{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2008:LUOBAUDVYI2XHMDF6ZFFXS4C4H","short_pith_number":"pith:LUOBAUDV","schema_version":"1.0","canonical_sha256":"5d1c105075c23573b065f64a5bcb82e1c0cbf41f16bd79af6d7e648793787c8f","source":{"kind":"arxiv","id":"0809.3912","version":1},"attestation_state":"computed","paper":{"title":"Monitoring the radio spectra of selected blazars in the Fermi-GST era. The Effelsberg 100 m telescope covering the cm band","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"E. Angelakis, J. A. Zensus, L. Fuhrmann, N. Marchili, T. P. Krichbaum","submitted_at":"2008-09-23T13:34:14Z","abstract_excerpt":"The analysis of the spectral energy distribution variability at frequencies from radio to TeV is a powerful tool in the investigation of the dynamics, the physics and the structure evolution occurring in the most exotic flavour of active galaxies, the blazars. In particular, the presence of {\\sl Fermi-GST} is providing a unique opportunity for such studies delivering $\\gamma$-ray data of unprecedented quality. Here we introduce a monitoring program that has been running at the Effelsberg 100m telescope since January 2007, underpinning a broad multi-frequency collaboration of facilities that co"},"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":"0809.3912","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph","submitted_at":"2008-09-23T13:34:14Z","cross_cats_sorted":[],"title_canon_sha256":"7f675052fc2f6b3fcc7ee5c6a20f6cb9dd0935846b2e7dab2eacf06aff3fdf8f","abstract_canon_sha256":"235d90cc6b11db0d35f19cea24c1c15d44b0afd5887a0527ed2c9d8178be33ab"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:14:32.826214Z","signature_b64":"ANCNyjIrlfG4bIHpj6n1WS83qTCuP4dvycJ9FRvPHIE9zS6CIzM8SA/Vb85THgUEWX1FhtDbX/vXeAIv34cKDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5d1c105075c23573b065f64a5bcb82e1c0cbf41f16bd79af6d7e648793787c8f","last_reissued_at":"2026-07-04T15:14:32.825801Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:14:32.825801Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Monitoring the radio spectra of selected blazars in the Fermi-GST era. The Effelsberg 100 m telescope covering the cm band","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"E. Angelakis, J. A. Zensus, L. Fuhrmann, N. Marchili, T. P. Krichbaum","submitted_at":"2008-09-23T13:34:14Z","abstract_excerpt":"The analysis of the spectral energy distribution variability at frequencies from radio to TeV is a powerful tool in the investigation of the dynamics, the physics and the structure evolution occurring in the most exotic flavour of active galaxies, the blazars. In particular, the presence of {\\sl Fermi-GST} is providing a unique opportunity for such studies delivering $\\gamma$-ray data of unprecedented quality. Here we introduce a monitoring program that has been running at the Effelsberg 100m telescope since January 2007, underpinning a broad multi-frequency collaboration of facilities that co"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0809.3912","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/0809.3912/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":"0809.3912","created_at":"2026-07-04T15:14:32.825859+00:00"},{"alias_kind":"arxiv_version","alias_value":"0809.3912v1","created_at":"2026-07-04T15:14:32.825859+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0809.3912","created_at":"2026-07-04T15:14:32.825859+00:00"},{"alias_kind":"pith_short_12","alias_value":"LUOBAUDVYI2X","created_at":"2026-07-04T15:14:32.825859+00:00"},{"alias_kind":"pith_short_16","alias_value":"LUOBAUDVYI2XHMDF","created_at":"2026-07-04T15:14:32.825859+00:00"},{"alias_kind":"pith_short_8","alias_value":"LUOBAUDV","created_at":"2026-07-04T15:14:32.825859+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/LUOBAUDVYI2XHMDF6ZFFXS4C4H","json":"https://pith.science/pith/LUOBAUDVYI2XHMDF6ZFFXS4C4H.json","graph_json":"https://pith.science/api/pith-number/LUOBAUDVYI2XHMDF6ZFFXS4C4H/graph.json","events_json":"https://pith.science/api/pith-number/LUOBAUDVYI2XHMDF6ZFFXS4C4H/events.json","paper":"https://pith.science/paper/LUOBAUDV"},"agent_actions":{"view_html":"https://pith.science/pith/LUOBAUDVYI2XHMDF6ZFFXS4C4H","download_json":"https://pith.science/pith/LUOBAUDVYI2XHMDF6ZFFXS4C4H.json","view_paper":"https://pith.science/paper/LUOBAUDV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0809.3912&json=true","fetch_graph":"https://pith.science/api/pith-number/LUOBAUDVYI2XHMDF6ZFFXS4C4H/graph.json","fetch_events":"https://pith.science/api/pith-number/LUOBAUDVYI2XHMDF6ZFFXS4C4H/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LUOBAUDVYI2XHMDF6ZFFXS4C4H/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LUOBAUDVYI2XHMDF6ZFFXS4C4H/action/storage_attestation","attest_author":"https://pith.science/pith/LUOBAUDVYI2XHMDF6ZFFXS4C4H/action/author_attestation","sign_citation":"https://pith.science/pith/LUOBAUDVYI2XHMDF6ZFFXS4C4H/action/citation_signature","submit_replication":"https://pith.science/pith/LUOBAUDVYI2XHMDF6ZFFXS4C4H/action/replication_record"}},"created_at":"2026-07-04T15:14:32.825859+00:00","updated_at":"2026-07-04T15:14:32.825859+00:00"}