{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:FZ3ZEJ3D77PFLQ3ST6OQIQYERX","short_pith_number":"pith:FZ3ZEJ3D","schema_version":"1.0","canonical_sha256":"2e77922763ffde55c3729f9d0443048dfb088fec6dea7bf13f4b63b7bda0c8f6","source":{"kind":"arxiv","id":"1101.5342","version":1},"attestation_state":"computed","paper":{"title":"Chandra Discovery of 10 New X-Ray Jets Associated With FR II Radio Core-Selected AGNs in the MOJAVE Sample","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.HE","authors_text":"Brandon Hogan, Herman Marshall, Matthew Lister, Nathan Cooper, Preeti Kharb","submitted_at":"2011-01-27T17:17:46Z","abstract_excerpt":"The Chandra X-ray observatory has proven to be a vital tool for studying high-energy emission processes in jets associated with Active Galactic Nuclei (AGN).We have compiled a sample of 27 AGN selected from the radio flux-limited MOJAVE (Monitoring of Jets in AGN with VLBA Experiments) sample of highly relativistically beamed jets to look for correlations between X-ray and radio emission on kiloparsec scales. The sample consists of all MOJAVE quasars which have over 100 mJy of extended radio emission at 1.4 GHz and a radio structure of at least 3\" in size. Previous Chandra observations have re"},"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":"1101.5342","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2011-01-27T17:17:46Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"3c50ecd59fb59ad8aa8cc28afd7e253ec3ba814004f616b6a0a3439df01f3f02","abstract_canon_sha256":"d51134c51dc987a1b1af1281ab6b2b4c3bcca8a04e96ca664d21761aeda344a8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:03:21.271922Z","signature_b64":"gj3aIAm7HHHx12vhyWErtY2hetN7uw3t5w209ibdELhsCjQNgI6iFs3EOl17CQ5ziwGqF2suQWJ4ogXoCDz7BA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2e77922763ffde55c3729f9d0443048dfb088fec6dea7bf13f4b63b7bda0c8f6","last_reissued_at":"2026-05-18T02:03:21.271361Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:03:21.271361Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Chandra Discovery of 10 New X-Ray Jets Associated With FR II Radio Core-Selected AGNs in the MOJAVE Sample","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.HE","authors_text":"Brandon Hogan, Herman Marshall, Matthew Lister, Nathan Cooper, Preeti Kharb","submitted_at":"2011-01-27T17:17:46Z","abstract_excerpt":"The Chandra X-ray observatory has proven to be a vital tool for studying high-energy emission processes in jets associated with Active Galactic Nuclei (AGN).We have compiled a sample of 27 AGN selected from the radio flux-limited MOJAVE (Monitoring of Jets in AGN with VLBA Experiments) sample of highly relativistically beamed jets to look for correlations between X-ray and radio emission on kiloparsec scales. The sample consists of all MOJAVE quasars which have over 100 mJy of extended radio emission at 1.4 GHz and a radio structure of at least 3\" in size. Previous Chandra observations have re"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1101.5342","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":"1101.5342","created_at":"2026-05-18T02:03:21.271445+00:00"},{"alias_kind":"arxiv_version","alias_value":"1101.5342v1","created_at":"2026-05-18T02:03:21.271445+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1101.5342","created_at":"2026-05-18T02:03:21.271445+00:00"},{"alias_kind":"pith_short_12","alias_value":"FZ3ZEJ3D77PF","created_at":"2026-05-18T12:26:28.662955+00:00"},{"alias_kind":"pith_short_16","alias_value":"FZ3ZEJ3D77PFLQ3S","created_at":"2026-05-18T12:26:28.662955+00:00"},{"alias_kind":"pith_short_8","alias_value":"FZ3ZEJ3D","created_at":"2026-05-18T12:26:28.662955+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/FZ3ZEJ3D77PFLQ3ST6OQIQYERX","json":"https://pith.science/pith/FZ3ZEJ3D77PFLQ3ST6OQIQYERX.json","graph_json":"https://pith.science/api/pith-number/FZ3ZEJ3D77PFLQ3ST6OQIQYERX/graph.json","events_json":"https://pith.science/api/pith-number/FZ3ZEJ3D77PFLQ3ST6OQIQYERX/events.json","paper":"https://pith.science/paper/FZ3ZEJ3D"},"agent_actions":{"view_html":"https://pith.science/pith/FZ3ZEJ3D77PFLQ3ST6OQIQYERX","download_json":"https://pith.science/pith/FZ3ZEJ3D77PFLQ3ST6OQIQYERX.json","view_paper":"https://pith.science/paper/FZ3ZEJ3D","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1101.5342&json=true","fetch_graph":"https://pith.science/api/pith-number/FZ3ZEJ3D77PFLQ3ST6OQIQYERX/graph.json","fetch_events":"https://pith.science/api/pith-number/FZ3ZEJ3D77PFLQ3ST6OQIQYERX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FZ3ZEJ3D77PFLQ3ST6OQIQYERX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FZ3ZEJ3D77PFLQ3ST6OQIQYERX/action/storage_attestation","attest_author":"https://pith.science/pith/FZ3ZEJ3D77PFLQ3ST6OQIQYERX/action/author_attestation","sign_citation":"https://pith.science/pith/FZ3ZEJ3D77PFLQ3ST6OQIQYERX/action/citation_signature","submit_replication":"https://pith.science/pith/FZ3ZEJ3D77PFLQ3ST6OQIQYERX/action/replication_record"}},"created_at":"2026-05-18T02:03:21.271445+00:00","updated_at":"2026-05-18T02:03:21.271445+00:00"}