{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2014:KIS2JTDUUD4IKFCU6NRICPATCE","short_pith_number":"pith:KIS2JTDU","canonical_record":{"source":{"id":"1405.6750","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-05-26T21:59:43Z","cross_cats_sorted":[],"title_canon_sha256":"01f030d7eb3ab3fd85ac5ad1e5a6b4872bf7f1dce8c658f5c4a08dc31e68ae49","abstract_canon_sha256":"b9a3fa58265e473ee962cd511a9df8ca743920bc020cd685f43a8dd894f21796"},"schema_version":"1.0"},"canonical_sha256":"5225a4cc74a0f8851454f362813c13112011011cfcaabd8534be9f93abb95b02","source":{"kind":"arxiv","id":"1405.6750","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1405.6750","created_at":"2026-05-18T01:43:06Z"},{"alias_kind":"arxiv_version","alias_value":"1405.6750v1","created_at":"2026-05-18T01:43:06Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1405.6750","created_at":"2026-05-18T01:43:06Z"},{"alias_kind":"pith_short_12","alias_value":"KIS2JTDUUD4I","created_at":"2026-05-18T12:28:35Z"},{"alias_kind":"pith_short_16","alias_value":"KIS2JTDUUD4IKFCU","created_at":"2026-05-18T12:28:35Z"},{"alias_kind":"pith_short_8","alias_value":"KIS2JTDU","created_at":"2026-05-18T12:28:35Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2014:KIS2JTDUUD4IKFCU6NRICPATCE","target":"record","payload":{"canonical_record":{"source":{"id":"1405.6750","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-05-26T21:59:43Z","cross_cats_sorted":[],"title_canon_sha256":"01f030d7eb3ab3fd85ac5ad1e5a6b4872bf7f1dce8c658f5c4a08dc31e68ae49","abstract_canon_sha256":"b9a3fa58265e473ee962cd511a9df8ca743920bc020cd685f43a8dd894f21796"},"schema_version":"1.0"},"canonical_sha256":"5225a4cc74a0f8851454f362813c13112011011cfcaabd8534be9f93abb95b02","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:43:06.078593Z","signature_b64":"j67euYJu7zK3e3iy1eT2HhHjkvXJj5dNXTktN9QWWL2WaaMBzfvQ+r15KrJO0oA2j0C/OPu36x6OeFxYFWLzCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5225a4cc74a0f8851454f362813c13112011011cfcaabd8534be9f93abb95b02","last_reissued_at":"2026-05-18T01:43:06.077705Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:43:06.077705Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1405.6750","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:43:06Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"OPBGEUodvEEan5THpCOgYylIlR4v1od++O4eDzB5Fr80ZvPzBFRSrpVzKcKVpnB9sYEddxZvcCuNy6BVy5xsBA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-20T12:57:56.446630Z"},"content_sha256":"07935173c19b1169ecb0fa8bf33964d127d82d94357be63f7f2b1084064ef543","schema_version":"1.0","event_id":"sha256:07935173c19b1169ecb0fa8bf33964d127d82d94357be63f7f2b1084064ef543"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2014:KIS2JTDUUD4IKFCU6NRICPATCE","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Spectral and Timing Properties of the Black Hole X-ray Binary H 1743-322 in the Low/hard State Studied with Suzaku","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Aya Kubota, Chris Done, Kazutaka Yamaoka, Megumi Shidatsu, Shin'ya Yamada, Takafumi Hori, Takahiro Nagayama, Yoshihiro Ueda, Yuki Moritani","submitted_at":"2014-05-26T21:59:43Z","abstract_excerpt":"We report on the results from Suzaku observations of the Galactic black hole X-ray binary H 1743-322 in the low/hard state during its outburst in 2012 October. We appropriately take into account the effects of dust-scattering to accurately analyze the X-ray spectra. The time-averaged spectra in the 1-200 keV band are dominated by a hard power-law component of a photon index of \\approx 1.6 with a high-energy cutoff at \\approx 60 keV, which is well described with Comptonization of the disk emission by hot corona. We estimate the inner disk radius from the multi-color disk component, and find tha"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1405.6750","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T01:43:06Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"lS0PRv85IZQ3sbhdwI83IHaeECmh131eCDO1pQbMa+cAGouqq0QhpnoKBljhK971ZIevm9J/pBV0/+n1WtVfBg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-20T12:57:56.447008Z"},"content_sha256":"06dd45e5682a0ee4d68ff5e3dd01962562587dd36f7373ed0d28fe0e0e219283","schema_version":"1.0","event_id":"sha256:06dd45e5682a0ee4d68ff5e3dd01962562587dd36f7373ed0d28fe0e0e219283"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/KIS2JTDUUD4IKFCU6NRICPATCE/bundle.json","state_url":"https://pith.science/pith/KIS2JTDUUD4IKFCU6NRICPATCE/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/KIS2JTDUUD4IKFCU6NRICPATCE/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":"2026-05-20T12:57:56Z","links":{"resolver":"https://pith.science/pith/KIS2JTDUUD4IKFCU6NRICPATCE","bundle":"https://pith.science/pith/KIS2JTDUUD4IKFCU6NRICPATCE/bundle.json","state":"https://pith.science/pith/KIS2JTDUUD4IKFCU6NRICPATCE/state.json","well_known_bundle":"https://pith.science/.well-known/pith/KIS2JTDUUD4IKFCU6NRICPATCE/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2014:KIS2JTDUUD4IKFCU6NRICPATCE","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":"b9a3fa58265e473ee962cd511a9df8ca743920bc020cd685f43a8dd894f21796","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-05-26T21:59:43Z","title_canon_sha256":"01f030d7eb3ab3fd85ac5ad1e5a6b4872bf7f1dce8c658f5c4a08dc31e68ae49"},"schema_version":"1.0","source":{"id":"1405.6750","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1405.6750","created_at":"2026-05-18T01:43:06Z"},{"alias_kind":"arxiv_version","alias_value":"1405.6750v1","created_at":"2026-05-18T01:43:06Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1405.6750","created_at":"2026-05-18T01:43:06Z"},{"alias_kind":"pith_short_12","alias_value":"KIS2JTDUUD4I","created_at":"2026-05-18T12:28:35Z"},{"alias_kind":"pith_short_16","alias_value":"KIS2JTDUUD4IKFCU","created_at":"2026-05-18T12:28:35Z"},{"alias_kind":"pith_short_8","alias_value":"KIS2JTDU","created_at":"2026-05-18T12:28:35Z"}],"graph_snapshots":[{"event_id":"sha256:06dd45e5682a0ee4d68ff5e3dd01962562587dd36f7373ed0d28fe0e0e219283","target":"graph","created_at":"2026-05-18T01:43:06Z","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 report on the results from Suzaku observations of the Galactic black hole X-ray binary H 1743-322 in the low/hard state during its outburst in 2012 October. We appropriately take into account the effects of dust-scattering to accurately analyze the X-ray spectra. The time-averaged spectra in the 1-200 keV band are dominated by a hard power-law component of a photon index of \\approx 1.6 with a high-energy cutoff at \\approx 60 keV, which is well described with Comptonization of the disk emission by hot corona. We estimate the inner disk radius from the multi-color disk component, and find tha","authors_text":"Aya Kubota, Chris Done, Kazutaka Yamaoka, Megumi Shidatsu, Shin'ya Yamada, Takafumi Hori, Takahiro Nagayama, Yoshihiro Ueda, Yuki Moritani","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-05-26T21:59:43Z","title":"Spectral and Timing Properties of the Black Hole X-ray Binary H 1743-322 in the Low/hard State Studied with Suzaku"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1405.6750","kind":"arxiv","version":1},"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":"sha256:07935173c19b1169ecb0fa8bf33964d127d82d94357be63f7f2b1084064ef543","target":"record","created_at":"2026-05-18T01:43:06Z","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":"b9a3fa58265e473ee962cd511a9df8ca743920bc020cd685f43a8dd894f21796","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-05-26T21:59:43Z","title_canon_sha256":"01f030d7eb3ab3fd85ac5ad1e5a6b4872bf7f1dce8c658f5c4a08dc31e68ae49"},"schema_version":"1.0","source":{"id":"1405.6750","kind":"arxiv","version":1}},"canonical_sha256":"5225a4cc74a0f8851454f362813c13112011011cfcaabd8534be9f93abb95b02","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"5225a4cc74a0f8851454f362813c13112011011cfcaabd8534be9f93abb95b02","first_computed_at":"2026-05-18T01:43:06.077705Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:43:06.077705Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"j67euYJu7zK3e3iy1eT2HhHjkvXJj5dNXTktN9QWWL2WaaMBzfvQ+r15KrJO0oA2j0C/OPu36x6OeFxYFWLzCA==","signature_status":"signed_v1","signed_at":"2026-05-18T01:43:06.078593Z","signed_message":"canonical_sha256_bytes"},"source_id":"1405.6750","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:07935173c19b1169ecb0fa8bf33964d127d82d94357be63f7f2b1084064ef543","sha256:06dd45e5682a0ee4d68ff5e3dd01962562587dd36f7373ed0d28fe0e0e219283"],"state_sha256":"a34f863622ae90f44bd31a79c1b614b723461f133cb7f001e79eb6bd6ab2a648"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"MtIeHdeqBDHqzFtlYsXS6LhhdFEqZhrkqDyJ3xWfEJQQE6JrMiLy6XYXOLAZxm2eLOCz9VxYlqUVIylxVsllAQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-20T12:57:56.448996Z","bundle_sha256":"4103eecde6f78645cbeb56848e0c0b29c26238c5ef73f1ca01ac9baa02621451"}}