{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:UIJYQUMP52VVCW4A3HYNHDCJVJ","short_pith_number":"pith:UIJYQUMP","schema_version":"1.0","canonical_sha256":"a21388518feeab515b80d9f0d38c49aa560537c47c0982858bae6c2e049f1eba","source":{"kind":"arxiv","id":"1401.3573","version":1},"attestation_state":"computed","paper":{"title":"The Agile Alert System For Gamma-Ray Transients","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.IM","authors_text":"A. Argan, A. Bulgarelli, A. Pellizzoni, A. Trois, A.W. Chen, C. Pittori, D. Beneventano, E. Scalise, F. Gianotti, F. Longo, F. Lucarelli, F. Verrecchia, G. Annoni, G. Fanari, G. Pucella, G. Valentini, L. Salotti, M. Cerone, M. Tavani, M. Trifoglio, N. Parmiggiani, P. Giommi, P. Sabatini, P. Santolamazza, P. Tempesta, S. Colafrancesco, S. Vercellone, V. Conforti, V. Fioretti","submitted_at":"2014-01-15T13:21:44Z","abstract_excerpt":"In recent years, a new generation of space missions offered great opportunities of discovery in high-energy astrophysics. In this article we focus on the scientific operations of the Gamma-Ray Imaging Detector (GRID) onboard the AGILE space mission. The AGILE-GRID, sensitive in the energy range of 30 MeV-30 GeV, has detected many gamma-ray transients of galactic and extragalactic origins. This work presents the AGILE innovative approach to fast gamma-ray transient detection, which is a challenging task and a crucial part of the AGILE scientific program. The goals are to describe: (1) the AGILE"},"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":"1401.3573","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2014-01-15T13:21:44Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"833a604a13e8d4783066cf46891dccad72912751544bbe917a2dd7ec6a1f99dd","abstract_canon_sha256":"98a55594392487fafa43cc973c293570a44e10711b63ccd39496f677a874241d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:02:08.394779Z","signature_b64":"DRuNogEUl0AsTULI/7scoYinIpfvZC+5X3Zg/S0A6mg/+VdNG+qA3UVUE+jqr0RgZCqsdAzI+balH+49Nm8JBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a21388518feeab515b80d9f0d38c49aa560537c47c0982858bae6c2e049f1eba","last_reissued_at":"2026-05-18T03:02:08.394006Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:02:08.394006Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Agile Alert System For Gamma-Ray Transients","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.IM","authors_text":"A. Argan, A. Bulgarelli, A. Pellizzoni, A. Trois, A.W. Chen, C. Pittori, D. Beneventano, E. Scalise, F. Gianotti, F. Longo, F. Lucarelli, F. Verrecchia, G. Annoni, G. Fanari, G. Pucella, G. Valentini, L. Salotti, M. Cerone, M. Tavani, M. Trifoglio, N. Parmiggiani, P. Giommi, P. Sabatini, P. Santolamazza, P. Tempesta, S. Colafrancesco, S. Vercellone, V. Conforti, V. Fioretti","submitted_at":"2014-01-15T13:21:44Z","abstract_excerpt":"In recent years, a new generation of space missions offered great opportunities of discovery in high-energy astrophysics. In this article we focus on the scientific operations of the Gamma-Ray Imaging Detector (GRID) onboard the AGILE space mission. The AGILE-GRID, sensitive in the energy range of 30 MeV-30 GeV, has detected many gamma-ray transients of galactic and extragalactic origins. This work presents the AGILE innovative approach to fast gamma-ray transient detection, which is a challenging task and a crucial part of the AGILE scientific program. The goals are to describe: (1) the AGILE"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1401.3573","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":"1401.3573","created_at":"2026-05-18T03:02:08.394125+00:00"},{"alias_kind":"arxiv_version","alias_value":"1401.3573v1","created_at":"2026-05-18T03:02:08.394125+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1401.3573","created_at":"2026-05-18T03:02:08.394125+00:00"},{"alias_kind":"pith_short_12","alias_value":"UIJYQUMP52VV","created_at":"2026-05-18T12:28:52.271510+00:00"},{"alias_kind":"pith_short_16","alias_value":"UIJYQUMP52VVCW4A","created_at":"2026-05-18T12:28:52.271510+00:00"},{"alias_kind":"pith_short_8","alias_value":"UIJYQUMP","created_at":"2026-05-18T12:28:52.271510+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/UIJYQUMP52VVCW4A3HYNHDCJVJ","json":"https://pith.science/pith/UIJYQUMP52VVCW4A3HYNHDCJVJ.json","graph_json":"https://pith.science/api/pith-number/UIJYQUMP52VVCW4A3HYNHDCJVJ/graph.json","events_json":"https://pith.science/api/pith-number/UIJYQUMP52VVCW4A3HYNHDCJVJ/events.json","paper":"https://pith.science/paper/UIJYQUMP"},"agent_actions":{"view_html":"https://pith.science/pith/UIJYQUMP52VVCW4A3HYNHDCJVJ","download_json":"https://pith.science/pith/UIJYQUMP52VVCW4A3HYNHDCJVJ.json","view_paper":"https://pith.science/paper/UIJYQUMP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1401.3573&json=true","fetch_graph":"https://pith.science/api/pith-number/UIJYQUMP52VVCW4A3HYNHDCJVJ/graph.json","fetch_events":"https://pith.science/api/pith-number/UIJYQUMP52VVCW4A3HYNHDCJVJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UIJYQUMP52VVCW4A3HYNHDCJVJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UIJYQUMP52VVCW4A3HYNHDCJVJ/action/storage_attestation","attest_author":"https://pith.science/pith/UIJYQUMP52VVCW4A3HYNHDCJVJ/action/author_attestation","sign_citation":"https://pith.science/pith/UIJYQUMP52VVCW4A3HYNHDCJVJ/action/citation_signature","submit_replication":"https://pith.science/pith/UIJYQUMP52VVCW4A3HYNHDCJVJ/action/replication_record"}},"created_at":"2026-05-18T03:02:08.394125+00:00","updated_at":"2026-05-18T03:02:08.394125+00:00"}