{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:2REJSZFJQ2O2ZFN7FE6IC2QATO","short_pith_number":"pith:2REJSZFJ","schema_version":"1.0","canonical_sha256":"d4489964a9869dac95bf293c816a009ba2817e1bf18418a203063f72fa211995","source":{"kind":"arxiv","id":"1501.02706","version":1},"attestation_state":"computed","paper":{"title":"A common stochastic process rules gamma-ray burst prompt emission and X-ray flares","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Baldeschi, C. Guidorzi, F. Frontera, L. Amati, R. Margutti, S. Dichiara","submitted_at":"2015-01-12T16:39:27Z","abstract_excerpt":"Prompt gamma-ray and early X-ray afterglow emission in gamma-ray bursts (GRBs) are characterized by a bursty behavior and are often interspersed with long quiescent times. There is compelling evidence that X-ray flares are linked to prompt gamma-rays. However, the physical mechanism that leads to the complex temporal distribution of gamma-ray pulses and X-ray flares is not understood. Here we show that the waiting time distribution (WTD) of pulses and flares exhibits a power-law tail extending over 4 decades with index ~2 and can be the manifestation of a common time-dependent Poisson process."},"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":"1501.02706","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2015-01-12T16:39:27Z","cross_cats_sorted":[],"title_canon_sha256":"1c1d7d7207484d827c9425b792931fd59a1a6b5be68543b29b7a105f1cef2390","abstract_canon_sha256":"58be54f880e4f5b9328ad9ed9b57fecb8352d143fe41416f062610439fa4d766"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:11.588405Z","signature_b64":"1HpWLYPIVcRkeVgSW5eZzzKeWeTeREvjtsRXfES3HRaPP/W22LYI7Vq03jNVm/lMeyXC0rOPmSDV+MO29Tb5BQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d4489964a9869dac95bf293c816a009ba2817e1bf18418a203063f72fa211995","last_reissued_at":"2026-05-18T01:41:11.587733Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:11.587733Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A common stochastic process rules gamma-ray burst prompt emission and X-ray flares","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Baldeschi, C. Guidorzi, F. Frontera, L. Amati, R. Margutti, S. Dichiara","submitted_at":"2015-01-12T16:39:27Z","abstract_excerpt":"Prompt gamma-ray and early X-ray afterglow emission in gamma-ray bursts (GRBs) are characterized by a bursty behavior and are often interspersed with long quiescent times. There is compelling evidence that X-ray flares are linked to prompt gamma-rays. However, the physical mechanism that leads to the complex temporal distribution of gamma-ray pulses and X-ray flares is not understood. Here we show that the waiting time distribution (WTD) of pulses and flares exhibits a power-law tail extending over 4 decades with index ~2 and can be the manifestation of a common time-dependent Poisson process."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1501.02706","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":"1501.02706","created_at":"2026-05-18T01:41:11.587828+00:00"},{"alias_kind":"arxiv_version","alias_value":"1501.02706v1","created_at":"2026-05-18T01:41:11.587828+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1501.02706","created_at":"2026-05-18T01:41:11.587828+00:00"},{"alias_kind":"pith_short_12","alias_value":"2REJSZFJQ2O2","created_at":"2026-05-18T12:29:02.477457+00:00"},{"alias_kind":"pith_short_16","alias_value":"2REJSZFJQ2O2ZFN7","created_at":"2026-05-18T12:29:02.477457+00:00"},{"alias_kind":"pith_short_8","alias_value":"2REJSZFJ","created_at":"2026-05-18T12:29:02.477457+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/2REJSZFJQ2O2ZFN7FE6IC2QATO","json":"https://pith.science/pith/2REJSZFJQ2O2ZFN7FE6IC2QATO.json","graph_json":"https://pith.science/api/pith-number/2REJSZFJQ2O2ZFN7FE6IC2QATO/graph.json","events_json":"https://pith.science/api/pith-number/2REJSZFJQ2O2ZFN7FE6IC2QATO/events.json","paper":"https://pith.science/paper/2REJSZFJ"},"agent_actions":{"view_html":"https://pith.science/pith/2REJSZFJQ2O2ZFN7FE6IC2QATO","download_json":"https://pith.science/pith/2REJSZFJQ2O2ZFN7FE6IC2QATO.json","view_paper":"https://pith.science/paper/2REJSZFJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1501.02706&json=true","fetch_graph":"https://pith.science/api/pith-number/2REJSZFJQ2O2ZFN7FE6IC2QATO/graph.json","fetch_events":"https://pith.science/api/pith-number/2REJSZFJQ2O2ZFN7FE6IC2QATO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2REJSZFJQ2O2ZFN7FE6IC2QATO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2REJSZFJQ2O2ZFN7FE6IC2QATO/action/storage_attestation","attest_author":"https://pith.science/pith/2REJSZFJQ2O2ZFN7FE6IC2QATO/action/author_attestation","sign_citation":"https://pith.science/pith/2REJSZFJQ2O2ZFN7FE6IC2QATO/action/citation_signature","submit_replication":"https://pith.science/pith/2REJSZFJQ2O2ZFN7FE6IC2QATO/action/replication_record"}},"created_at":"2026-05-18T01:41:11.587828+00:00","updated_at":"2026-05-18T01:41:11.587828+00:00"}