{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2017:WCFH6U6B43AVD3P57TNUBX2JIU","short_pith_number":"pith:WCFH6U6B","canonical_record":{"source":{"id":"1706.05002","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-06-15T14:52:44Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"9e05fa55df47e8935b02ca44e0afda8b560884259ac2ed1ee96897b94a490d14","abstract_canon_sha256":"8423872319a5716cd85905cd821b6ca7b39a73c4b56d22ff0852d15bfd197df6"},"schema_version":"1.0"},"canonical_sha256":"b08a7f53c1e6c151edfdfcdb40df49452ccde735b7ae7b27a99775adeb030fc8","source":{"kind":"arxiv","id":"1706.05002","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1706.05002","created_at":"2026-05-18T00:22:59Z"},{"alias_kind":"arxiv_version","alias_value":"1706.05002v2","created_at":"2026-05-18T00:22:59Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1706.05002","created_at":"2026-05-18T00:22:59Z"},{"alias_kind":"pith_short_12","alias_value":"WCFH6U6B43AV","created_at":"2026-05-18T12:31:53Z"},{"alias_kind":"pith_short_16","alias_value":"WCFH6U6B43AVD3P5","created_at":"2026-05-18T12:31:53Z"},{"alias_kind":"pith_short_8","alias_value":"WCFH6U6B","created_at":"2026-05-18T12:31:53Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2017:WCFH6U6B43AVD3P57TNUBX2JIU","target":"record","payload":{"canonical_record":{"source":{"id":"1706.05002","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-06-15T14:52:44Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"9e05fa55df47e8935b02ca44e0afda8b560884259ac2ed1ee96897b94a490d14","abstract_canon_sha256":"8423872319a5716cd85905cd821b6ca7b39a73c4b56d22ff0852d15bfd197df6"},"schema_version":"1.0"},"canonical_sha256":"b08a7f53c1e6c151edfdfcdb40df49452ccde735b7ae7b27a99775adeb030fc8","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:22:59.249164Z","signature_b64":"6vtQDLrULQt1D1vCIMx/PcE8SQEKDkNCKGzUm7Ml3pU6VHP4zM0xzKvItT1axioj8PLgEPSiZHDUVIppeqUgBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b08a7f53c1e6c151edfdfcdb40df49452ccde735b7ae7b27a99775adeb030fc8","last_reissued_at":"2026-05-18T00:22:59.248742Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:22:59.248742Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1706.05002","source_version":2,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:22:59Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"TtzZF5xo60Cr1IdJN8UNBurN55oLIjwp2lz8RSrbs0n3XvUwaextDHqyYOWZY4Gd35DSVJKUgI0/4c+X/jmwCw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-20T13:04:05.274186Z"},"content_sha256":"b9c4c02ab0e825bae750d541174af66c9dd7c8ca348ca103bff5d588e1a05b88","schema_version":"1.0","event_id":"sha256:b9c4c02ab0e825bae750d541174af66c9dd7c8ca348ca103bff5d588e1a05b88"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2017:WCFH6U6B43AVD3P57TNUBX2JIU","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"A multi-wavelength study of SXP 1062, the long period X-ray pulsar associated with a supernova remnant","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.HE","authors_text":"A. Gonzalez-Galan, F. Haberl, J. S. Gallagher III, L. M. Oskinova, M. A. Guerrero, M. Kuehnel, M. P. E. Schurch, S. B. Popov","submitted_at":"2017-06-15T14:52:44Z","abstract_excerpt":"SXP 1062 is a Be X-ray binary located in the Small Magellanic Cloud. It hosts a long-period X-ray pulsar and is likely associated with the supernova remnant MCSNR J0127-7332. In this work we present a multi-wavelength view on SXP 1062 in different luminosity regimes. We consider monitoring campaigns in optical (OGLE survey) and X-ray (SWIFT telescope). During these campaigns a tight coincidence of X-ray and optical outbursts is observed. We interpret this as typical Type I outbursts as often detected in Be X-ray binaries at periastron passage of the neutron star. To study different X-ray lumin"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1706.05002","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:22:59Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"s6Xw4c0RHrdKSBzmKMSQumxN4QZ0gGddM1aaUvlBEpLDHshffmPCI4F+wTTYaLrOGjSISY6XtSStl52OkUv3Bg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-20T13:04:05.274555Z"},"content_sha256":"8642aafd59e4829106e763d1fac2950520173e045554e34f37d927ada76b6b89","schema_version":"1.0","event_id":"sha256:8642aafd59e4829106e763d1fac2950520173e045554e34f37d927ada76b6b89"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/WCFH6U6B43AVD3P57TNUBX2JIU/bundle.json","state_url":"https://pith.science/pith/WCFH6U6B43AVD3P57TNUBX2JIU/