{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:NJQFJCRAKDPWEAYT3GACM7RTOC","short_pith_number":"pith:NJQFJCRA","schema_version":"1.0","canonical_sha256":"6a60548a2050df620313d980267e3370a60b219991c31473bf2ca511f03e076a","source":{"kind":"arxiv","id":"1508.05898","version":2},"attestation_state":"computed","paper":{"title":"New measurements of $\\Omega_m$ from gamma-ray bursts","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.CO","authors_text":"Elena Zaninoni, Lorenzo Amati, Luca Izzo, Marco Muccino, Massimo Della Valle","submitted_at":"2015-08-24T18:07:30Z","abstract_excerpt":"Context: Data from cosmic microwave background radiation (CMB), baryon acoustic oscillations (BAO), and supernovae Ia (SNe-Ia) support a constant dark energy equation of state with $w_0 \\sim -1$. Measuring the evolution of $w$ along the redshift is one of the most demanding challenges for observational cosmology. Aims: We discuss the existence of a close relation for GRBs, named Combo-relation, based on characteristic parameters of GRB phenomenology such as the prompt intrinsic peak energy $E_{p,i}$, the X-ray afterglow, the initial luminosity of the shallow phase $L_0$, the rest-frame duratio"},"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":"1508.05898","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2015-08-24T18:07:30Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"7220ac1b9fd4bb85a38ba04307c777fab91cc2d6752ffd90c3350ef9fa0f7e99","abstract_canon_sha256":"300f2980737e8157633e358a6a9672f8c2fdfac8f363a86ef803b9b461b65f88"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:29:44.930813Z","signature_b64":"00/cCCLLioNU5bkuokbft6dGaHUzdpYvh8Mdk5nJNaBcq0/CDS51m062ugva2YbwjNbvWvGmHkrGTf5hJnnzCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6a60548a2050df620313d980267e3370a60b219991c31473bf2ca511f03e076a","last_reissued_at":"2026-05-18T01:29:44.930387Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:29:44.930387Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"New measurements of $\\Omega_m$ from gamma-ray bursts","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.CO","authors_text":"Elena Zaninoni, Lorenzo Amati, Luca Izzo, Marco Muccino, Massimo Della Valle","submitted_at":"2015-08-24T18:07:30Z","abstract_excerpt":"Context: Data from cosmic microwave background radiation (CMB), baryon acoustic oscillations (BAO), and supernovae Ia (SNe-Ia) support a constant dark energy equation of state with $w_0 \\sim -1$. Measuring the evolution of $w$ along the redshift is one of the most demanding challenges for observational cosmology. Aims: We discuss the existence of a close relation for GRBs, named Combo-relation, based on characteristic parameters of GRB phenomenology such as the prompt intrinsic peak energy $E_{p,i}$, the X-ray afterglow, the initial luminosity of the shallow phase $L_0$, the rest-frame duratio"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1508.05898","kind":"arxiv","version":2},"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":"1508.05898","created_at":"2026-05-18T01:29:44.930454+00:00"},{"alias_kind":"arxiv_version","alias_value":"1508.05898v2","created_at":"2026-05-18T01:29:44.930454+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1508.05898","created_at":"2026-05-18T01:29:44.930454+00:00"},{"alias_kind":"pith_short_12","alias_value":"NJQFJCRAKDPW","created_at":"2026-05-18T12:29:32.376354+00:00"},{"alias_kind":"pith_short_16","alias_value":"NJQFJCRAKDPWEAYT","created_at":"2026-05-18T12:29:32.376354+00:00"},{"alias_kind":"pith_short_8","alias_value":"NJQFJCRA","created_at":"2026-05-18T12:29:32.376354+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2603.27616","citing_title":"Model-independent test of the cosmic distance duality relation with recent observational data","ref_index":70,"is_internal_anchor":true},{"citing_arxiv_id":"2604.03167","citing_title":"Mapping the redshift drift at various redshifts through cosmography","ref_index":89,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/NJQFJCRAKDPWEAYT3GACM7RTOC","json":"https://pith.science/pith/NJQFJCRAKDPWEAYT3GACM7RTOC.json","graph_json":"https://pith.science/api/pith-number/NJQFJCRAKDPWEAYT3GACM7RTOC/graph.json","events_json":"https://pith.science/api/pith-number/NJQFJCRAKDPWEAYT3GACM7RTOC/events.json","paper":"https://pith.science/paper/NJQFJCRA"},"agent_actions":{"view_html":"https://pith.science/pith/NJQFJCRAKDPWEAYT3GACM7RTOC","download_json":"https://pith.science/pith/NJQFJCRAKDPWEAYT3GACM7RTOC.json","view_paper":"https://pith.science/paper/NJQFJCRA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1508.05898&json=true","fetch_graph":"https://pith.science/api/pith-number/NJQFJCRAKDPWEAYT3GACM7RTOC/graph.json","fetch_events":"https://pith.science/api/pith-number/NJQFJCRAKDPWEAYT3GACM7RTOC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NJQFJCRAKDPWEAYT3GACM7RTOC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NJQFJCRAKDPWEAYT3GACM7RTOC/action/storage_attestation","attest_author":"https://pith.science/pith/NJQFJCRAKDPWEAYT3GACM7RTOC/action/author_attestation","sign_citation":"https://pith.science/pith/NJQFJCRAKDPWEAYT3GACM7RTOC/action/citation_signature","submit_replication":"https://pith.science/pith/NJQFJCRAKDPWEAYT3GACM7RTOC/action/replication_record"}},"created_at":"2026-05-18T01:29:44.930454+00:00","updated_at":"2026-05-18T01:29:44.930454+00:00"}