{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:HLCQZA2C6NB7VKZ6KORARZLKHX","short_pith_number":"pith:HLCQZA2C","schema_version":"1.0","canonical_sha256":"3ac50c8342f343faab3e53a208e56a3dec6aa72c68c929bf3a12c244c7b39fac","source":{"kind":"arxiv","id":"1006.2507","version":2},"attestation_state":"computed","paper":{"title":"Possible gamma-ray emission of radio intermediate AGN III Zw 2 and its implication on the evolution of jets in AGNs","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"H. T. Liu, Jin Zhang, J. M. Bai, Liang Chen","submitted_at":"2010-06-13T02:50:17Z","abstract_excerpt":"AGNs with hard $\\gamma$-ray emission identified so far are radio-loud. III Zw 2 is a radio intermediate AGN with a relativistic jet. We study its spectral energy distribution (SED) and find that the broad band emissions are dominated by the non-thermal emissions from the jet. We model its SED through a synchrotron + inverse Compton (IC) model. The results show that the IC component of III Zw 2 peaks at a few MeV, and the flux density drops rapidly at higher energy with photon index $\\Gamma\\approx3.3$ above 0.1 GeV. The predicted flux is slightly over the sensitivity of $Fermi$/LAT, but it is n"},"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":"1006.2507","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2010-06-13T02:50:17Z","cross_cats_sorted":[],"title_canon_sha256":"4b089db118bcadbe75f7a479698a2f710ca02142a39d241d4252eb52cc5fb421","abstract_canon_sha256":"14100046c10c4c9a4c69c2a09a1aa8c36a9643ef7464987f8039ea6839144cfd"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:41:15.042541Z","signature_b64":"DtwHsYpRcixZrBCk65bSr8oNqE42KWsWwRfcKGjFjeUodvnP8a3Vgurj0eqMLWj3o+H5NJRYOB0dyEE4OBlBAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3ac50c8342f343faab3e53a208e56a3dec6aa72c68c929bf3a12c244c7b39fac","last_reissued_at":"2026-05-18T04:41:15.041951Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:41:15.041951Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Possible gamma-ray emission of radio intermediate AGN III Zw 2 and its implication on the evolution of jets in AGNs","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"H. T. Liu, Jin Zhang, J. M. Bai, Liang Chen","submitted_at":"2010-06-13T02:50:17Z","abstract_excerpt":"AGNs with hard $\\gamma$-ray emission identified so far are radio-loud. III Zw 2 is a radio intermediate AGN with a relativistic jet. We study its spectral energy distribution (SED) and find that the broad band emissions are dominated by the non-thermal emissions from the jet. We model its SED through a synchrotron + inverse Compton (IC) model. The results show that the IC component of III Zw 2 peaks at a few MeV, and the flux density drops rapidly at higher energy with photon index $\\Gamma\\approx3.3$ above 0.1 GeV. The predicted flux is slightly over the sensitivity of $Fermi$/LAT, but it is n"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1006.2507","kind":"arxiv","version":2},"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":"1006.2507","created_at":"2026-05-18T04:41:15.042025+00:00"},{"alias_kind":"arxiv_version","alias_value":"1006.2507v2","created_at":"2026-05-18T04:41:15.042025+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1006.2507","created_at":"2026-05-18T04:41:15.042025+00:00"},{"alias_kind":"pith_short_12","alias_value":"HLCQZA2C6NB7","created_at":"2026-05-18T12:26:07.630475+00:00"},{"alias_kind":"pith_short_16","alias_value":"HLCQZA2C6NB7VKZ6","created_at":"2026-05-18T12:26:07.630475+00:00"},{"alias_kind":"pith_short_8","alias_value":"HLCQZA2C","created_at":"2026-05-18T12:26:07.630475+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/HLCQZA2C6NB7VKZ6KORARZLKHX","json":"https://pith.science/pith/HLCQZA2C6NB7VKZ6KORARZLKHX.json","graph_json":"https://pith.science/api/pith-number/HLCQZA2C6NB7VKZ6KORARZLKHX/graph.json","events_json":"https://pith.science/api/pith-number/HLCQZA2C6NB7VKZ6KORARZLKHX/events.json","paper":"https://pith.science/paper/HLCQZA2C"},"agent_actions":{"view_html":"https://pith.science/pith/HLCQZA2C6NB7VKZ6KORARZLKHX","download_json":"https://pith.science/pith/HLCQZA2C6NB7VKZ6KORARZLKHX.json","view_paper":"https://pith.science/paper/HLCQZA2C","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1006.2507&json=true","fetch_graph":"https://pith.science/api/pith-number/HLCQZA2C6NB7VKZ6KORARZLKHX/graph.json","fetch_events":"https://pith.science/api/pith-number/HLCQZA2C6NB7VKZ6KORARZLKHX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HLCQZA2C6NB7VKZ6KORARZLKHX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HLCQZA2C6NB7VKZ6KORARZLKHX/action/storage_attestation","attest_author":"https://pith.science/pith/HLCQZA2C6NB7VKZ6KORARZLKHX/action/author_attestation","sign_citation":"https://pith.science/pith/HLCQZA2C6NB7VKZ6KORARZLKHX/action/citation_signature","submit_replication":"https://pith.science/pith/HLCQZA2C6NB7VKZ6KORARZLKHX/action/replication_record"}},"created_at":"2026-05-18T04:41:15.042025+00:00","updated_at":"2026-05-18T04:41:15.042025+00:00"}