{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2007:T4QLPUFQJFNMMN357MMNFVKSJT","short_pith_number":"pith:T4QLPUFQ","schema_version":"1.0","canonical_sha256":"9f20b7d0b0495ac6377dfb18d2d5524cd9ad68b1a6feb4ac0782cae73db389df","source":{"kind":"arxiv","id":"0704.3944","version":1},"attestation_state":"computed","paper":{"title":"Simultaneous Radio to (Sub-) mm-Monitoring of Variability and Spectral Shape Evolution of potential GLAST Blazars","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. C. S. Readhead, E. Angelakis, J. A. Zensus, L. Fuhrmann, T. P. Krichbaum","submitted_at":"2007-04-30T14:09:36Z","abstract_excerpt":"The Large Area Telescope (LAT) instrument onboard GLAST offers a tremendous opportunity for future blazar studies. In order to fully benefit from its capabilities and to maximize the scientific return from the LAT, it is of great importance to conduct dedicated multi-frequency monitoring campaigns that will result comprehensive observations. Consequently, we initiated an effort to conduct a GLAST-dedicated, quasi-simultaneous, broad-band flux-density (and polarization) monitoring of potential GLAST blazars with the Effelsberg and OVRO radio telescopes (11cm to 7mm wavelength). Here, we present"},"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":"0704.3944","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2007-04-30T14:09:36Z","cross_cats_sorted":[],"title_canon_sha256":"264aeb9d55a71e573af80127b549a09dbaa4bf6fe8d5078efb991379ef1af1b7","abstract_canon_sha256":"f86d7d98ca2ca7ea9c62dba77a4c604fe0d6914923f41eec4f9ae7dbd926ffd6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:44:18.257954Z","signature_b64":"WyaO0AbdKOI9J5Xnl4fzU0AgeLAOZr9h9GOEVQIve3G0p1zwj8a3HNjnzm5WoEI8iBkJ7M5CFzguWjMR5lI+CQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9f20b7d0b0495ac6377dfb18d2d5524cd9ad68b1a6feb4ac0782cae73db389df","last_reissued_at":"2026-07-04T15:44:18.257607Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:44:18.257607Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Simultaneous Radio to (Sub-) mm-Monitoring of Variability and Spectral Shape Evolution of potential GLAST Blazars","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. C. S. Readhead, E. Angelakis, J. A. Zensus, L. Fuhrmann, T. P. Krichbaum","submitted_at":"2007-04-30T14:09:36Z","abstract_excerpt":"The Large Area Telescope (LAT) instrument onboard GLAST offers a tremendous opportunity for future blazar studies. In order to fully benefit from its capabilities and to maximize the scientific return from the LAT, it is of great importance to conduct dedicated multi-frequency monitoring campaigns that will result comprehensive observations. Consequently, we initiated an effort to conduct a GLAST-dedicated, quasi-simultaneous, broad-band flux-density (and polarization) monitoring of potential GLAST blazars with the Effelsberg and OVRO radio telescopes (11cm to 7mm wavelength). Here, we present"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0704.3944","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/0704.3944/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":"0704.3944","created_at":"2026-07-04T15:44:18.257669+00:00"},{"alias_kind":"arxiv_version","alias_value":"0704.3944v1","created_at":"2026-07-04T15:44:18.257669+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0704.3944","created_at":"2026-07-04T15:44:18.257669+00:00"},{"alias_kind":"pith_short_12","alias_value":"T4QLPUFQJFNM","created_at":"2026-07-04T15:44:18.257669+00:00"},{"alias_kind":"pith_short_16","alias_value":"T4QLPUFQJFNMMN35","created_at":"2026-07-04T15:44:18.257669+00:00"},{"alias_kind":"pith_short_8","alias_value":"T4QLPUFQ","created_at":"2026-07-04T15:44:18.257669+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/T4QLPUFQJFNMMN357MMNFVKSJT","json":"https://pith.science/pith/T4QLPUFQJFNMMN357MMNFVKSJT.json","graph_json":"https://pith.science/api/pith-number/T4QLPUFQJFNMMN357MMNFVKSJT/graph.json","events_json":"https://pith.science/api/pith-number/T4QLPUFQJFNMMN357MMNFVKSJT/events.json","paper":"https://pith.science/paper/T4QLPUFQ"},"agent_actions":{"view_html":"https://pith.science/pith/T4QLPUFQJFNMMN357MMNFVKSJT","download_json":"https://pith.science/pith/T4QLPUFQJFNMMN357MMNFVKSJT.json","view_paper":"https://pith.science/paper/T4QLPUFQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0704.3944&json=true","fetch_graph":"https://pith.science/api/pith-number/T4QLPUFQJFNMMN357MMNFVKSJT/graph.json","fetch_events":"https://pith.science/api/pith-number/T4QLPUFQJFNMMN357MMNFVKSJT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/T4QLPUFQJFNMMN357MMNFVKSJT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/T4QLPUFQJFNMMN357MMNFVKSJT/action/storage_attestation","attest_author":"https://pith.science/pith/T4QLPUFQJFNMMN357MMNFVKSJT/action/author_attestation","sign_citation":"https://pith.science/pith/T4QLPUFQJFNMMN357MMNFVKSJT/action/citation_signature","submit_replication":"https://pith.science/pith/T4QLPUFQJFNMMN357MMNFVKSJT/action/replication_record"}},"created_at":"2026-07-04T15:44:18.257669+00:00","updated_at":"2026-07-04T15:44:18.257669+00:00"}