{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:HBWXNME6CYHRJBVFUULCXA5D4I","short_pith_number":"pith:HBWXNME6","schema_version":"1.0","canonical_sha256":"386d76b09e160f1486a5a5162b83a3e230e44fa938acfe8a7ee7068216c7d8df","source":{"kind":"arxiv","id":"1106.5627","version":3},"attestation_state":"computed","paper":{"title":"Millimeter Radio Continuum Emissions as the Activity of Super Massive Black Holes in Nearby Early-Type Galaxies and Low-Luminosity Active Galactic Nuclei","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.CO","authors_text":"Akihiro Doi, Hiroshi Nagai, Kotaro Kohno, Kouichiro Nakanishi, Seiji Kameno","submitted_at":"2011-06-28T11:13:57Z","abstract_excerpt":"We conducted millimeter continuum observations for samples of nearby early-type galaxies (21 sources) and nearby low-luminosity active galactic nuclei (LLAGN; 16 sources) at 100 GHz (3 mm) using the Nobeyama Millimeter Array (NMA). In addition, we performed quasi-simultaneous observations at 150 GHz (2 mm) and 100 GHz for five LLAGNs. Compact nuclear emissions showing flat or inverted spectra at centimeter-to-millimeter wavelengths were found in many LLAGNs and several early-type galaxies. Moreover, significant flux variability was detected in three LLAGNs. These radio properties are similar t"},"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":"1106.5627","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2011-06-28T11:13:57Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"2f9371cee1296be86471731ab6328423ac69edca80fd4a178590df402c50e3c2","abstract_canon_sha256":"8fdab0fa7e245cb27b53d5befe04f364ae4e3ad7819f466e7e086dbc0e9a3966"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:01:29.911692Z","signature_b64":"a0yVRLe+wuqebGYxYNJ0LGNmOKAMf3kXX7omEcvJ/ITQDEhSqPkxFTbykKm81cTsxlutfLBpOGxvO3CptwF0Cw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"386d76b09e160f1486a5a5162b83a3e230e44fa938acfe8a7ee7068216c7d8df","last_reissued_at":"2026-05-18T02:01:29.911285Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:01:29.911285Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Millimeter Radio Continuum Emissions as the Activity of Super Massive Black Holes in Nearby Early-Type Galaxies and Low-Luminosity Active Galactic Nuclei","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.CO","authors_text":"Akihiro Doi, Hiroshi Nagai, Kotaro Kohno, Kouichiro Nakanishi, Seiji Kameno","submitted_at":"2011-06-28T11:13:57Z","abstract_excerpt":"We conducted millimeter continuum observations for samples of nearby early-type galaxies (21 sources) and nearby low-luminosity active galactic nuclei (LLAGN; 16 sources) at 100 GHz (3 mm) using the Nobeyama Millimeter Array (NMA). In addition, we performed quasi-simultaneous observations at 150 GHz (2 mm) and 100 GHz for five LLAGNs. Compact nuclear emissions showing flat or inverted spectra at centimeter-to-millimeter wavelengths were found in many LLAGNs and several early-type galaxies. Moreover, significant flux variability was detected in three LLAGNs. These radio properties are similar t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1106.5627","kind":"arxiv","version":3},"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":"1106.5627","created_at":"2026-05-18T02:01:29.911359+00:00"},{"alias_kind":"arxiv_version","alias_value":"1106.5627v3","created_at":"2026-05-18T02:01:29.911359+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1106.5627","created_at":"2026-05-18T02:01:29.911359+00:00"},{"alias_kind":"pith_short_12","alias_value":"HBWXNME6CYHR","created_at":"2026-05-18T12:26:30.835961+00:00"},{"alias_kind":"pith_short_16","alias_value":"HBWXNME6CYHRJBVF","created_at":"2026-05-18T12:26:30.835961+00:00"},{"alias_kind":"pith_short_8","alias_value":"HBWXNME6","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/HBWXNME6CYHRJBVFUULCXA5D4I","json":"https://pith.science/pith/HBWXNME6CYHRJBVFUULCXA5D4I.json","graph_json":"https://pith.science/api/pith-number/HBWXNME6CYHRJBVFUULCXA5D4I/graph.json","events_json":"https://pith.science/api/pith-number/HBWXNME6CYHRJBVFUULCXA5D4I/events.json","paper":"https://pith.science/paper/HBWXNME6"},"agent_actions":{"view_html":"https://pith.science/pith/HBWXNME6CYHRJBVFUULCXA5D4I","download_json":"https://pith.science/pith/HBWXNME6CYHRJBVFUULCXA5D4I.json","view_paper":"https://pith.science/paper/HBWXNME6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1106.5627&json=true","fetch_graph":"https://pith.science/api/pith-number/HBWXNME6CYHRJBVFUULCXA5D4I/graph.json","fetch_events":"https://pith.science/api/pith-number/HBWXNME6CYHRJBVFUULCXA5D4I/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HBWXNME6CYHRJBVFUULCXA5D4I/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HBWXNME6CYHRJBVFUULCXA5D4I/action/storage_attestation","attest_author":"https://pith.science/pith/HBWXNME6CYHRJBVFUULCXA5D4I/action/author_attestation","sign_citation":"https://pith.science/pith/HBWXNME6CYHRJBVFUULCXA5D4I/action/citation_signature","submit_replication":"https://pith.science/pith/HBWXNME6CYHRJBVFUULCXA5D4I/action/replication_record"}},"created_at":"2026-05-18T02:01:29.911359+00:00","updated_at":"2026-05-18T02:01:29.911359+00:00"}