{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:X3WKVD57WSHAAQ57PZ74J4PPOZ","short_pith_number":"pith:X3WKVD57","schema_version":"1.0","canonical_sha256":"beecaa8fbfb48e0043bf7e7fc4f1ef767df060ba93422bc844c2c26fec284ffb","source":{"kind":"arxiv","id":"2403.17581","version":1},"attestation_state":"computed","paper":{"title":"The power of relativistic jets: a comparative study","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Alan P. Marscher, Benedetta Dalla Barba, Elena Dalla Bont\\`a, Emilia J\\\"arvel\\\"a, Heinz Andernach, Luigi Foschini, Merja Tornikoski, Paola Marziani, Sonia Ant\\'on, Svetlana G. Jorstad","submitted_at":"2024-03-26T10:43:38Z","abstract_excerpt":"We present the results of a comparison between different methods to estimate the power of relativistic jets from active galactic nuclei (AGN). We selected a sample of 32 objects (21 flat-spectrum radio quasars, 7 BL Lacertae Objects, 2 misaligned AGN, and 2 changing-look AGN) from the Very Large Baseline Array (VLBA) observations at 43 GHz of the Boston University blazar program. We then calculated the total, radiative, and kinetic jet power from both radio and high-energy gamma-ray observations, and compare the values. We found an excellent agreement between the radiative power calculated by "},"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":"2403.17581","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2024-03-26T10:43:38Z","cross_cats_sorted":[],"title_canon_sha256":"12f96236f817d97264f38608735ce49132d72038c3dc9749380f4ba0f672289c","abstract_canon_sha256":"dfa54c66176abc3c7c52d5fb9e280687dd7ab0978174a1a12267fbd9e350359d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:00:52.799507Z","signature_b64":"9WUWpLzFH0OyWsgaF0BDCVqfqrAjEN1Sr/5ZO013LOOHo8WMdbWC9uQ8n3IqoxeCx7hqT1hIphXKrCsUaO4IDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"beecaa8fbfb48e0043bf7e7fc4f1ef767df060ba93422bc844c2c26fec284ffb","last_reissued_at":"2026-07-05T08:00:52.798976Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:00:52.798976Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The power of relativistic jets: a comparative study","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Alan P. Marscher, Benedetta Dalla Barba, Elena Dalla Bont\\`a, Emilia J\\\"arvel\\\"a, Heinz Andernach, Luigi Foschini, Merja Tornikoski, Paola Marziani, Sonia Ant\\'on, Svetlana G. Jorstad","submitted_at":"2024-03-26T10:43:38Z","abstract_excerpt":"We present the results of a comparison between different methods to estimate the power of relativistic jets from active galactic nuclei (AGN). We selected a sample of 32 objects (21 flat-spectrum radio quasars, 7 BL Lacertae Objects, 2 misaligned AGN, and 2 changing-look AGN) from the Very Large Baseline Array (VLBA) observations at 43 GHz of the Boston University blazar program. We then calculated the total, radiative, and kinetic jet power from both radio and high-energy gamma-ray observations, and compare the values. We found an excellent agreement between the radiative power calculated by "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2403.17581","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2403.17581/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2403.17581","created_at":"2026-07-05T08:00:52.799040+00:00"},{"alias_kind":"arxiv_version","alias_value":"2403.17581v1","created_at":"2026-07-05T08:00:52.799040+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2403.17581","created_at":"2026-07-05T08:00:52.799040+00:00"},{"alias_kind":"pith_short_12","alias_value":"X3WKVD57WSHA","created_at":"2026-07-05T08:00:52.799040+00:00"},{"alias_kind":"pith_short_16","alias_value":"X3WKVD57WSHAAQ57","created_at":"2026-07-05T08:00:52.799040+00:00"},{"alias_kind":"pith_short_8","alias_value":"X3WKVD57","created_at":"2026-07-05T08:00:52.799040+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2608.08733","citing_title":"Simulation-based inference for AGN jet population modelling: Towards more robust comparisons of black hole jet speeds","ref_index":67,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/X3WKVD57WSHAAQ57PZ74J4PPOZ","json":"https://pith.science/pith/X3WKVD57WSHAAQ57PZ74J4PPOZ.json","graph_json":"https://pith.science/api/pith-number/X3WKVD57WSHAAQ57PZ74J4PPOZ/graph.json","events_json":"https://pith.science/api/pith-number/X3WKVD57WSHAAQ57PZ74J4PPOZ/events.json","paper":"https://pith.science/paper/X3WKVD57"},"agent_actions":{"view_html":"https://pith.science/pith/X3WKVD57WSHAAQ57PZ74J4PPOZ","download_json":"https://pith.science/pith/X3WKVD57WSHAAQ57PZ74J4PPOZ.json","view_paper":"https://pith.science/paper/X3WKVD57","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2403.17581&json=true","fetch_graph":"https://pith.science/api/pith-number/X3WKVD57WSHAAQ57PZ74J4PPOZ/graph.json","fetch_events":"https://pith.science/api/pith-number/X3WKVD57WSHAAQ57PZ74J4PPOZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/X3WKVD57WSHAAQ57PZ74J4PPOZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/X3WKVD57WSHAAQ57PZ74J4PPOZ/action/storage_attestation","attest_author":"https://pith.science/pith/X3WKVD57WSHAAQ57PZ74J4PPOZ/action/author_attestation","sign_citation":"https://pith.science/pith/X3WKVD57WSHAAQ57PZ74J4PPOZ/action/citation_signature","submit_replication":"https://pith.science/pith/X3WKVD57WSHAAQ57PZ74J4PPOZ/action/replication_record"}},"created_at":"2026-07-05T08:00:52.799040+00:00","updated_at":"2026-07-05T08:00:52.799040+00:00"}