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/WCFH6U6B43AVD3P57TNUBX2JIU/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-05-20T13:04:05Z","links":{"resolver":"https://pith.science/pith/WCFH6U6B43AVD3P57TNUBX2JIU","bundle":"https://pith.science/pith/WCFH6U6B43AVD3P57TNUBX2JIU/bundle.json","state":"https://pith.science/pith/WCFH6U6B43AVD3P57TNUBX2JIU/state.json","well_known_bundle":"https://pith.science/.well-known/pith/WCFH6U6B43AVD3P57TNUBX2JIU/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2017:WCFH6U6B43AVD3P57TNUBX2JIU","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"8423872319a5716cd85905cd821b6ca7b39a73c4b56d22ff0852d15bfd197df6","cross_cats_sorted":["astro-ph.SR"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-06-15T14:52:44Z","title_canon_sha256":"9e05fa55df47e8935b02ca44e0afda8b560884259ac2ed1ee96897b94a490d14"},"schema_version":"1.0","source":{"id":"1706.05002","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1706.05002","created_at":"2026-05-18T00:22:59Z"},{"alias_kind":"arxiv_version","alias_value":"1706.05002v2","created_at":"2026-05-18T00:22:59Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1706.05002","created_at":"2026-05-18T00:22:59Z"},{"alias_kind":"pith_short_12","alias_value":"WCFH6U6B43AV","created_at":"2026-05-18T12:31:53Z"},{"alias_kind":"pith_short_16","alias_value":"WCFH6U6B43AVD3P5","created_at":"2026-05-18T12:31:53Z"},{"alias_kind":"pith_short_8","alias_value":"WCFH6U6B","created_at":"2026-05-18T12:31:53Z"}],"graph_snapshots":[{"event_id":"sha256:8642aafd59e4829106e763d1fac2950520173e045554e34f37d927ada76b6b89","target":"graph","created_at":"2026-05-18T00:22:59Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"SXP 1062 is a Be X-ray binary located in the Small Magellanic Cloud. It hosts a long-period X-ray pulsar and is likely associated with the supernova remnant MCSNR J0127-7332. In this work we present a multi-wavelength view on SXP 1062 in different luminosity regimes. We consider monitoring campaigns in optical (OGLE survey) and X-ray (SWIFT telescope). During these campaigns a tight coincidence of X-ray and optical outbursts is observed. We interpret this as typical Type I outbursts as often detected in Be X-ray binaries at periastron passage of the neutron star. To study different X-ray lumin","authors_text":"A. Gonzalez-Galan, F. Haberl, J. S. Gallagher III, L. M. Oskinova, M. A. Guerrero, M. Kuehnel, M. P. E. Schurch, S. B. Popov","cross_cats":["astro-ph.SR"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-06-15T14:52:44Z","title":"A multi-wavelength study of SXP 1062, the long period X-ray pulsar associated with a supernova remnant"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1706.05002","kind":"arxiv","version":2},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:b9c4c02ab0e825bae750d541174af66c9dd7c8ca348ca103bff5d588e1a05b88","target":"record","created_at":"2026-05-18T00:22:59Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"8423872319a5716cd85905cd821b6ca7b39a73c4b56d22ff0852d15bfd197df6","cross_cats_sorted":["astro-ph.SR"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-06-15T14:52:44Z","title_canon_sha256":"9e05fa55df47e8935b02ca44e0afda8b560884259ac2ed1ee96897b94a490d14"},"schema_version":"1.0","source":{"id":"1706.05002","kind":"arxiv","version":2}},"canonical_sha256":"b08a7f53c1e6c151edfdfcdb40df49452ccde735b7ae7b27a99775adeb030fc8","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"b08a7f53c1e6c151edfdfcdb40df49452ccde735b7ae7b27a99775adeb030fc8","first_computed_at":"2026-05-18T00:22:59.248742Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:22:59.248742Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"6vtQDLrULQt1D1vCIMx/PcE8SQEKDkNCKGzUm7Ml3pU6VHP4zM0xzKvItT1axioj8PLgEPSiZHDUVIppeqUgBg==","signature_status":"signed_v1","signed_at":"2026-05-18T00:22:59.249164Z","signed_message":"canonical_sha256_bytes"},"source_id":"1706.05002","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:b9c4c02ab0e825bae750d541174af66c9dd7c8ca348ca103bff5d588e1a05b88","sha256:8642aafd59e4829106e763d1fac2950520173e045554e34f37d927ada76b6b89"],"state_sha256":"fdecaecb0b91e34aa59c9c97dc371c49614c8e44a73b54d1d2211253c10e2441"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"YCr79ZjpHXlFf2jyXfA+aJgyhR4NiyKM73YddmFYSmC8bxRrhxSQxX7ZXk+xXEINEywL2k4RgESY/1rl9DYeDA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-20T13:04:05.276745Z","bundle_sha256":"940327ddf42aca3a7a42739ad163148a9024ba62bd3c9860bacb774f61bdbad4"}}