{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2013:HUZ5SCHRJE3OCX7NAS26GWW53P","short_pith_number":"pith:HUZ5SCHR","canonical_record":{"source":{"id":"1312.7029","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-12-25T23:28:48Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"ce3ca79f23a9128a51032fdd0859e67266105efceb9f47f50dccb8ee49802df2","abstract_canon_sha256":"f56d6bf332919b6c54f89b8799175fdfd6e2b86d2e9b703904c6b8d43b520bb5"},"schema_version":"1.0"},"canonical_sha256":"3d33d908f14936e15fed04b5e35adddbe71b177a82324f432971f4107b4bf27a","source":{"kind":"arxiv","id":"1312.7029","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1312.7029","created_at":"2026-05-18T02:52:58Z"},{"alias_kind":"arxiv_version","alias_value":"1312.7029v2","created_at":"2026-05-18T02:52:58Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1312.7029","created_at":"2026-05-18T02:52:58Z"},{"alias_kind":"pith_short_12","alias_value":"HUZ5SCHRJE3O","created_at":"2026-05-18T12:27:46Z"},{"alias_kind":"pith_short_16","alias_value":"HUZ5SCHRJE3OCX7N","created_at":"2026-05-18T12:27:46Z"},{"alias_kind":"pith_short_8","alias_value":"HUZ5SCHR","created_at":"2026-05-18T12:27:46Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2013:HUZ5SCHRJE3OCX7NAS26GWW53P","target":"record","payload":{"canonical_record":{"source":{"id":"1312.7029","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-12-25T23:28:48Z","cross_cats_sorted":["astro-ph.GA"],"title_canon_sha256":"ce3ca79f23a9128a51032fdd0859e67266105efceb9f47f50dccb8ee49802df2","abstract_canon_sha256":"f56d6bf332919b6c54f89b8799175fdfd6e2b86d2e9b703904c6b8d43b520bb5"},"schema_version":"1.0"},"canonical_sha256":"3d33d908f14936e15fed04b5e35adddbe71b177a82324f432971f4107b4bf27a","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:52:58.008496Z","signature_b64":"OLBc5SYJ+Zhgp5vtOPoFe9iTQXvjJAdTzIk8nFWx5AbzWc06UgXWpoaf569ila8OnCdBQxSCHmXgkXz4T6lCBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3d33d908f14936e15fed04b5e35adddbe71b177a82324f432971f4107b4bf27a","last_reissued_at":"2026-05-18T02:52:58.007987Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:52:58.007987Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1312.7029","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":"2026-05-18T02:52:58Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"QUSR3FiK1eL37R64LIpaEEztBgg9GfWRofRelW7SpX7D2Hui5vlIBd8RPiemAo7Hnr8GsB7AgWYhLHRBUIAtCQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-30T13:12:47.158958Z"},"content_sha256":"7a1cd737f20d878b20ce659482f96b33532f2181d5a4beb2ad1b3703b2fd6314","schema_version":"1.0","event_id":"sha256:7a1cd737f20d878b20ce659482f96b33532f2181d5a4beb2ad1b3703b2fd6314"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2013:HUZ5SCHRJE3OCX7NAS26GWW53P","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"A thin diffuse component of the Galactic Ridge X-ray emission and heating of the interstellar medium contributed by the radiation of Galactic X-ray binaries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"Margherita Molaro, Rashid Sunyaev, Rishi Khatri","submitted_at":"2013-12-25T23:28:48Z","abstract_excerpt":"We predict a thin (scale height $\\sim$ 80 pc) diffuse component of the Galactic Ridge X-ray emission (GRXE) arising from the scattering of the radiation of bright X-ray binaries (XBs) by the interstellar medium (ISM). The morphology of this scattered component is expected to trace the clumpy molecular and HI clouds. We calculate this contribution to the GRXE from known Galactic XBs assuming that they are all persistent. The known XBs sample is incomplete, however, because it is flux limited and spans the lifetime of X-ray astronomy ($\\sim 50$ years). We therefore also use a simulated sample of"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1312.7029","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":"2026-05-18T02:52:58Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"9Mz41LXmXvVq9n5bWBfZF6rjky1OJ4aSa7m0sf/nZBBNuuK/SsZ5U/HIyFU7oDkrPZa7lG3LqSEn+em7EavdDw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-30T13:12:47.159790Z"},"content_sha256":"8e02b75c0e320a9466a27ef3a663bfabf9f2b6a8edcc21f9368da1262e4f0549","schema_version":"1.0","event_id":"sha256:8e02b75c0e320a9466a27ef3a663bfabf9f2b6a8edcc21f9368da1262e4f0549"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/HUZ5SCHRJE3OCX7NAS26GWW53P/bundle.json","state_url":"https://pith.science/pith/HUZ5SCHRJE3OCX7NAS26GWW53P/