{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:2LNH77VE5ZKW2DDXANSJK7O3MA","short_pith_number":"pith:2LNH77VE","schema_version":"1.0","canonical_sha256":"d2da7ffea4ee556d0c770364957ddb6022a34ff483eb52609018e28bba4653ca","source":{"kind":"arxiv","id":"1006.5699","version":1},"attestation_state":"computed","paper":{"title":"A relationship between AGN jet power and radio power","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"B. R. McNamara (Univ. Waterloo), C. Jones (CfA), C. L. Carilli (NRAO), K. W. Cavagnolo (Univ. Waterloo), L. Birzan (Leiden Univ.), P. E. J. Nulsen (CfA)","submitted_at":"2010-06-29T18:29:10Z","abstract_excerpt":"Using Chandra X-ray and VLA radio data, we investigate the scaling relationship between jet power, P_jet, and synchrotron luminosity, P_rad. We expand the sample presented in Birzan et al. (2008) to lower radio power by incorporating measurements for 21 gEs to determine if the Birzan et al. (2008) P_jet-P_rad scaling relations are continuous in form and scatter from giant elliptical galaxies (gEs) up to brightest cluster galaxies (BCGs). We find a mean scaling relation of P_jet approximately 5.8x10^43 (P_rad/10^40)^(0.70) erg/s which is continuous over ~6-8 decades in P_jet and P_rad with a sc"},"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":"1006.5699","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2010-06-29T18:29:10Z","cross_cats_sorted":[],"title_canon_sha256":"2579130a2d4045094fe9fee73b8d7aee4061af2b94d9e94b599c3b757fd753cd","abstract_canon_sha256":"86fdd0adaa0e82efa039599b41bc7bd15b26bc1e84f1e6da3f739c2c3ced02be"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:06:34.298215Z","signature_b64":"jts/DmL0NWRBNWFNs4cgoOQdVh5TycsOHqK/Ah6Ul3KRpJ4GaCjYjzimwTlhHSIbTnHSz14bgtMIATwT2UCMDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d2da7ffea4ee556d0c770364957ddb6022a34ff483eb52609018e28bba4653ca","last_reissued_at":"2026-05-18T02:06:34.297402Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:06:34.297402Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A relationship between AGN jet power and radio power","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"B. R. McNamara (Univ. Waterloo), C. Jones (CfA), C. L. Carilli (NRAO), K. W. Cavagnolo (Univ. Waterloo), L. Birzan (Leiden Univ.), P. E. J. Nulsen (CfA)","submitted_at":"2010-06-29T18:29:10Z","abstract_excerpt":"Using Chandra X-ray and VLA radio data, we investigate the scaling relationship between jet power, P_jet, and synchrotron luminosity, P_rad. We expand the sample presented in Birzan et al. (2008) to lower radio power by incorporating measurements for 21 gEs to determine if the Birzan et al. (2008) P_jet-P_rad scaling relations are continuous in form and scatter from giant elliptical galaxies (gEs) up to brightest cluster galaxies (BCGs). We find a mean scaling relation of P_jet approximately 5.8x10^43 (P_rad/10^40)^(0.70) erg/s which is continuous over ~6-8 decades in P_jet and P_rad with a sc"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1006.5699","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":"1006.5699","created_at":"2026-05-18T02:06:34.297533+00:00"},{"alias_kind":"arxiv_version","alias_value":"1006.5699v1","created_at":"2026-05-18T02:06:34.297533+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1006.5699","created_at":"2026-05-18T02:06:34.297533+00:00"},{"alias_kind":"pith_short_12","alias_value":"2LNH77VE5ZKW","created_at":"2026-05-18T12:26:03.138858+00:00"},{"alias_kind":"pith_short_16","alias_value":"2LNH77VE5ZKW2DDX","created_at":"2026-05-18T12:26:03.138858+00:00"},{"alias_kind":"pith_short_8","alias_value":"2LNH77VE","created_at":"2026-05-18T12:26:03.138858+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.21320","citing_title":"FR0 radio galaxy jets -- I. linking jet dynamics and high-energy emission in LEDA 55267 and LEDA 58287","ref_index":36,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/2LNH77VE5ZKW2DDXANSJK7O3MA","json":"https://pith.science/pith/2LNH77VE5ZKW2DDXANSJK7O3MA.json","graph_json":"https://pith.science/api/pith-number/2LNH77VE5ZKW2DDXANSJK7O3MA/graph.json","events_json":"https://pith.science/api/pith-number/2LNH77VE5ZKW2DDXANSJK7O3MA/events.json","paper":"https://pith.science/paper/2LNH77VE"},"agent_actions":{"view_html":"https://pith.science/pith/2LNH77VE5ZKW2DDXANSJK7O3MA","download_json":"https://pith.science/pith/2LNH77VE5ZKW2DDXANSJK7O3MA.json","view_paper":"https://pith.science/paper/2LNH77VE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1006.5699&json=true","fetch_graph":"https://pith.science/api/pith-number/2LNH77VE5ZKW2DDXANSJK7O3MA/graph.json","fetch_events":"https://pith.science/api/pith-number/2LNH77VE5ZKW2DDXANSJK7O3MA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2LNH77VE5ZKW2DDXANSJK7O3MA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2LNH77VE5ZKW2DDXANSJK7O3MA/action/storage_attestation","attest_author":"https://pith.science/pith/2LNH77VE5ZKW2DDXANSJK7O3MA/action/author_attestation","sign_citation":"https://pith.science/pith/2LNH77VE5ZKW2DDXANSJK7O3MA/action/citation_signature","submit_replication":"https://pith.science/pith/2LNH77VE5ZKW2DDXANSJK7O3MA/action/replication_record"}},"created_at":"2026-05-18T02:06:34.297533+00:00","updated_at":"2026-05-18T02:06:34.297533+00:00"}