{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:F7RV7QLQ5MRRPOKMIQYEYQQ5R2","short_pith_number":"pith:F7RV7QLQ","schema_version":"1.0","canonical_sha256":"2fe35fc170eb2317b94c44304c421d8e9300326aaad6306c1ca5088a9512c0c7","source":{"kind":"arxiv","id":"2204.11803","version":1},"attestation_state":"computed","paper":{"title":"Testing High-Energy Emission Models for Blazars with X-ray Polarimetry","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Abel L. Peirson, Ioannis Liodakis, Roger W. Romani","submitted_at":"2022-04-25T17:25:04Z","abstract_excerpt":"Both leptonic and hadronic emission processes may contribute to blazar jet emission; which dominates in blazars's high energy emission component remains an open question. Some intermediate synchrotron peaked blazars transition from their low to high energy emission components in the X-ray band making them excellent laboratories to probe both components simultaneously, and good targets for the newly launched Imaging X-ray Polarimetry Explorer. We characterize the spectral energy distributions for three such blazars: CGRaBS~J0211+1051, TXS~0506+056, and S5~0716+714, predicting their X-ray polari"},"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":"2204.11803","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2022-04-25T17:25:04Z","cross_cats_sorted":[],"title_canon_sha256":"d2b4db2a9e75a23ea02a18e42fa00ee5a83797f59a2dcfc75dcd21af936ffc83","abstract_canon_sha256":"47db0361bd5a1203df989af2dfa6a079c99e224e726b9e3bff0a01a0810273e2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:27:57.644057Z","signature_b64":"IJwcvjzDCazOIdsBN5RrYoa35H6C7EuFV7AEBu9a4oT0xsDp2WrQ8vsLw319x4JIO+VwC5+jKiuomjOufWATCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2fe35fc170eb2317b94c44304c421d8e9300326aaad6306c1ca5088a9512c0c7","last_reissued_at":"2026-07-05T04:27:57.643144Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:27:57.643144Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Testing High-Energy Emission Models for Blazars with X-ray Polarimetry","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Abel L. Peirson, Ioannis Liodakis, Roger W. Romani","submitted_at":"2022-04-25T17:25:04Z","abstract_excerpt":"Both leptonic and hadronic emission processes may contribute to blazar jet emission; which dominates in blazars's high energy emission component remains an open question. Some intermediate synchrotron peaked blazars transition from their low to high energy emission components in the X-ray band making them excellent laboratories to probe both components simultaneously, and good targets for the newly launched Imaging X-ray Polarimetry Explorer. We characterize the spectral energy distributions for three such blazars: CGRaBS~J0211+1051, TXS~0506+056, and S5~0716+714, predicting their X-ray polari"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2204.11803","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/2204.11803/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":"2204.11803","created_at":"2026-07-05T04:27:57.643279+00:00"},{"alias_kind":"arxiv_version","alias_value":"2204.11803v1","created_at":"2026-07-05T04:27:57.643279+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2204.11803","created_at":"2026-07-05T04:27:57.643279+00:00"},{"alias_kind":"pith_short_12","alias_value":"F7RV7QLQ5MRR","created_at":"2026-07-05T04:27:57.643279+00:00"},{"alias_kind":"pith_short_16","alias_value":"F7RV7QLQ5MRRPOKM","created_at":"2026-07-05T04:27:57.643279+00:00"},{"alias_kind":"pith_short_8","alias_value":"F7RV7QLQ","created_at":"2026-07-05T04:27:57.643279+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/F7RV7QLQ5MRRPOKMIQYEYQQ5R2","json":"https://pith.science/pith/F7RV7QLQ5MRRPOKMIQYEYQQ5R2.json","graph_json":"https://pith.science/api/pith-number/F7RV7QLQ5MRRPOKMIQYEYQQ5R2/graph.json","events_json":"https://pith.science/api/pith-number/F7RV7QLQ5MRRPOKMIQYEYQQ5R2/events.json","paper":"https://pith.science/paper/F7RV7QLQ"},"agent_actions":{"view_html":"https://pith.science/pith/F7RV7QLQ5MRRPOKMIQYEYQQ5R2","download_json":"https://pith.science/pith/F7RV7QLQ5MRRPOKMIQYEYQQ5R2.json","view_paper":"https://pith.science/paper/F7RV7QLQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2204.11803&json=true","fetch_graph":"https://pith.science/api/pith-number/F7RV7QLQ5MRRPOKMIQYEYQQ5R2/graph.json","fetch_events":"https://pith.science/api/pith-number/F7RV7QLQ5MRRPOKMIQYEYQQ5R2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/F7RV7QLQ5MRRPOKMIQYEYQQ5R2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/F7RV7QLQ5MRRPOKMIQYEYQQ5R2/action/storage_attestation","attest_author":"https://pith.science/pith/F7RV7QLQ5MRRPOKMIQYEYQQ5R2/action/author_attestation","sign_citation":"https://pith.science/pith/F7RV7QLQ5MRRPOKMIQYEYQQ5R2/action/citation_signature","submit_replication":"https://pith.science/pith/F7RV7QLQ5MRRPOKMIQYEYQQ5R2/action/replication_record"}},"created_at":"2026-07-05T04:27:57.643279+00:00","updated_at":"2026-07-05T04:27:57.643279+00:00"}