{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:6DDUQJIQTPOL3RDOZZHZY2W4HL","short_pith_number":"pith:6DDUQJIQ","schema_version":"1.0","canonical_sha256":"f0c74825109bdcbdc46ece4f9c6adc3ad8b28abf14db8e8c7148961569907a5a","source":{"kind":"arxiv","id":"1802.00637","version":2},"attestation_state":"computed","paper":{"title":"Effects of Interstellar Dust Scattering on the X-ray Eclipses of the LMXB AX J1745.6-2901 in the Galactic Center","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Chichuan Jin, Frank Haberl, Gabriele Ponti, Lynne Valencic, Randall Smith","submitted_at":"2018-02-02T11:07:44Z","abstract_excerpt":"AX J1745.6-2901 is an eclipsing low mass X-ray binary (LMXB) in the Galactic Centre (GC). It shows significant X-ray excess emission during the eclipse phase, and its eclipse light curve shows an asymmetric shape. We use archival XMM-Newton and Chandra observations to study the origin of these peculiar X-ray eclipsing phenomena. We find that the shape of the observed X-ray eclipse light curves depends on both photon energy and the shape of the source extraction region, and also shows differences between the two instruments. By performing detailed simulations for the time-dependent X-ray dust s"},"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":"1802.00637","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2018-02-02T11:07:44Z","cross_cats_sorted":[],"title_canon_sha256":"7061d73aaa0152f3bcc9b5c62ac1e8d73df8c27c78ce2d55160e6b8709fdf01b","abstract_canon_sha256":"5b621ae060d462b028895f55ab118f244dd8ddcedce6c3febca5ac3dfa077cb5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:17:38.858446Z","signature_b64":"AIDMpf6FJLqZgJIcwAuXMo/M02QGspKqtS1GccpSroB1Cp4dOTrnitWqYdh4zYy7zb/Rr/DmyzaEW6bWEziVBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f0c74825109bdcbdc46ece4f9c6adc3ad8b28abf14db8e8c7148961569907a5a","last_reissued_at":"2026-05-18T00:17:38.857932Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:17:38.857932Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Effects of Interstellar Dust Scattering on the X-ray Eclipses of the LMXB AX J1745.6-2901 in the Galactic Center","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Chichuan Jin, Frank Haberl, Gabriele Ponti, Lynne Valencic, Randall Smith","submitted_at":"2018-02-02T11:07:44Z","abstract_excerpt":"AX J1745.6-2901 is an eclipsing low mass X-ray binary (LMXB) in the Galactic Centre (GC). It shows significant X-ray excess emission during the eclipse phase, and its eclipse light curve shows an asymmetric shape. We use archival XMM-Newton and Chandra observations to study the origin of these peculiar X-ray eclipsing phenomena. We find that the shape of the observed X-ray eclipse light curves depends on both photon energy and the shape of the source extraction region, and also shows differences between the two instruments. By performing detailed simulations for the time-dependent X-ray dust s"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1802.00637","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":""},"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":"1802.00637","created_at":"2026-05-18T00:17:38.858033+00:00"},{"alias_kind":"arxiv_version","alias_value":"1802.00637v2","created_at":"2026-05-18T00:17:38.858033+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1802.00637","created_at":"2026-05-18T00:17:38.858033+00:00"},{"alias_kind":"pith_short_12","alias_value":"6DDUQJIQTPOL","created_at":"2026-05-18T12:32:08.215937+00:00"},{"alias_kind":"pith_short_16","alias_value":"6DDUQJIQTPOL3RDO","created_at":"2026-05-18T12:32:08.215937+00:00"},{"alias_kind":"pith_short_8","alias_value":"6DDUQJIQ","created_at":"2026-05-18T12:32:08.215937+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/6DDUQJIQTPOL3RDOZZHZY2W4HL","json":"https://pith.science/pith/6DDUQJIQTPOL3RDOZZHZY2W4HL.json","graph_json":"https://pith.science/api/pith-number/6DDUQJIQTPOL3RDOZZHZY2W4HL/graph.json","events_json":"https://pith.science/api/pith-number/6DDUQJIQTPOL3RDOZZHZY2W4HL/events.json","paper":"https://pith.science/paper/6DDUQJIQ"},"agent_actions":{"view_html":"https://pith.science/pith/6DDUQJIQTPOL3RDOZZHZY2W4HL","download_json":"https://pith.science/pith/6DDUQJIQTPOL3RDOZZHZY2W4HL.json","view_paper":"https://pith.science/paper/6DDUQJIQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1802.00637&json=true","fetch_graph":"https://pith.science/api/pith-number/6DDUQJIQTPOL3RDOZZHZY2W4HL/graph.json","fetch_events":"https://pith.science/api/pith-number/6DDUQJIQTPOL3RDOZZHZY2W4HL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6DDUQJIQTPOL3RDOZZHZY2W4HL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6DDUQJIQTPOL3RDOZZHZY2W4HL/action/storage_attestation","attest_author":"https://pith.science/pith/6DDUQJIQTPOL3RDOZZHZY2W4HL/action/author_attestation","sign_citation":"https://pith.science/pith/6DDUQJIQTPOL3RDOZZHZY2W4HL/action/citation_signature","submit_replication":"https://pith.science/pith/6DDUQJIQTPOL3RDOZZHZY2W4HL/action/replication_record"}},"created_at":"2026-05-18T00:17:38.858033+00:00","updated_at":"2026-05-18T00:17:38.858033+00:00"}