQO5FIV7FCPOHTZ.json","view_paper":"https://pith.science/paper/JYYB6XJ2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1203.4636&json=true","fetch_graph":"https://pith.science/api/pith-number/JYYB6XJ2OISIQO5FIV7FCPOHTZ/graph.json","fetch_events":"https://pith.science/api/pith-number/JYYB6XJ2OISIQO5FIV7FCPOHTZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JYYB6XJ2OISIQO5FIV7FCPOHTZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JYYB6XJ2OISIQO5FIV7FCPOHTZ/action/storage_attestation","attest_author":"https://pith.science/pith/JYYB6XJ2OISIQO5FIV7FCPOHTZ/action/author_attestation","sign_citation":"https://pith.science/pith/JYYB6XJ2OISIQO5FIV7FCPOHTZ/action/citation_signature","submit_replication":"https://pith.science/pith/JYYB6XJ2OISIQO5FIV7FCPOHTZ/action/replication_record"}},"created_at":"2026-05-18T01:58:05.167432+00:00","updated_at":"2026-05-18T01:58:05.167432+00:00"}