{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2009:7TC64NMBDFGWSAMKZZJTFAXZYN","short_pith_number":"pith:7TC64NMB","canonical_record":{"source":{"id":"0909.3283","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2009-09-17T17:37:25Z","cross_cats_sorted":[],"title_canon_sha256":"8860906e4c89256b4a001daeb41fd87a69aeca11db52796b82cf4f660ab2edf5","abstract_canon_sha256":"21448d189555939d82abf0b55c2a4e0de355bff025d21b8b19096c5ed161a126"},"schema_version":"1.0"},"canonical_sha256":"fcc5ee3581194d69018ace533282f9c37c14cd5e85ce5e4642846be60639952e","source":{"kind":"arxiv","id":"0909.3283","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"0909.3283","created_at":"2026-05-18T02:11:46Z"},{"alias_kind":"arxiv_version","alias_value":"0909.3283v1","created_at":"2026-05-18T02:11:46Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0909.3283","created_at":"2026-05-18T02:11:46Z"},{"alias_kind":"pith_short_12","alias_value":"7TC64NMBDFGW","created_at":"2026-05-18T12:25:58Z"},{"alias_kind":"pith_short_16","alias_value":"7TC64NMBDFGWSAMK","created_at":"2026-05-18T12:25:58Z"},{"alias_kind":"pith_short_8","alias_value":"7TC64NMB","created_at":"2026-05-18T12:25:58Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2009:7TC64NMBDFGWSAMKZZJTFAXZYN","target":"record","payload":{"canonical_record":{"source":{"id":"0909.3283","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2009-09-17T17:37:25Z","cross_cats_sorted":[],"title_canon_sha256":"8860906e4c89256b4a001daeb41fd87a69aeca11db52796b82cf4f660ab2edf5","abstract_canon_sha256":"21448d189555939d82abf0b55c2a4e0de355bff025d21b8b19096c5ed161a126"},"schema_version":"1.0"},"canonical_sha256":"fcc5ee3581194d69018ace533282f9c37c14cd5e85ce5e4642846be60639952e","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:11:46.736287Z","signature_b64":"bbTBzfxmft/NEb8gJG6ALav2yYS/lan8IPrRvkR08yom0jsbhI/WOlfcPxHrU8U7lGPnsZcYgmySvPOTIUePDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fcc5ee3581194d69018ace533282f9c37c14cd5e85ce5e4642846be60639952e","last_reissued_at":"2026-05-18T02:11:46.735580Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:11:46.735580Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"0909.3283","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":"2026-05-18T02:11:46Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"dlGlYvOBL/2SOfLpuM+w2WEOKjchHD7fOr2BaSq517JPOhMGYdk2ITJW78Edd7fm6YQbbO1V+FMQlka6P/FrCA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-02T23:05:24.372726Z"},"content_sha256":"35e9954ad8e03b976fc2171a5f563405e2bd006a6a0f22b6735325f4c70e4de8","schema_version":"1.0","event_id":"sha256:35e9954ad8e03b976fc2171a5f563405e2bd006a6a0f22b6735325f4c70e4de8"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2009:7TC64NMBDFGWSAMKZZJTFAXZYN","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"The infrared/X-ray correlation of GX 339-4: Probing hard X-ray emission in accreting black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"C. D. Bailyn, E. Kalemci, E. Koerding, J. A. Tomsick, M. Coriat, M. M. Buxton, S. Corbel","submitted_at":"2009-09-17T17:37:25Z","abstract_excerpt":"GX 339-4 has been one of the key sources for unravelling the accretion ejection coupling in accreting stellar mass black holes. After a long period of quiescence between 1999 and 2002, GX 339-4 underwent a series of 4 outbursts that have been intensively observed by many ground based observatories [radio, infrared(IR), optical] and satellites (X-rays). Here, we present results of these broad-band observational campaigns, focusing on the optical-IR (OIR)/X-ray flux correlations over the four outbursts. We found tight OIR/X-ray correlations over four decades with the presence of a break in the I"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0909.3283","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":"2026-05-18T02:11:46Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"FO1vGBYqdIY7XInflvDcoB9VtfE0H1LFDyjtvxj3s5JSkN5l69vof20UVlt5vVzJhLm4ew4wgqecUkYg11VVCg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-02T23:05:24.373079Z"},"content_sha256":"dd89930f90830fd1efadaee2690da6c1f612c4c22ead3be3aa4145c77f1705e4","schema_version":"1.0","event_id":"sha256:dd89930f90830fd1efadaee2690da6c1f612c4c22ead3be3aa4145c77f1705e4"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/7TC64NMBDFGWSAMKZZJTFAXZYN/bundle.json","state_url":"https://pith.science/pith/7TC64