{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:4JL7UJ5VKSYB3T3RENCCWWFGGQ","short_pith_number":"pith:4JL7UJ5V","schema_version":"1.0","canonical_sha256":"e257fa27b554b01dcf7123442b58a6343c5634b6f7c1dfb059fb0031e16f180c","source":{"kind":"arxiv","id":"1610.06625","version":1},"attestation_state":"computed","paper":{"title":"M@TE - Monitoring at TeV Energies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.IM","authors_text":"Daniela Dorner, Gagik Tovmassian, Magdalena Gonzalez, Ruben Alfaro, Thomas Bretz","submitted_at":"2016-10-20T23:15:38Z","abstract_excerpt":"Blazars are extremely variable objects emitting radiation across the electromagnetic spectrum and showing variability on time scales from minutes to years. For the understanding of the emission mechanisms, simultaneous multi-wavelength observations are crucial. Various models for flares predict simultaneous flux increases in the X-ray and gamma-ray band or more complex variability patterns, depending on the dominant process responsible for the gamma-ray emission. Monitoring at TeV energies is providing important information to distinguish between different models. To study duty cycle and varia"},"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":"1610.06625","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2016-10-20T23:15:38Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"8aa645d14e0dc985005a7ea53b57041bb87bf05096f668a52540975eafaa9178","abstract_canon_sha256":"dfbe2e040d7494e8e3f51ad01c00eea121216b14c37a7ef8f090d1fdd78bfd65"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:38:30.971541Z","signature_b64":"RXBxvl0xN8Prf5pt1aAgJYLr5EZVWktBXyTRCx8uzcJmGaMQF7UJAN2avCSArCP/yqlR2TWd6MIaK33qKnpIAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e257fa27b554b01dcf7123442b58a6343c5634b6f7c1dfb059fb0031e16f180c","last_reissued_at":"2026-05-18T00:38:30.970958Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:38:30.970958Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"M@TE - Monitoring at TeV Energies","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.IM","authors_text":"Daniela Dorner, Gagik Tovmassian, Magdalena Gonzalez, Ruben Alfaro, Thomas Bretz","submitted_at":"2016-10-20T23:15:38Z","abstract_excerpt":"Blazars are extremely variable objects emitting radiation across the electromagnetic spectrum and showing variability on time scales from minutes to years. For the understanding of the emission mechanisms, simultaneous multi-wavelength observations are crucial. Various models for flares predict simultaneous flux increases in the X-ray and gamma-ray band or more complex variability patterns, depending on the dominant process responsible for the gamma-ray emission. Monitoring at TeV energies is providing important information to distinguish between different models. To study duty cycle and varia"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1610.06625","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":"1610.06625","created_at":"2026-05-18T00:38:30.971043+00:00"},{"alias_kind":"arxiv_version","alias_value":"1610.06625v1","created_at":"2026-05-18T00:38:30.971043+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1610.06625","created_at":"2026-05-18T00:38:30.971043+00:00"},{"alias_kind":"pith_short_12","alias_value":"4JL7UJ5VKSYB","created_at":"2026-05-18T12:29:58.707656+00:00"},{"alias_kind":"pith_short_16","alias_value":"4JL7UJ5VKSYB3T3R","created_at":"2026-05-18T12:29:58.707656+00:00"},{"alias_kind":"pith_short_8","alias_value":"4JL7UJ5V","created_at":"2026-05-18T12:29:58.707656+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/4JL7UJ5VKSYB3T3RENCCWWFGGQ","json":"https://pith.science/pith/4JL7UJ5VKSYB3T3RENCCWWFGGQ.json","graph_json":"https://pith.science/api/pith-number/4JL7UJ5VKSYB3T3RENCCWWFGGQ/graph.json","events_json":"https://pith.science/api/pith-number/4JL7UJ5VKSYB3T3RENCCWWFGGQ/events.json","paper":"https://pith.science/paper/4JL7UJ5V"},"agent_actions":{"view_html":"https://pith.science/pith/4JL7UJ5VKSYB3T3RENCCWWFGGQ","download_json":"https://pith.science/pith/4JL7UJ5VKSYB3T3RENCCWWFGGQ.json","view_paper":"https://pith.science/paper/4JL7UJ5V","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1610.06625&json=true","fetch_graph":"https://pith.science/api/pith-number/4JL7UJ5VKSYB3T3RENCCWWFGGQ/graph.json","fetch_events":"https://pith.science/api/pith-number/4JL7UJ5VKSYB3T3RENCCWWFGGQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4JL7UJ5VKSYB3T3RENCCWWFGGQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4JL7UJ5VKSYB3T3RENCCWWFGGQ/action/storage_attestation","attest_author":"https://pith.science/pith/4JL7UJ5VKSYB3T3RENCCWWFGGQ/action/author_attestation","sign_citation":"https://pith.science/pith/4JL7UJ5VKSYB3T3RENCCWWFGGQ/action/citation_signature","submit_replication":"https://pith.science/pith/4JL7UJ5VKSYB3T3RENCCWWFGGQ/action/replication_record"}},"created_at":"2026-05-18T00:38:30.971043+00:00","updated_at":"2026-05-18T00:38:30.971043+00:00"}