{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2009:J7SXKKE4WVMDWDLBKYMJ7SHI5H","short_pith_number":"pith:J7SXKKE4","schema_version":"1.0","canonical_sha256":"4fe575289cb5583b0d6156189fc8e8e9d57a5e497d42f66312e7a2b788b92b6b","source":{"kind":"arxiv","id":"0910.4261","version":1},"attestation_state":"computed","paper":{"title":"Radio and spectroscopic properties of miniature radio galaxies: revealing the bulk of the radio-loud AGN population","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Alessandro Capetti (2) ((1) Universita' degli Studi di Torino, Italy), Italy (2) INAF - Osservatorio Astronomico di Torino, Ranieri D. Baldi (1)","submitted_at":"2009-10-22T09:23:26Z","abstract_excerpt":"We explore radio and spectroscopic properties of a sample of 14 miniature radio galaxies, i.e. early-type core galaxies hosting radio-loud AGN of extremely low radio power, 10^(27-29) erg s^(-1) Hz^(-1) at 1.4 GHz. Miniature radio galaxies smoothly extend the relationships found for the more powerful FRI radio galaxies between emission line, optical and radio nuclear luminosities to lower levels. However, they have a deficit of a factor of ~100 in extended radio emission with respect to that of the classical example of 3CR/FRI. This is not due to their low luminosity, since we found radio gala"},"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":"0910.4261","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2009-10-22T09:23:26Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"7d95eb6994448ecb518c4d9bc4c2dbed76515babcb4eca52387380aa9b588f77","abstract_canon_sha256":"5f490392e28feafe65f213f4f72046781610ea49fd8b6563a39c0b2904655825"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:11:12.793030Z","signature_b64":"zz9KLGoLhjs4pSxfrTgtV5BXnH/193D4LaevmmMRZY+UNUgy6L5oSu+xrjF8ZWIydwpXVv4Moenb/6wIgDsSDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4fe575289cb5583b0d6156189fc8e8e9d57a5e497d42f66312e7a2b788b92b6b","last_reissued_at":"2026-05-18T02:11:12.792113Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:11:12.792113Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Radio and spectroscopic properties of miniature radio galaxies: revealing the bulk of the radio-loud AGN population","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.CO","authors_text":"Alessandro Capetti (2) ((1) Universita' degli Studi di Torino, Italy), Italy (2) INAF - Osservatorio Astronomico di Torino, Ranieri D. Baldi (1)","submitted_at":"2009-10-22T09:23:26Z","abstract_excerpt":"We explore radio and spectroscopic properties of a sample of 14 miniature radio galaxies, i.e. early-type core galaxies hosting radio-loud AGN of extremely low radio power, 10^(27-29) erg s^(-1) Hz^(-1) at 1.4 GHz. Miniature radio galaxies smoothly extend the relationships found for the more powerful FRI radio galaxies between emission line, optical and radio nuclear luminosities to lower levels. However, they have a deficit of a factor of ~100 in extended radio emission with respect to that of the classical example of 3CR/FRI. This is not due to their low luminosity, since we found radio gala"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0910.4261","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":"0910.4261","created_at":"2026-05-18T02:11:12.792269+00:00"},{"alias_kind":"arxiv_version","alias_value":"0910.4261v1","created_at":"2026-05-18T02:11:12.792269+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0910.4261","created_at":"2026-05-18T02:11:12.792269+00:00"},{"alias_kind":"pith_short_12","alias_value":"J7SXKKE4WVMD","created_at":"2026-05-18T12:26:00.592388+00:00"},{"alias_kind":"pith_short_16","alias_value":"J7SXKKE4WVMDWDLB","created_at":"2026-05-18T12:26:00.592388+00:00"},{"alias_kind":"pith_short_8","alias_value":"J7SXKKE4","created_at":"2026-05-18T12:26:00.592388+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/J7SXKKE4WVMDWDLBKYMJ7SHI5H","json":"https://pith.science/pith/J7SXKKE4WVMDWDLBKYMJ7SHI5H.json","graph_json":"https://pith.science/api/pith-number/J7SXKKE4WVMDWDLBKYMJ7SHI5H/graph.json","events_json":"https://pith.science/api/pith-number/J7SXKKE4WVMDWDLBKYMJ7SHI5H/events.json","paper":"https://pith.science/paper/J7SXKKE4"},"agent_actions":{"view_html":"https://pith.science/pith/J7SXKKE4WVMDWDLBKYMJ7SHI5H","download_json":"https://pith.science/pith/J7SXKKE4WVMDWDLBKYMJ7SHI5H.json","view_paper":"https://pith.science/paper/J7SXKKE4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0910.4261&json=true","fetch_graph":"https://pith.science/api/pith-number/J7SXKKE4WVMDWDLBKYMJ7SHI5H/graph.json","fetch_events":"https://pith.science/api/pith-number/J7SXKKE4WVMDWDLBKYMJ7SHI5H/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/J7SXKKE4WVMDWDLBKYMJ7SHI5H/action/timestamp_anchor","attest_storage":"https://pith.science/pith/J7SXKKE4WVMDWDLBKYMJ7SHI5H/action/storage_attestation","attest_author":"https://pith.science/pith/J7SXKKE4WVMDWDLBKYMJ7SHI5H/action/author_attestation","sign_citation":"https://pith.science/pith/J7SXKKE4WVMDWDLBKYMJ7SHI5H/action/citation_signature","submit_replication":"https://pith.science/pith/J7SXKKE4WVMDWDLBKYMJ7SHI5H/action/replication_record"}},"created_at":"2026-05-18T02:11:12.792269+00:00","updated_at":"2026-05-18T02:11:12.792269+00:00"}