NMBDFGWSAMKZZJTFAXZYN/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/7TC64NMBDFGWSAMKZZJTFAXZYN/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":"2026-06-02T23:05:24Z","links":{"resolver":"https://pith.science/pith/7TC64NMBDFGWSAMKZZJTFAXZYN","bundle":"https://pith.science/pith/7TC64NMBDFGWSAMKZZJTFAXZYN/bundle.json","state":"https://pith.science/pith/7TC64NMBDFGWSAMKZZJTFAXZYN/state.json","well_known_bundle":"https://pith.science/.well-known/pith/7TC64NMBDFGWSAMKZZJTFAXZYN/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2009:7TC64NMBDFGWSAMKZZJTFAXZYN","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":"21448d189555939d82abf0b55c2a4e0de355bff025d21b8b19096c5ed161a126","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2009-09-17T17:37:25Z","title_canon_sha256":"8860906e4c89256b4a001daeb41fd87a69aeca11db52796b82cf4f660ab2edf5"},"schema_version":"1.0","source":{"id":"0909.3283","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"0909.3283","created_at":"2026-05-18T02:11:46Z"},{"alias_kind":"arxiv_version","alias_value":"0909.3283v1","created_at":"2026-05-18T02:11:46Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0909.3283","created_at":"2026-05-18T02:11:46Z"},{"alias_kind":"pith_short_12","alias_value":"7TC64NMBDFGW","created_at":"2026-05-18T12:25:58Z"},{"alias_kind":"pith_short_16","alias_value":"7TC64NMBDFGWSAMK","created_at":"2026-05-18T12:25:58Z"},{"alias_kind":"pith_short_8","alias_value":"7TC64NMB","created_at":"2026-05-18T12:25:58Z"}],"graph_snapshots":[{"event_id":"sha256:dd89930f90830fd1efadaee2690da6c1f612c4c22ead3be3aa4145c77f1705e4","target":"graph","created_at":"2026-05-18T02:11:46Z","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":"GX 339-4 has been one of the key sources for unravelling the accretion ejection coupling in accreting stellar mass black holes. After a long period of quiescence between 1999 and 2002, GX 339-4 underwent a series of 4 outbursts that have been intensively observed by many ground based observatories [radio, infrared(IR), optical] and satellites (X-rays). Here, we present results of these broad-band observational campaigns, focusing on the optical-IR (OIR)/X-ray flux correlations over the four outbursts. We found tight OIR/X-ray correlations over four decades with the presence of a break in the I","authors_text":"C. D. Bailyn, E. Kalemci, E. Koerding, J. A. Tomsick, M. Coriat, M. M. Buxton, S. Corbel","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2009-09-17T17:37:25Z","title":"The infrared/X-ray correlation of GX 339-4: Probing hard X-ray emission in accreting black holes"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0909.3283","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":"sha256:35e9954ad8e03b976fc2171a5f563405e2bd006a6a0f22b6735325f4c70e4de8","target":"record","created_at":"2026-05-18T02:11:46Z","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":"21448d189555939d82abf0b55c2a4e0de355bff025d21b8b19096c5ed161a126","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2009-09-17T17:37:25Z","title_canon_sha256":"8860906e4c89256b4a001daeb41fd87a69aeca11db52796b82cf4f660ab2edf5"},"schema_version":"1.0","source":{"id":"0909.3283","kind":"arxiv","version":1}},"canonical_sha256":"fcc5ee3581194d69018ace533282f9c37c14cd5e85ce5e4642846be60639952e","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"fcc5ee3581194d69018ace533282f9c37c14cd5e85ce5e4642846be60639952e","first_computed_at":"2026-05-18T02:11:46.735580Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:11:46.735580Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"bbTBzfxmft/NEb8gJG6ALav2yYS/lan8IPrRvkR08yom0jsbhI/WOlfcPxHrU8U7lGPnsZcYgmySvPOTIUePDw==","signature_status":"signed_v1","signed_at":"2026-05-18T02:11:46.736287Z","signed_message":"canonical_sha256_bytes"},"source_id":"0909.3283","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:35e9954ad8e03b976fc2171a5f563405e2bd006a6a0f22b6735325f4c70e4de8","sha256:dd89930f90830fd1efadaee2690da6c1f612c4c22ead3be3aa4145c77f1705e4"],"state_sha256":"5dc68b3a2d0cb8d01ed23bec478b88432a302ea0a6c7c77d408512716feef449"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Hi71XGPRDRmizwWuPk/iHPuZ5U/fzQECO7w0I83XaTsthsuM1OHJW50+8Aog3Bsro75BJL3UNZKHKHhtoPwDCg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-02T23:05:24.375647Z","bundle_sha256":"c2979886dcee2283b18cd013bdccd6c3068f546f93cf592ad634952927db9670"}}