{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2008:LOVXMVESHPQDNNQCCA2INLSZ7T","short_pith_number":"pith:LOVXMVES","schema_version":"1.0","canonical_sha256":"5bab7654923be036b602103486ae59fcd15e034df8d2f95c66b403d38e03a6a7","source":{"kind":"arxiv","id":"0812.3823","version":1},"attestation_state":"computed","paper":{"title":"The solar wind charge-transfer X-ray emission in the 1/4 keV energy range: inferences on Local Bubble hot gas at low Z","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"D. Koutroumpa, J. C. Raymond, R. Lallement, V. Kharchenko","submitted_at":"2008-12-19T16:02:40Z","abstract_excerpt":"We present calculations of the heliospheric SWCX emission spectra and their contributions in the ROSAT 1/4 keV band. We compare our results with the soft X-ray diffuse background (SXRB) emission detected in front of 378 identified shadowing regions during the ROSAT All-Sky Survey (Snowden et al. 2000). This foreground component is principally attributed to the hot gas of the so-called Local Bubble (LB), an irregularly shaped cavity of ~50-150 pc around the Sun, which is supposed to contain ~10^6 K plasma. Our results suggest that the SWCX emission from the heliosphere is bright enough to accou"},"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":"0812.3823","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph","submitted_at":"2008-12-19T16:02:40Z","cross_cats_sorted":[],"title_canon_sha256":"8566f70a85da7015aec7341342547f024eda7350c5751dfc005cd956da055c19","abstract_canon_sha256":"72c34fb19cad726de11f53e7eb682b09184f5cb5edfac9e8d0c854c9e1e4cf0e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:29:24.344501Z","signature_b64":"IvkjwaYlCMg1ob8dWjk8Nn8ujbdFHJvhpeL59YS+bPYAETc1nIimi7yjXbY8ywmQXiFOjRVUHZbTL0ASaQqmAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5bab7654923be036b602103486ae59fcd15e034df8d2f95c66b403d38e03a6a7","last_reissued_at":"2026-05-18T04:29:24.344019Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:29:24.344019Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The solar wind charge-transfer X-ray emission in the 1/4 keV energy range: inferences on Local Bubble hot gas at low Z","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"D. Koutroumpa, J. C. Raymond, R. Lallement, V. Kharchenko","submitted_at":"2008-12-19T16:02:40Z","abstract_excerpt":"We present calculations of the heliospheric SWCX emission spectra and their contributions in the ROSAT 1/4 keV band. We compare our results with the soft X-ray diffuse background (SXRB) emission detected in front of 378 identified shadowing regions during the ROSAT All-Sky Survey (Snowden et al. 2000). This foreground component is principally attributed to the hot gas of the so-called Local Bubble (LB), an irregularly shaped cavity of ~50-150 pc around the Sun, which is supposed to contain ~10^6 K plasma. Our results suggest that the SWCX emission from the heliosphere is bright enough to accou"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0812.3823","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":"0812.3823","created_at":"2026-05-18T04:29:24.344095+00:00"},{"alias_kind":"arxiv_version","alias_value":"0812.3823v1","created_at":"2026-05-18T04:29:24.344095+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0812.3823","created_at":"2026-05-18T04:29:24.344095+00:00"},{"alias_kind":"pith_short_12","alias_value":"LOVXMVESHPQD","created_at":"2026-05-18T12:25:57.157939+00:00"},{"alias_kind":"pith_short_16","alias_value":"LOVXMVESHPQDNNQC","created_at":"2026-05-18T12:25:57.157939+00:00"},{"alias_kind":"pith_short_8","alias_value":"LOVXMVES","created_at":"2026-05-18T12:25:57.157939+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/LOVXMVESHPQDNNQCCA2INLSZ7T","json":"https://pith.science/pith/LOVXMVESHPQDNNQCCA2INLSZ7T.json","graph_json":"https://pith.science/api/pith-number/LOVXMVESHPQDNNQCCA2INLSZ7T/graph.json","events_json":"https://pith.science/api/pith-number/LOVXMVESHPQDNNQCCA2INLSZ7T/events.json","paper":"https://pith.science/paper/LOVXMVES"},"agent_actions":{"view_html":"https://pith.science/pith/LOVXMVESHPQDNNQCCA2INLSZ7T","download_json":"https://pith.science/pith/LOVXMVESHPQDNNQCCA2INLSZ7T.json","view_paper":"https://pith.science/paper/LOVXMVES","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0812.3823&json=true","fetch_graph":"https://pith.science/api/pith-number/LOVXMVESHPQDNNQCCA2INLSZ7T/graph.json","fetch_events":"https://pith.science/api/pith-number/LOVXMVESHPQDNNQCCA2INLSZ7T/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LOVXMVESHPQDNNQCCA2INLSZ7T/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LOVXMVESHPQDNNQCCA2INLSZ7T/action/storage_attestation","attest_author":"https://pith.science/pith/LOVXMVESHPQDNNQCCA2INLSZ7T/action/author_attestation","sign_citation":"https://pith.science/pith/LOVXMVESHPQDNNQCCA2INLSZ7T/action/citation_signature","submit_replication":"https://pith.science/pith/LOVXMVESHPQDNNQCCA2INLSZ7T/action/replication_record"}},"created_at":"2026-05-18T04:29:24.344095+00:00","updated_at":"2026-05-18T04:29:24.344095+00:00"}