{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2008:73DAENZDEPBZKBESGL5SHNGAP7","short_pith_number":"pith:73DAENZD","schema_version":"1.0","canonical_sha256":"fec602372323c395049232fb23b4c07fddd609906acab3fc704de8dea978f652","source":{"kind":"arxiv","id":"0812.0909","version":1},"attestation_state":"computed","paper":{"title":"Catching blazars in the act! GLAST triggers for TeV observation of blazars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"(2) IMPRS for Astronomy, B. Behera (1)(2), Cosmic Physics, Germany, Heidelberg), S. J. Wagner (1) ((1) Landessternwarte, University of Heidelberg","submitted_at":"2008-12-04T11:25:05Z","abstract_excerpt":"The double humped SED (Spectral Energy Distribution) of blazars, and their flaring phenomena can be explained by various leptonic and hadronic models. However, accurate modeling of the high frequency component and clear identification of the correct emission mechanism would require simultaneous measurements in both the MeV-GeV band and the TeV band. Due to the differences in the sensitivity and the field of view of the instruments required to do these measurements, it is essential to identify active states of blazars likely to be detected with TeV instruments.\n  Using a reasonable intergalacti"},"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":"0812.0909","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph","submitted_at":"2008-12-04T11:25:05Z","cross_cats_sorted":[],"title_canon_sha256":"258f7b05833c55d30a1861ac0bee6de992bc29cb0fa9c783339a9274ca015646","abstract_canon_sha256":"3753a844a2fe570c98aa6a632278f0a140f02805487372c4ca8d52eb68ecc670"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:09:04.040714Z","signature_b64":"a5QTDWoFLabZqY/HDx8F3WGK9wHu0NAD4ZjLm/mDnqvMZQJ9H844M5P1joflKgKfx1uXjSNNGPvdl0Rp1H7/DQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fec602372323c395049232fb23b4c07fddd609906acab3fc704de8dea978f652","last_reissued_at":"2026-05-18T04:09:04.040100Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:09:04.040100Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Catching blazars in the act! GLAST triggers for TeV observation of blazars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"(2) IMPRS for Astronomy, B. Behera (1)(2), Cosmic Physics, Germany, Heidelberg), S. J. Wagner (1) ((1) Landessternwarte, University of Heidelberg","submitted_at":"2008-12-04T11:25:05Z","abstract_excerpt":"The double humped SED (Spectral Energy Distribution) of blazars, and their flaring phenomena can be explained by various leptonic and hadronic models. However, accurate modeling of the high frequency component and clear identification of the correct emission mechanism would require simultaneous measurements in both the MeV-GeV band and the TeV band. Due to the differences in the sensitivity and the field of view of the instruments required to do these measurements, it is essential to identify active states of blazars likely to be detected with TeV instruments.\n  Using a reasonable intergalacti"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0812.0909","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":"0812.0909","created_at":"2026-05-18T04:09:04.040179+00:00"},{"alias_kind":"arxiv_version","alias_value":"0812.0909v1","created_at":"2026-05-18T04:09:04.040179+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0812.0909","created_at":"2026-05-18T04:09:04.040179+00:00"},{"alias_kind":"pith_short_12","alias_value":"73DAENZDEPBZ","created_at":"2026-05-18T12:25:56.245647+00:00"},{"alias_kind":"pith_short_16","alias_value":"73DAENZDEPBZKBES","created_at":"2026-05-18T12:25:56.245647+00:00"},{"alias_kind":"pith_short_8","alias_value":"73DAENZD","created_at":"2026-05-18T12:25:56.245647+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/73DAENZDEPBZKBESGL5SHNGAP7","json":"https://pith.science/pith/73DAENZDEPBZKBESGL5SHNGAP7.json","graph_json":"https://pith.science/api/pith-number/73DAENZDEPBZKBESGL5SHNGAP7/graph.json","events_json":"https://pith.science/api/pith-number/73DAENZDEPBZKBESGL5SHNGAP7/events.json","paper":"https://pith.science/paper/73DAENZD"},"agent_actions":{"view_html":"https://pith.science/pith/73DAENZDEPBZKBESGL5SHNGAP7","download_json":"https://pith.science/pith/73DAENZDEPBZKBESGL5SHNGAP7.json","view_paper":"https://pith.science/paper/73DAENZD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0812.0909&json=true","fetch_graph":"https://pith.science/api/pith-number/73DAENZDEPBZKBESGL5SHNGAP7/graph.json","fetch_events":"https://pith.science/api/pith-number/73DAENZDEPBZKBESGL5SHNGAP7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/73DAENZDEPBZKBESGL5SHNGAP7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/73DAENZDEPBZKBESGL5SHNGAP7/action/storage_attestation","attest_author":"https://pith.science/pith/73DAENZDEPBZKBESGL5SHNGAP7/action/author_attestation","sign_citation":"https://pith.science/pith/73DAENZDEPBZKBESGL5SHNGAP7/action/citation_signature","submit_replication":"https://pith.science/pith/73DAENZDEPBZKBESGL5SHNGAP7/action/replication_record"}},"created_at":"2026-05-18T04:09:04.040179+00:00","updated_at":"2026-05-18T04:09:04.040179+00:00"}