{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:SKQV7GVPEO6ADPWBW3CNQC3HQZ","short_pith_number":"pith:SKQV7GVP","schema_version":"1.0","canonical_sha256":"92a15f9aaf23bc01bec1b6c4d80b678662367ad4c2c7aa6a6773b387eb53bf46","source":{"kind":"arxiv","id":"1109.5866","version":1},"attestation_state":"computed","paper":{"title":"Obscuring Supersoft X-ray Sources in Stellar Winds","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Carsten Dominik, Gijs Nelemans, Mikkel Thomas B{\\o}je Nielsen","submitted_at":"2011-09-27T12:56:08Z","abstract_excerpt":"We investigate the possibility of obscuring supersoft X-ray sources in the winds of companion stars. We derive limits on the amount of circumstellar material needed to fully obscure a 'canonical' supersoft X-ray source in the Large Magellanic Cloud, as observed with the Chandra X-ray Observatory."},"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":"1109.5866","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2011-09-27T12:56:08Z","cross_cats_sorted":[],"title_canon_sha256":"53950a1d2d7a38847d5941e02a3dd27edc34fb4d94668e5d6c633e4e6426cf1a","abstract_canon_sha256":"3b42cb7c4c8d02b5c5337f9b0a1403442c6ae70182275c86cc02ff8d77608cf4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:12:11.089265Z","signature_b64":"Xa2R9PgX2UNmjRjC8fJq5ZGYUrLuth0k4VeDJrxtmoUUUydSbN1NAHwVUmp64Gz9wV11qBO3T613n1fABY7LAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"92a15f9aaf23bc01bec1b6c4d80b678662367ad4c2c7aa6a6773b387eb53bf46","last_reissued_at":"2026-05-18T04:12:11.088733Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:12:11.088733Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Obscuring Supersoft X-ray Sources in Stellar Winds","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Carsten Dominik, Gijs Nelemans, Mikkel Thomas B{\\o}je Nielsen","submitted_at":"2011-09-27T12:56:08Z","abstract_excerpt":"We investigate the possibility of obscuring supersoft X-ray sources in the winds of companion stars. We derive limits on the amount of circumstellar material needed to fully obscure a 'canonical' supersoft X-ray source in the Large Magellanic Cloud, as observed with the Chandra X-ray Observatory."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1109.5866","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":"1109.5866","created_at":"2026-05-18T04:12:11.088814+00:00"},{"alias_kind":"arxiv_version","alias_value":"1109.5866v1","created_at":"2026-05-18T04:12:11.088814+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1109.5866","created_at":"2026-05-18T04:12:11.088814+00:00"},{"alias_kind":"pith_short_12","alias_value":"SKQV7GVPEO6A","created_at":"2026-05-18T12:26:41.206345+00:00"},{"alias_kind":"pith_short_16","alias_value":"SKQV7GVPEO6ADPWB","created_at":"2026-05-18T12:26:41.206345+00:00"},{"alias_kind":"pith_short_8","alias_value":"SKQV7GVP","created_at":"2026-05-18T12:26:41.206345+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/SKQV7GVPEO6ADPWBW3CNQC3HQZ","json":"https://pith.science/pith/SKQV7GVPEO6ADPWBW3CNQC3HQZ.json","graph_json":"https://pith.science/api/pith-number/SKQV7GVPEO6ADPWBW3CNQC3HQZ/graph.json","events_json":"https://pith.science/api/pith-number/SKQV7GVPEO6ADPWBW3CNQC3HQZ/events.json","paper":"https://pith.science/paper/SKQV7GVP"},"agent_actions":{"view_html":"https://pith.science/pith/SKQV7GVPEO6ADPWBW3CNQC3HQZ","download_json":"https://pith.science/pith/SKQV7GVPEO6ADPWBW3CNQC3HQZ.json","view_paper":"https://pith.science/paper/SKQV7GVP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1109.5866&json=true","fetch_graph":"https://pith.science/api/pith-number/SKQV7GVPEO6ADPWBW3CNQC3HQZ/graph.json","fetch_events":"https://pith.science/api/pith-number/SKQV7GVPEO6ADPWBW3CNQC3HQZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SKQV7GVPEO6ADPWBW3CNQC3HQZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SKQV7GVPEO6ADPWBW3CNQC3HQZ/action/storage_attestation","attest_author":"https://pith.science/pith/SKQV7GVPEO6ADPWBW3CNQC3HQZ/action/author_attestation","sign_citation":"https://pith.science/pith/SKQV7GVPEO6ADPWBW3CNQC3HQZ/action/citation_signature","submit_replication":"https://pith.science/pith/SKQV7GVPEO6ADPWBW3CNQC3HQZ/action/replication_record"}},"created_at":"2026-05-18T04:12:11.088814+00:00","updated_at":"2026-05-18T04:12:11.088814+00:00"}