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/HUZ5SCHRJE3OCX7NAS26GWW53P/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":"2026-05-30T13:12:47Z","links":{"resolver":"https://pith.science/pith/HUZ5SCHRJE3OCX7NAS26GWW53P","bundle":"https://pith.science/pith/HUZ5SCHRJE3OCX7NAS26GWW53P/bundle.json","state":"https://pith.science/pith/HUZ5SCHRJE3OCX7NAS26GWW53P/state.json","well_known_bundle":"https://pith.science/.well-known/pith/HUZ5SCHRJE3OCX7NAS26GWW53P/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2013:HUZ5SCHRJE3OCX7NAS26GWW53P","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":"f56d6bf332919b6c54f89b8799175fdfd6e2b86d2e9b703904c6b8d43b520bb5","cross_cats_sorted":["astro-ph.GA"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-12-25T23:28:48Z","title_canon_sha256":"ce3ca79f23a9128a51032fdd0859e67266105efceb9f47f50dccb8ee49802df2"},"schema_version":"1.0","source":{"id":"1312.7029","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1312.7029","created_at":"2026-05-18T02:52:58Z"},{"alias_kind":"arxiv_version","alias_value":"1312.7029v2","created_at":"2026-05-18T02:52:58Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1312.7029","created_at":"2026-05-18T02:52:58Z"},{"alias_kind":"pith_short_12","alias_value":"HUZ5SCHRJE3O","created_at":"2026-05-18T12:27:46Z"},{"alias_kind":"pith_short_16","alias_value":"HUZ5SCHRJE3OCX7N","created_at":"2026-05-18T12:27:46Z"},{"alias_kind":"pith_short_8","alias_value":"HUZ5SCHR","created_at":"2026-05-18T12:27:46Z"}],"graph_snapshots":[{"event_id":"sha256:8e02b75c0e320a9466a27ef3a663bfabf9f2b6a8edcc21f9368da1262e4f0549","target":"graph","created_at":"2026-05-18T02:52:58Z","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":"We predict a thin (scale height $\\sim$ 80 pc) diffuse component of the Galactic Ridge X-ray emission (GRXE) arising from the scattering of the radiation of bright X-ray binaries (XBs) by the interstellar medium (ISM). The morphology of this scattered component is expected to trace the clumpy molecular and HI clouds. We calculate this contribution to the GRXE from known Galactic XBs assuming that they are all persistent. The known XBs sample is incomplete, however, because it is flux limited and spans the lifetime of X-ray astronomy ($\\sim 50$ years). We therefore also use a simulated sample of","authors_text":"Margherita Molaro, Rashid Sunyaev, Rishi Khatri","cross_cats":["astro-ph.GA"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-12-25T23:28:48Z","title":"A thin diffuse component of the Galactic Ridge X-ray emission and heating of the interstellar medium contributed by the radiation of Galactic X-ray binaries"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1312.7029","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":"sha256:7a1cd737f20d878b20ce659482f96b33532f2181d5a4beb2ad1b3703b2fd6314","target":"record","created_at":"2026-05-18T02:52:58Z","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":"f56d6bf332919b6c54f89b8799175fdfd6e2b86d2e9b703904c6b8d43b520bb5","cross_cats_sorted":["astro-ph.GA"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-12-25T23:28:48Z","title_canon_sha256":"ce3ca79f23a9128a51032fdd0859e67266105efceb9f47f50dccb8ee49802df2"},"schema_version":"1.0","source":{"id":"1312.7029","kind":"arxiv","version":2}},"canonical_sha256":"3d33d908f14936e15fed04b5e35adddbe71b177a82324f432971f4107b4bf27a","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"3d33d908f14936e15fed04b5e35adddbe71b177a82324f432971f4107b4bf27a","first_computed_at":"2026-05-18T02:52:58.007987Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:52:58.007987Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"OLBc5SYJ+Zhgp5vtOPoFe9iTQXvjJAdTzIk8nFWx5AbzWc06UgXWpoaf569ila8OnCdBQxSCHmXgkXz4T6lCBg==","signature_status":"signed_v1","signed_at":"2026-05-18T02:52:58.008496Z","signed_message":"canonical_sha256_bytes"},"source_id":"1312.7029","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:7a1cd737f20d878b20ce659482f96b33532f2181d5a4beb2ad1b3703b2fd6314","sha256:8e02b75c0e320a9466a27ef3a663bfabf9f2b6a8edcc21f9368da1262e4f0549"],"state_sha256":"d5b1d49b9ab61b73cb08f416a994fd4dea96397181e9f38fa3f4c2906c8bada7"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"h93kGRjuk9JKifq0UVSakSiC7Xv/iuRA23hAvE+f8Mcp+FjLG+WZFcA/MAq+bCjFaIopvcYeO14hlfgbfmr3Bw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-30T13:12:47.163942Z","bundle_sha256":"3c1c69cf53c4bd2cfdc89b505f3d7be61250a7fd3677b0ef7866ac742f5c20a8"}}