{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:IQI4O44A263XKVMMBDDXMKVCXD","short_pith_number":"pith:IQI4O44A","schema_version":"1.0","canonical_sha256":"4411c77380d7b775558c08c7762aa2b8e7670c0893e4ea5281b0e0b782199ae7","source":{"kind":"arxiv","id":"1306.4471","version":1},"attestation_state":"computed","paper":{"title":"Assessment of detectability of neutral interstellar deuterium by IBEX observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"D.F. Rodr\\'iguez, D.J. McComas, E. M\\\"obius, J.M. Sok\\'o\\l, M.A. Kubiak, M. Bzowski, P. Wurz","submitted_at":"2013-06-19T09:59:06Z","abstract_excerpt":"The abundance of deuterium in the interstellar gas in front of the Sun gives insight into the processes of filtration of neutral interstellar species through the heliospheric interface and potentially into the chemical evolution of the Galactic gas. We investigate the possibility of detection of neutral interstellar deuterium at 1 AU from the Sun by direct sampling by the Interstellar Boundary Explorer (IBEX). We simulate the flux of neutral interstellar D at IBEX for the actual measurement conditions. We assess the number of interstellar D atom counts expected during the first three years of "},"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":"1306.4471","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2013-06-19T09:59:06Z","cross_cats_sorted":[],"title_canon_sha256":"6565566c7dbf035fad889b503f0d8c6849940ddb773242fb55d755bf0e784ca7","abstract_canon_sha256":"bb15936e60355e8097fa80b4c64b1bf74a5a7d0809cf4649504cfdd2b40148c3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:49:14.965699Z","signature_b64":"SYmfTiiq4lUYVFlzHOl8rJpG8SzVSgXlBpRiOeJA2rElU5ur/sPps8H7ZydKFbbKM14WJWi8554KphpG/z5zDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4411c77380d7b775558c08c7762aa2b8e7670c0893e4ea5281b0e0b782199ae7","last_reissued_at":"2026-05-18T01:49:14.965060Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:49:14.965060Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Assessment of detectability of neutral interstellar deuterium by IBEX observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"D.F. Rodr\\'iguez, D.J. McComas, E. M\\\"obius, J.M. Sok\\'o\\l, M.A. Kubiak, M. Bzowski, P. Wurz","submitted_at":"2013-06-19T09:59:06Z","abstract_excerpt":"The abundance of deuterium in the interstellar gas in front of the Sun gives insight into the processes of filtration of neutral interstellar species through the heliospheric interface and potentially into the chemical evolution of the Galactic gas. We investigate the possibility of detection of neutral interstellar deuterium at 1 AU from the Sun by direct sampling by the Interstellar Boundary Explorer (IBEX). We simulate the flux of neutral interstellar D at IBEX for the actual measurement conditions. We assess the number of interstellar D atom counts expected during the first three years of "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1306.4471","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":"1306.4471","created_at":"2026-05-18T01:49:14.965161+00:00"},{"alias_kind":"arxiv_version","alias_value":"1306.4471v1","created_at":"2026-05-18T01:49:14.965161+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1306.4471","created_at":"2026-05-18T01:49:14.965161+00:00"},{"alias_kind":"pith_short_12","alias_value":"IQI4O44A263X","created_at":"2026-05-18T12:27:46.883200+00:00"},{"alias_kind":"pith_short_16","alias_value":"IQI4O44A263XKVMM","created_at":"2026-05-18T12:27:46.883200+00:00"},{"alias_kind":"pith_short_8","alias_value":"IQI4O44A","created_at":"2026-05-18T12:27:46.883200+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/IQI4O44A263XKVMMBDDXMKVCXD","json":"https://pith.science/pith/IQI4O44A263XKVMMBDDXMKVCXD.json","graph_json":"https://pith.science/api/pith-number/IQI4O44A263XKVMMBDDXMKVCXD/graph.json","events_json":"https://pith.science/api/pith-number/IQI4O44A263XKVMMBDDXMKVCXD/events.json","paper":"https://pith.science/paper/IQI4O44A"},"agent_actions":{"view_html":"https://pith.science/pith/IQI4O44A263XKVMMBDDXMKVCXD","download_json":"https://pith.science/pith/IQI4O44A263XKVMMBDDXMKVCXD.json","view_paper":"https://pith.science/paper/IQI4O44A","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1306.4471&json=true","fetch_graph":"https://pith.science/api/pith-number/IQI4O44A263XKVMMBDDXMKVCXD/graph.json","fetch_events":"https://pith.science/api/pith-number/IQI4O44A263XKVMMBDDXMKVCXD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IQI4O44A263XKVMMBDDXMKVCXD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IQI4O44A263XKVMMBDDXMKVCXD/action/storage_attestation","attest_author":"https://pith.science/pith/IQI4O44A263XKVMMBDDXMKVCXD/action/author_attestation","sign_citation":"https://pith.science/pith/IQI4O44A263XKVMMBDDXMKVCXD/action/citation_signature","submit_replication":"https://pith.science/pith/IQI4O44A263XKVMMBDDXMKVCXD/action/replication_record"}},"created_at":"2026-05-18T01:49:14.965161+00:00","updated_at":"2026-05-18T01:49:14.965161+00:00"}