{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2010:VO5FGTT3CNUMSIMEWGUPI6AZGW","short_pith_number":"pith:VO5FGTT3","canonical_record":{"source":{"id":"1008.5060","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2010-08-30T11:46:31Z","cross_cats_sorted":[],"title_canon_sha256":"43460fc66a0932b47fd48e3c979b9ca0d998508dd50c08e91907a9ed858e1136","abstract_canon_sha256":"dfc16c9bfcb883484db6691b8dfdca508f85382129279cfa8f31d8279fe695f2"},"schema_version":"1.0"},"canonical_sha256":"abba534e7b1368c92184b1a8f4781935a545f7970371505bbe8ce914e7967f14","source":{"kind":"arxiv","id":"1008.5060","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1008.5060","created_at":"2026-05-18T02:05:41Z"},{"alias_kind":"arxiv_version","alias_value":"1008.5060v1","created_at":"2026-05-18T02:05:41Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1008.5060","created_at":"2026-05-18T02:05:41Z"},{"alias_kind":"pith_short_12","alias_value":"VO5FGTT3CNUM","created_at":"2026-05-18T12:26:15Z"},{"alias_kind":"pith_short_16","alias_value":"VO5FGTT3CNUMSIME","created_at":"2026-05-18T12:26:15Z"},{"alias_kind":"pith_short_8","alias_value":"VO5FGTT3","created_at":"2026-05-18T12:26:15Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2010:VO5FGTT3CNUMSIMEWGUPI6AZGW","target":"record","payload":{"canonical_record":{"source":{"id":"1008.5060","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2010-08-30T11:46:31Z","cross_cats_sorted":[],"title_canon_sha256":"43460fc66a0932b47fd48e3c979b9ca0d998508dd50c08e91907a9ed858e1136","abstract_canon_sha256":"dfc16c9bfcb883484db6691b8dfdca508f85382129279cfa8f31d8279fe695f2"},"schema_version":"1.0"},"canonical_sha256":"abba534e7b1368c92184b1a8f4781935a545f7970371505bbe8ce914e7967f14","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:05:41.450636Z","signature_b64":"nvfoVYt5G5Xa7U8RvW+Etf9LkJpLbp6ZDN2ZTu0vFgEC85Em74s0Ho87wLN0NsdmJfVYSlO+NBv7+LGzOXCoDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"abba534e7b1368c92184b1a8f4781935a545f7970371505bbe8ce914e7967f14","last_reissued_at":"2026-05-18T02:05:41.450010Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:05:41.450010Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1008.5060","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":"2026-05-18T02:05:41Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"cx05kKxkdOq6v419a2o9TCl7/eK7jIFuUErg8azqBuiEFVoyaNHXKB+GEZDcAwM6IfHaj4zch8Bfp6YUNlfaDQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-03T20:26:04.183437Z"},"content_sha256":"190ffe404349562d6df29582495970ec51183d01dc7e8d7ea9bcb7967c012bac","schema_version":"1.0","event_id":"sha256:190ffe404349562d6df29582495970ec51183d01dc7e8d7ea9bcb7967c012bac"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2010:VO5FGTT3CNUMSIMEWGUPI6AZGW","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Compact Binaries in Star Clusters II - Escapers and Detection Rates","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"J. M. B. Downing, M. Giersz, M. J. Benacquista, R. Spurzem","submitted_at":"2010-08-30T11:46:31Z","abstract_excerpt":"We use a self-consistent Monte Carlo treatment of stellar dynamics to investigate black hole binaries that are dynamically ejected from globular clusters to determine if they will be gravitational wave sources. We find that many of the ejected binaries have initially short periods and will merge within a Hubble time due to gravitational wave radiation. Thus they are potential sources for ground-based gravitational wave detectors. We estimate the yearly detection rate for current and advanced ground-based detectors and find a modest enhancement over the rate predicted for binaries produced by p"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1008.5060","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":"2026-05-18T02:05:41Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"KIjcD5JHCimgCvFAb4W2khD27uukmT6FhE7qaOj7zmCqZW+tcms52m9nglGk4/j9oaOZzZTujdgFQ5QMXfy8Dw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-03T20:26:04.183780Z"},"content_sha256":"7c461e567962ac3179ac60ec1c978c31df734ef9fa57e30380ff9f7d8baf9812","schema_version":"1.0","event_id":"sha256:7c461e567962ac3179ac60ec1c978c31df734ef9fa57e30380ff9f7d8baf9812"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/VO5FGTT3CNUMSIMEWGUPI6AZGW/bundle.json","state_url":"https://pith.science/pith