{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:DSOVGJQ4LSILBKWNIBRVCMIYGY","short_pith_number":"pith:DSOVGJQ4","schema_version":"1.0","canonical_sha256":"1c9d53261c5c90b0aacd40635131183630614cfaafa72d66d0fac216a64dc186","source":{"kind":"arxiv","id":"1905.12357","version":1},"attestation_state":"computed","paper":{"title":"Constraints on the environment and energetics of the Broad-Line Ic SN2014ad from deep radio and X-ray observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Kamble, C. Guidorzi, D. L. Coppejans, M. Marongiu, R. Margutti, R. Martone","submitted_at":"2019-05-29T12:06:18Z","abstract_excerpt":"Broad-line type Ic Supernovae (BL-Ic SNe) are characterized by high ejecta velocity ($\\gtrsim 10^4$ km s$^{-1}$) and are sometimes associated with the relativistic jets typical of long duration ($\\gtrsim 2$ s) Gamma-Ray Bursts (L-GRBs). The reason why a small fraction of BL-Ic SNe harbor relativistic jets is not known. Here we present deep X-ray and radio observations of the BL-Ic SN2014ad extending from $13$ to $930$ days post explosion. SN2014ad was not detected at either frequency and has no observational evidence of a GRB counterpart. The proximity of SN2014ad ($d\\sim 26$ Mpc) enables very"},"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":"1905.12357","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2019-05-29T12:06:18Z","cross_cats_sorted":[],"title_canon_sha256":"91dd983aaab9dc19e239df25b2e2725cabdddbaf2f2c33d6f46e1a9f8a1a4014","abstract_canon_sha256":"6f566fef3599873a88c2fcf857ea884fd6f90e4cf98ff8857f3c9636d8b7747f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:40:43.234296Z","signature_b64":"H6RsR7y3rOM6pdudL7+sMSr+5QD25z8Fu26r5wq8vpH1D7VwVq8nJgK0z94cR1QDJ11BwIGgTseG+HxFsCb/AQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1c9d53261c5c90b0aacd40635131183630614cfaafa72d66d0fac216a64dc186","last_reissued_at":"2026-05-17T23:40:43.233574Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:40:43.233574Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Constraints on the environment and energetics of the Broad-Line Ic SN2014ad from deep radio and X-ray observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Kamble, C. Guidorzi, D. L. Coppejans, M. Marongiu, R. Margutti, R. Martone","submitted_at":"2019-05-29T12:06:18Z","abstract_excerpt":"Broad-line type Ic Supernovae (BL-Ic SNe) are characterized by high ejecta velocity ($\\gtrsim 10^4$ km s$^{-1}$) and are sometimes associated with the relativistic jets typical of long duration ($\\gtrsim 2$ s) Gamma-Ray Bursts (L-GRBs). The reason why a small fraction of BL-Ic SNe harbor relativistic jets is not known. Here we present deep X-ray and radio observations of the BL-Ic SN2014ad extending from $13$ to $930$ days post explosion. SN2014ad was not detected at either frequency and has no observational evidence of a GRB counterpart. The proximity of SN2014ad ($d\\sim 26$ Mpc) enables very"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1905.12357","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":"1905.12357","created_at":"2026-05-17T23:40:43.233661+00:00"},{"alias_kind":"arxiv_version","alias_value":"1905.12357v1","created_at":"2026-05-17T23:40:43.233661+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1905.12357","created_at":"2026-05-17T23:40:43.233661+00:00"},{"alias_kind":"pith_short_12","alias_value":"DSOVGJQ4LSIL","created_at":"2026-05-18T12:33:15.570797+00:00"},{"alias_kind":"pith_short_16","alias_value":"DSOVGJQ4LSILBKWN","created_at":"2026-05-18T12:33:15.570797+00:00"},{"alias_kind":"pith_short_8","alias_value":"DSOVGJQ4","created_at":"2026-05-18T12:33:15.570797+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/DSOVGJQ4LSILBKWNIBRVCMIYGY","json":"https://pith.science/pith/DSOVGJQ4LSILBKWNIBRVCMIYGY.json","graph_json":"https://pith.science/api/pith-number/DSOVGJQ4LSILBKWNIBRVCMIYGY/graph.json","events_json":"https://pith.science/api/pith-number/DSOVGJQ4LSILBKWNIBRVCMIYGY/events.json","paper":"https://pith.science/paper/DSOVGJQ4"},"agent_actions":{"view_html":"https://pith.science/pith/DSOVGJQ4LSILBKWNIBRVCMIYGY","download_json":"https://pith.science/pith/DSOVGJQ4LSILBKWNIBRVCMIYGY.json","view_paper":"https://pith.science/paper/DSOVGJQ4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1905.12357&json=true","fetch_graph":"https://pith.science/api/pith-number/DSOVGJQ4LSILBKWNIBRVCMIYGY/graph.json","fetch_events":"https://pith.science/api/pith-number/DSOVGJQ4LSILBKWNIBRVCMIYGY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DSOVGJQ4LSILBKWNIBRVCMIYGY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DSOVGJQ4LSILBKWNIBRVCMIYGY/action/storage_attestation","attest_author":"https://pith.science/pith/DSOVGJQ4LSILBKWNIBRVCMIYGY/action/author_attestation","sign_citation":"https://pith.science/pith/DSOVGJQ4LSILBKWNIBRVCMIYGY/action/citation_signature","submit_replication":"https://pith.science/pith/DSOVGJQ4LSILBKWNIBRVCMIYGY/action/replication_record"}},"created_at":"2026-05-17T23:40:43.233661+00:00","updated_at":"2026-05-17T23:40:43.233661+00:00"}