{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:6FUF3WLN3ITVCUGV7AA3U7QZ6I","short_pith_number":"pith:6FUF3WLN","schema_version":"1.0","canonical_sha256":"f1685dd96dda275150d5f801ba7e19f2358e2cee66a6a93eba579334619f5828","source":{"kind":"arxiv","id":"1210.4789","version":1},"attestation_state":"computed","paper":{"title":"Investigating the Optical Counterpart Candidates of Four INTEGRAL Sources localized with Chandra","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Arash Bodaghee, Emrah Kalemci, Farid Rahoui, Jerome Rodriguez, John A. Tomsick, Jules Halpern, Mehtap \\\"Ozbey Arabac{\\i}, Sylvain Chaty","submitted_at":"2012-10-17T16:35:11Z","abstract_excerpt":"We report on the optical spectroscopic follow up observations of the candidate counterparts to four INTEGRAL sources: IGR J04069+5042, IGR J06552-1146, IGR J21188+4901 and IGR J22014+6034. The candidate counterparts were determined with Chandra, and the optical observations were performed with 1.5-m RTT-150 telescope (T\\\"{U}B\\.{I}TAK National Observatory, Antalya, Turkey) and 2.4-m Hiltner Telescope (MDM Observatory, Kitt Peak, Arizona). Our spectroscopic results show that one of the two candidates of IGR J04069+5042 and the one observed for IGR J06552-1146 could be active late-type stars in R"},"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":"1210.4789","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2012-10-17T16:35:11Z","cross_cats_sorted":[],"title_canon_sha256":"4c0f8b29948f686a3ec447a09749fd1d65926f492749de779cd3f3b759b86e96","abstract_canon_sha256":"27d3faff7c002e44c1e45e6469f6df1581a02e951e60c7c93a05abf13618ec52"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:09:26.255098Z","signature_b64":"psaAV0T3gXI5wKX5oL64VRhrlOXC+hPJJf9sgu2tyReM97BcYVZHoX8/7LnhoJGnACT7oS7aVYVJEW1TzhnDCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f1685dd96dda275150d5f801ba7e19f2358e2cee66a6a93eba579334619f5828","last_reissued_at":"2026-05-18T01:09:26.254667Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:09:26.254667Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Investigating the Optical Counterpart Candidates of Four INTEGRAL Sources localized with Chandra","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Arash Bodaghee, Emrah Kalemci, Farid Rahoui, Jerome Rodriguez, John A. Tomsick, Jules Halpern, Mehtap \\\"Ozbey Arabac{\\i}, Sylvain Chaty","submitted_at":"2012-10-17T16:35:11Z","abstract_excerpt":"We report on the optical spectroscopic follow up observations of the candidate counterparts to four INTEGRAL sources: IGR J04069+5042, IGR J06552-1146, IGR J21188+4901 and IGR J22014+6034. The candidate counterparts were determined with Chandra, and the optical observations were performed with 1.5-m RTT-150 telescope (T\\\"{U}B\\.{I}TAK National Observatory, Antalya, Turkey) and 2.4-m Hiltner Telescope (MDM Observatory, Kitt Peak, Arizona). Our spectroscopic results show that one of the two candidates of IGR J04069+5042 and the one observed for IGR J06552-1146 could be active late-type stars in R"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1210.4789","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":"1210.4789","created_at":"2026-05-18T01:09:26.254730+00:00"},{"alias_kind":"arxiv_version","alias_value":"1210.4789v1","created_at":"2026-05-18T01:09:26.254730+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1210.4789","created_at":"2026-05-18T01:09:26.254730+00:00"},{"alias_kind":"pith_short_12","alias_value":"6FUF3WLN3ITV","created_at":"2026-05-18T12:26:56.085431+00:00"},{"alias_kind":"pith_short_16","alias_value":"6FUF3WLN3ITVCUGV","created_at":"2026-05-18T12:26:56.085431+00:00"},{"alias_kind":"pith_short_8","alias_value":"6FUF3WLN","created_at":"2026-05-18T12:26:56.085431+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/6FUF3WLN3ITVCUGV7AA3U7QZ6I","json":"https://pith.science/pith/6FUF3WLN3ITVCUGV7AA3U7QZ6I.json","graph_json":"https://pith.science/api/pith-number/6FUF3WLN3ITVCUGV7AA3U7QZ6I/graph.json","events_json":"https://pith.science/api/pith-number/6FUF3WLN3ITVCUGV7AA3U7QZ6I/events.json","paper":"https://pith.science/paper/6FUF3WLN"},"agent_actions":{"view_html":"https://pith.science/pith/6FUF3WLN3ITVCUGV7AA3U7QZ6I","download_json":"https://pith.science/pith/6FUF3WLN3ITVCUGV7AA3U7QZ6I.json","view_paper":"https://pith.science/paper/6FUF3WLN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1210.4789&json=true","fetch_graph":"https://pith.science/api/pith-number/6FUF3WLN3ITVCUGV7AA3U7QZ6I/graph.json","fetch_events":"https://pith.science/api/pith-number/6FUF3WLN3ITVCUGV7AA3U7QZ6I/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6FUF3WLN3ITVCUGV7AA3U7QZ6I/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6FUF3WLN3ITVCUGV7AA3U7QZ6I/action/storage_attestation","attest_author":"https://pith.science/pith/6FUF3WLN3ITVCUGV7AA3U7QZ6I/action/author_attestation","sign_citation":"https://pith.science/pith/6FUF3WLN3ITVCUGV7AA3U7QZ6I/action/citation_signature","submit_replication":"https://pith.science/pith/6FUF3WLN3ITVCUGV7AA3U7QZ6I/action/replication_record"}},"created_at":"2026-05-18T01:09:26.254730+00:00","updated_at":"2026-05-18T01:09:26.254730+00:00"}