/VO5FGTT3CNUMSIMEWGUPI6AZGW/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/VO5FGTT3CNUMSIMEWGUPI6AZGW/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":"2026-06-03T20:26:04Z","links":{"resolver":"https://pith.science/pith/VO5FGTT3CNUMSIMEWGUPI6AZGW","bundle":"https://pith.science/pith/VO5FGTT3CNUMSIMEWGUPI6AZGW/bundle.json","state":"https://pith.science/pith/VO5FGTT3CNUMSIMEWGUPI6AZGW/state.json","well_known_bundle":"https://pith.science/.well-known/pith/VO5FGTT3CNUMSIMEWGUPI6AZGW/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2010:VO5FGTT3CNUMSIMEWGUPI6AZGW","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":"dfc16c9bfcb883484db6691b8dfdca508f85382129279cfa8f31d8279fe695f2","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2010-08-30T11:46:31Z","title_canon_sha256":"43460fc66a0932b47fd48e3c979b9ca0d998508dd50c08e91907a9ed858e1136"},"schema_version":"1.0","source":{"id":"1008.5060","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1008.5060","created_at":"2026-05-18T02:05:41Z"},{"alias_kind":"arxiv_version","alias_value":"1008.5060v1","created_at":"2026-05-18T02:05:41Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1008.5060","created_at":"2026-05-18T02:05:41Z"},{"alias_kind":"pith_short_12","alias_value":"VO5FGTT3CNUM","created_at":"2026-05-18T12:26:15Z"},{"alias_kind":"pith_short_16","alias_value":"VO5FGTT3CNUMSIME","created_at":"2026-05-18T12:26:15Z"},{"alias_kind":"pith_short_8","alias_value":"VO5FGTT3","created_at":"2026-05-18T12:26:15Z"}],"graph_snapshots":[{"event_id":"sha256:7c461e567962ac3179ac60ec1c978c31df734ef9fa57e30380ff9f7d8baf9812","target":"graph","created_at":"2026-05-18T02:05:41Z","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 use a self-consistent Monte Carlo treatment of stellar dynamics to investigate black hole binaries that are dynamically ejected from globular clusters to determine if they will be gravitational wave sources. We find that many of the ejected binaries have initially short periods and will merge within a Hubble time due to gravitational wave radiation. Thus they are potential sources for ground-based gravitational wave detectors. We estimate the yearly detection rate for current and advanced ground-based detectors and find a modest enhancement over the rate predicted for binaries produced by p","authors_text":"J. M. B. Downing, M. Giersz, M. J. Benacquista, R. Spurzem","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2010-08-30T11:46:31Z","title":"Compact Binaries in Star Clusters II - Escapers and Detection Rates"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1008.5060","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":"sha256:190ffe404349562d6df29582495970ec51183d01dc7e8d7ea9bcb7967c012bac","target":"record","created_at":"2026-05-18T02:05:41Z","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":"dfc16c9bfcb883484db6691b8dfdca508f85382129279cfa8f31d8279fe695f2","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2010-08-30T11:46:31Z","title_canon_sha256":"43460fc66a0932b47fd48e3c979b9ca0d998508dd50c08e91907a9ed858e1136"},"schema_version":"1.0","source":{"id":"1008.5060","kind":"arxiv","version":1}},"canonical_sha256":"abba534e7b1368c92184b1a8f4781935a545f7970371505bbe8ce914e7967f14","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"abba534e7b1368c92184b1a8f4781935a545f7970371505bbe8ce914e7967f14","first_computed_at":"2026-05-18T02:05:41.450010Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:05:41.450010Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"nvfoVYt5G5Xa7U8RvW+Etf9LkJpLbp6ZDN2ZTu0vFgEC85Em74s0Ho87wLN0NsdmJfVYSlO+NBv7+LGzOXCoDQ==","signature_status":"signed_v1","signed_at":"2026-05-18T02:05:41.450636Z","signed_message":"canonical_sha256_bytes"},"source_id":"1008.5060","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:190ffe404349562d6df29582495970ec51183d01dc7e8d7ea9bcb7967c012bac","sha256:7c461e567962ac3179ac60ec1c978c31df734ef9fa57e30380ff9f7d8baf9812"],"state_sha256":"af9496a3a9f315bfc39ab90162304b4cc85b68df24f29d9682bda633e8370d9d"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"ZgO+6vfIk+IJ8AwExhFGQNt3X3MVf7M0EZ4lXVt/QOsJLUojHKit0HJkyiGgW09Iv422ZtfkL1XgEe4WFhcFCw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-03T20:26:04.185715Z","bundle_sha256":"34622fee3af36b00163e971aa946803617727c9225a02cb92f14bcd14d66b9d6"}}