{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:TS2IVJOA2GQA6KJ63XZH245KQ2","short_pith_number":"pith:TS2IVJOA","schema_version":"1.0","canonical_sha256":"9cb48aa5c0d1a00f293eddf27d73aa869fcca83efc793aa2464db5ed9a94c5df","source":{"kind":"arxiv","id":"2209.15127","version":1},"attestation_state":"computed","paper":{"title":"Absorption lines from magnetically driven winds in X-ray binaries II: high resolution observational signatures expected from future X-ray observatories","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Gilles Henri, Gregoire Marcel, Jerome Rodriguez, Joern Wilms, Jonatan Jacquemin-Ide, Jonathan Ferreira, Julien Malzac, Maica Clavel, Maxime Parra, Mickael Coriat, Pierre-Olivier Petrucci, Renaud Belmont, Stephane Corbel, Sudeb Ranjan Datta, Susmita Chakravorty","submitted_at":"2022-09-29T22:41:47Z","abstract_excerpt":"In our self-similar, analytical, magneto-hydrodynamic (MHD) accretion-ejection solution, the density at the base of the outflow is explicitly dependent on the disk accretion rate - a unique property of this class of solutions. We had earlier found that the ejection index $p >\\sim 0.1 (\\dot{M}_{acc} \\propto r^p ) $ is a key MHD parameter that decides if the flow can cause absorption lines in the high resolution X-ray spectra of black hole binaries. Here we choose 3 dense warm solutions with $p = 0.1, 0.3, 0.45$ and carefully develop a methodology to generate spectra which are convolved with the"},"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":"2209.15127","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2022-09-29T22:41:47Z","cross_cats_sorted":[],"title_canon_sha256":"e7801ba5d086eeea096b4ed9e1c8d02e0946d3c070978f5019529dd6b10447ac","abstract_canon_sha256":"32b50425877bffe0758c895109e047d00263bc141aa6695623f858b665704ab8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:14:23.991144Z","signature_b64":"PVNW+7lENosH6CyPo2TtKERm5xGcZTRN6ZKH/g6g0wXbHDGL0LSaUji9ejQnzz4TsYrwVzGisoYIOoY3ecrCCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9cb48aa5c0d1a00f293eddf27d73aa869fcca83efc793aa2464db5ed9a94c5df","last_reissued_at":"2026-07-05T05:14:23.990611Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:14:23.990611Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Absorption lines from magnetically driven winds in X-ray binaries II: high resolution observational signatures expected from future X-ray observatories","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Gilles Henri, Gregoire Marcel, Jerome Rodriguez, Joern Wilms, Jonatan Jacquemin-Ide, Jonathan Ferreira, Julien Malzac, Maica Clavel, Maxime Parra, Mickael Coriat, Pierre-Olivier Petrucci, Renaud Belmont, Stephane Corbel, Sudeb Ranjan Datta, Susmita Chakravorty","submitted_at":"2022-09-29T22:41:47Z","abstract_excerpt":"In our self-similar, analytical, magneto-hydrodynamic (MHD) accretion-ejection solution, the density at the base of the outflow is explicitly dependent on the disk accretion rate - a unique property of this class of solutions. We had earlier found that the ejection index $p >\\sim 0.1 (\\dot{M}_{acc} \\propto r^p ) $ is a key MHD parameter that decides if the flow can cause absorption lines in the high resolution X-ray spectra of black hole binaries. Here we choose 3 dense warm solutions with $p = 0.1, 0.3, 0.45$ and carefully develop a methodology to generate spectra which are convolved with the"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2209.15127","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2209.15127/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":"2209.15127","created_at":"2026-07-05T05:14:23.990666+00:00"},{"alias_kind":"arxiv_version","alias_value":"2209.15127v1","created_at":"2026-07-05T05:14:23.990666+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2209.15127","created_at":"2026-07-05T05:14:23.990666+00:00"},{"alias_kind":"pith_short_12","alias_value":"TS2IVJOA2GQA","created_at":"2026-07-05T05:14:23.990666+00:00"},{"alias_kind":"pith_short_16","alias_value":"TS2IVJOA2GQA6KJ6","created_at":"2026-07-05T05:14:23.990666+00:00"},{"alias_kind":"pith_short_8","alias_value":"TS2IVJOA","created_at":"2026-07-05T05:14:23.990666+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/TS2IVJOA2GQA6KJ63XZH245KQ2","json":"https://pith.science/pith/TS2IVJOA2GQA6KJ63XZH245KQ2.json","graph_json":"https://pith.science/api/pith-number/TS2IVJOA2GQA6KJ63XZH245KQ2/graph.json","events_json":"https://pith.science/api/pith-number/TS2IVJOA2GQA6KJ63XZH245KQ2/events.json","paper":"https://pith.science/paper/TS2IVJOA"},"agent_actions":{"view_html":"https://pith.science/pith/TS2IVJOA2GQA6KJ63XZH245KQ2","download_json":"https://pith.science/pith/TS2IVJOA2GQA6KJ63XZH245KQ2.json","view_paper":"https://pith.science/paper/TS2IVJOA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2209.15127&json=true","fetch_graph":"https://pith.science/api/pith-number/TS2IVJOA2GQA6KJ63XZH245KQ2/graph.json","fetch_events":"https://pith.science/api/pith-number/TS2IVJOA2GQA6KJ63XZH245KQ2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TS2IVJOA2GQA6KJ63XZH245KQ2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TS2IVJOA2GQA6KJ63XZH245KQ2/action/storage_attestation","attest_author":"https://pith.science/pith/TS2IVJOA2GQA6KJ63XZH245KQ2/action/author_attestation","sign_citation":"https://pith.science/pith/TS2IVJOA2GQA6KJ63XZH245KQ2/action/citation_signature","submit_replication":"https://pith.science/pith/TS2IVJOA2GQA6KJ63XZH245KQ2/action/replication_record"}},"created_at":"2026-07-05T05:14:23.990666+00:00","updated_at":"2026-07-05T05:14:23.990666+00:00"}