{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:XTERLQGTG7HH267OL64LBU76UG","short_pith_number":"pith:XTERLQGT","schema_version":"1.0","canonical_sha256":"bcc915c0d337ce7d7bee5fb8b0d3fea18f35799850091be6f15d5f63ad457034","source":{"kind":"arxiv","id":"1612.00953","version":1},"attestation_state":"computed","paper":{"title":"Mass-scaling as a method to constrain outflows and particle acceleration from low-luminosity accreting black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"C. Ceccobello, C. S. Froning, E. Gallo, J. E. Nip, J. Neilsen, M. A. Nowak, P. Crumley, R. M. T. Connors, S. Markoff","submitted_at":"2016-12-03T10:50:56Z","abstract_excerpt":"The `fundamental plane of black hole accretion' (FP), a relation between the radio luminosities ($L_R$), X-ray luminosities ($L_X$), and masses ($M_{BH}$) of hard/quiescent state black hole binaries and low-luminosity active galactic nuclei, suggests some aspects of black hole accretion may be scale invariant. However, key questions still exist concerning the relationship between the inflow/outflow behaviour in the `classic' hard state and quiescence, which may impact this scaling. We show that the broadband spectra of A0620-00 and~\\sgra~(the least luminous stellar mass/supermassive black hole"},"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":"1612.00953","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-12-03T10:50:56Z","cross_cats_sorted":[],"title_canon_sha256":"7ba7a8538c2466121854668d11ce62102fc6a3142ba60c199bd39c01203f41d7","abstract_canon_sha256":"40aa62dff95c3480cd4660b23481e9477d9149cd77a654316dc850ebea573d64"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:46:13.590100Z","signature_b64":"fzA1k+vJQk9pYxuiZivuZRnru2DN5nMpQmWhy6kNvr/gDF1m23NccK5uKOAErZMdkcVFsAgC8zFnljGd8MS1Cw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bcc915c0d337ce7d7bee5fb8b0d3fea18f35799850091be6f15d5f63ad457034","last_reissued_at":"2026-05-18T00:46:13.589605Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:46:13.589605Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Mass-scaling as a method to constrain outflows and particle acceleration from low-luminosity accreting black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"C. Ceccobello, C. S. Froning, E. Gallo, J. E. Nip, J. Neilsen, M. A. Nowak, P. Crumley, R. M. T. Connors, S. Markoff","submitted_at":"2016-12-03T10:50:56Z","abstract_excerpt":"The `fundamental plane of black hole accretion' (FP), a relation between the radio luminosities ($L_R$), X-ray luminosities ($L_X$), and masses ($M_{BH}$) of hard/quiescent state black hole binaries and low-luminosity active galactic nuclei, suggests some aspects of black hole accretion may be scale invariant. However, key questions still exist concerning the relationship between the inflow/outflow behaviour in the `classic' hard state and quiescence, which may impact this scaling. We show that the broadband spectra of A0620-00 and~\\sgra~(the least luminous stellar mass/supermassive black hole"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1612.00953","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":"1612.00953","created_at":"2026-05-18T00:46:13.589682+00:00"},{"alias_kind":"arxiv_version","alias_value":"1612.00953v1","created_at":"2026-05-18T00:46:13.589682+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1612.00953","created_at":"2026-05-18T00:46:13.589682+00:00"},{"alias_kind":"pith_short_12","alias_value":"XTERLQGTG7HH","created_at":"2026-05-18T12:30:51.357362+00:00"},{"alias_kind":"pith_short_16","alias_value":"XTERLQGTG7HH267O","created_at":"2026-05-18T12:30:51.357362+00:00"},{"alias_kind":"pith_short_8","alias_value":"XTERLQGT","created_at":"2026-05-18T12:30:51.357362+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/XTERLQGTG7HH267OL64LBU76UG","json":"https://pith.science/pith/XTERLQGTG7HH267OL64LBU76UG.json","graph_json":"https://pith.science/api/pith-number/XTERLQGTG7HH267OL64LBU76UG/graph.json","events_json":"https://pith.science/api/pith-number/XTERLQGTG7HH267OL64LBU76UG/events.json","paper":"https://pith.science/paper/XTERLQGT"},"agent_actions":{"view_html":"https://pith.science/pith/XTERLQGTG7HH267OL64LBU76UG","download_json":"https://pith.science/pith/XTERLQGTG7HH267OL64LBU76UG.json","view_paper":"https://pith.science/paper/XTERLQGT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1612.00953&json=true","fetch_graph":"https://pith.science/api/pith-number/XTERLQGTG7HH267OL64LBU76UG/graph.json","fetch_events":"https://pith.science/api/pith-number/XTERLQGTG7HH267OL64LBU76UG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XTERLQGTG7HH267OL64LBU76UG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XTERLQGTG7HH267OL64LBU76UG/action/storage_attestation","attest_author":"https://pith.science/pith/XTERLQGTG7HH267OL64LBU76UG/action/author_attestation","sign_citation":"https://pith.science/pith/XTERLQGTG7HH267OL64LBU76UG/action/citation_signature","submit_replication":"https://pith.science/pith/XTERLQGTG7HH267OL64LBU76UG/action/replication_record"}},"created_at":"2026-05-18T00:46:13.589682+00:00","updated_at":"2026-05-18T00:46:13.589682+00:00"}