{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:3JMOJBJF64IONIAXVWQSJO4EQK","short_pith_number":"pith:3JMOJBJF","schema_version":"1.0","canonical_sha256":"da58e48525f710e6a017ada124bb8482a058d92f393a53eaba2274fda8460c72","source":{"kind":"arxiv","id":"2009.02076","version":2},"attestation_state":"computed","paper":{"title":"Pulsars with NenuFAR: backend and pipelines","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph","physics.ins-det"],"primary_cat":"astro-ph.IM","authors_text":"A.Bilous, A. Loh, A. Possenti, B. Cecconi, C.Briand, C.Tasse, C. Tiburzi, C. Viou, G. Shaifullah, G. Theureau, I. Cognard, J.-M. Grie{\\ss}meier, J. N. Girard, J. P. W. Verbiest, J. W. McKee, L. Bondonneau, L. Guillemot, L. Martin, M. Brionne, M. Pilia, M. Serylak, O. Wucknitz, P. Zarka, R. Dallier, R. Main, S. Chen, S. Corbel, S. Yerin, V. Kondratiev, Z. Wu","submitted_at":"2020-09-04T09:02:51Z","abstract_excerpt":"NenuFAR (New extension in Nan\\c{c}ay upgrading LoFAR) is a new radio telescope developed and built on the site of the Nan\\c{c}ay Radio Observatory. It is designed to observe the largely unexplored frequency window from 10 to 85\\,MHz, offering a high sensitivity across its full bandwidth. NenuFAR has started its \"early science\" operation in July 2019, with 58\\% of its final collecting area being available. Pulsars are one of the major topics for the scientific exploitation of this frequency range and represent an important challenge in terms of instrumentation. Designing instrumentation at thes"},"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":"2009.02076","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2020-09-04T09:02:51Z","cross_cats_sorted":["hep-ph","physics.ins-det"],"title_canon_sha256":"5e10e81a9c4d2c132031bed67c4be0b5c06d43e3e84a2724f91df7617b25224d","abstract_canon_sha256":"022ac334872c545067dde249d26d5366227deb0c8b696faab78644879cb377f2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:04:40.579169Z","signature_b64":"nZREQFknGYZL4Aeq2lN5FpQqC2LeH5cF253uti+Dsw2bg3wmm+rcMUgD9PNGINJsJClR6J/gBhd5dBkxFU/mBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"da58e48525f710e6a017ada124bb8482a058d92f393a53eaba2274fda8460c72","last_reissued_at":"2026-07-05T03:04:40.578780Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:04:40.578780Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Pulsars with NenuFAR: backend and pipelines","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph","physics.ins-det"],"primary_cat":"astro-ph.IM","authors_text":"A.Bilous, A. Loh, A. Possenti, B. Cecconi, C.Briand, C.Tasse, C. Tiburzi, C. Viou, G. Shaifullah, G. Theureau, I. Cognard, J.-M. Grie{\\ss}meier, J. N. Girard, J. P. W. Verbiest, J. W. McKee, L. Bondonneau, L. Guillemot, L. Martin, M. Brionne, M. Pilia, M. Serylak, O. Wucknitz, P. Zarka, R. Dallier, R. Main, S. Chen, S. Corbel, S. Yerin, V. Kondratiev, Z. Wu","submitted_at":"2020-09-04T09:02:51Z","abstract_excerpt":"NenuFAR (New extension in Nan\\c{c}ay upgrading LoFAR) is a new radio telescope developed and built on the site of the Nan\\c{c}ay Radio Observatory. It is designed to observe the largely unexplored frequency window from 10 to 85\\,MHz, offering a high sensitivity across its full bandwidth. NenuFAR has started its \"early science\" operation in July 2019, with 58\\% of its final collecting area being available. Pulsars are one of the major topics for the scientific exploitation of this frequency range and represent an important challenge in terms of instrumentation. Designing instrumentation at thes"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2009.02076","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2009.02076/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2009.02076","created_at":"2026-07-05T03:04:40.578841+00:00"},{"alias_kind":"arxiv_version","alias_value":"2009.02076v2","created_at":"2026-07-05T03:04:40.578841+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2009.02076","created_at":"2026-07-05T03:04:40.578841+00:00"},{"alias_kind":"pith_short_12","alias_value":"3JMOJBJF64IO","created_at":"2026-07-05T03:04:40.578841+00:00"},{"alias_kind":"pith_short_16","alias_value":"3JMOJBJF64IONIAX","created_at":"2026-07-05T03:04:40.578841+00:00"},{"alias_kind":"pith_short_8","alias_value":"3JMOJBJF","created_at":"2026-07-05T03:04:40.578841+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.06096","citing_title":"Exploring the Galactic plasma with pulsars in the SKA Era","ref_index":58,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/3JMOJBJF64IONIAXVWQSJO4EQK","json":"https://pith.science/pith/3JMOJBJF64IONIAXVWQSJO4EQK.json","graph_json":"https://pith.science/api/pith-number/3JMOJBJF64IONIAXVWQSJO4EQK/graph.json","events_json":"https://pith.science/api/pith-number/3JMOJBJF64IONIAXVWQSJO4EQK/events.json","paper":"https://pith.science/paper/3JMOJBJF"},"agent_actions":{"view_html":"https://pith.science/pith/3JMOJBJF64IONIAXVWQSJO4EQK","download_json":"https://pith.science/pith/3JMOJBJF64IONIAXVWQSJO4EQK.json","view_paper":"https://pith.science/paper/3JMOJBJF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2009.02076&json=true","fetch_graph":"https://pith.science/api/pith-number/3JMOJBJF64IONIAXVWQSJO4EQK/graph.json","fetch_events":"https://pith.science/api/pith-number/3JMOJBJF64IONIAXVWQSJO4EQK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3JMOJBJF64IONIAXVWQSJO4EQK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3JMOJBJF64IONIAXVWQSJO4EQK/action/storage_attestation","attest_author":"https://pith.science/pith/3JMOJBJF64IONIAXVWQSJO4EQK/action/author_attestation","sign_citation":"https://pith.science/pith/3JMOJBJF64IONIAXVWQSJO4EQK/action/citation_signature","submit_replication":"https://pith.science/pith/3JMOJBJF64IONIAXVWQSJO4EQK/action/replication_record"}},"created_at":"2026-07-05T03:04:40.578841+00:00","updated_at":"2026-07-05T03:04:40.578841+00:00"}