{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2011:APE6DYIC47W3BEP57HA3MKD3UK","short_pith_number":"pith:APE6DYIC","canonical_record":{"source":{"id":"1104.4810","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-04-25T20:58:15Z","cross_cats_sorted":[],"title_canon_sha256":"90c8c6750ba98a9e45db653b21edc72c0c73350d77a2031eaec34a62579a7a74","abstract_canon_sha256":"245aee90305fb0b5cf7f63e2b75b0cd669f6c5497a79f7d7259cad06b6b94a3b"},"schema_version":"1.0"},"canonical_sha256":"03c9e1e102e7edb091fdf9c1b6287ba2b2cb11b6325d0a511bcdfc027e736c36","source":{"kind":"arxiv","id":"1104.4810","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1104.4810","created_at":"2026-05-18T02:02:15Z"},{"alias_kind":"arxiv_version","alias_value":"1104.4810v2","created_at":"2026-05-18T02:02:15Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1104.4810","created_at":"2026-05-18T02:02:15Z"},{"alias_kind":"pith_short_12","alias_value":"APE6DYIC47W3","created_at":"2026-05-18T12:26:24Z"},{"alias_kind":"pith_short_16","alias_value":"APE6DYIC47W3BEP5","created_at":"2026-05-18T12:26:24Z"},{"alias_kind":"pith_short_8","alias_value":"APE6DYIC","created_at":"2026-05-18T12:26:24Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2011:APE6DYIC47W3BEP57HA3MKD3UK","target":"record","payload":{"canonical_record":{"source":{"id":"1104.4810","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-04-25T20:58:15Z","cross_cats_sorted":[],"title_canon_sha256":"90c8c6750ba98a9e45db653b21edc72c0c73350d77a2031eaec34a62579a7a74","abstract_canon_sha256":"245aee90305fb0b5cf7f63e2b75b0cd669f6c5497a79f7d7259cad06b6b94a3b"},"schema_version":"1.0"},"canonical_sha256":"03c9e1e102e7edb091fdf9c1b6287ba2b2cb11b6325d0a511bcdfc027e736c36","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:02:15.188468Z","signature_b64":"ivFNOO3Fm2qHSISMYm9dR4IUR/XDxiw3fDD40A0VcMKDKpmitEPRYPGPvJC/roEIQPzXgZzGF0DivcYU3ieZDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"03c9e1e102e7edb091fdf9c1b6287ba2b2cb11b6325d0a511bcdfc027e736c36","last_reissued_at":"2026-05-18T02:02:15.187704Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:02:15.187704Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1104.4810","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":"2026-05-18T02:02:15Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"AMb4ClUKsxVVrVI7YfRF9xfxpHWR36iHLchwxh8G32vitPOD4Gkcx8C85tiDbYbqwDIqpaxUDFEryd9pkdg7Cg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-02T16:30:14.257196Z"},"content_sha256":"bea8eb5a29a22834d60a07dcb3a584fccd6caa0df4ba01d760b7df3e813829ca","schema_version":"1.0","event_id":"sha256:bea8eb5a29a22834d60a07dcb3a584fccd6caa0df4ba01d760b7df3e813829ca"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2011:APE6DYIC47W3BEP57HA3MKD3UK","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"An Interferometric and Spectroscopic Analysis of the Multiple Star System HD 193322","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Alexander W. Fullerton, Brian D. Mason, Christopher D. Farrington, David P. O'Brien, Douglas R. Gies, Erika D. Grundstrom, Gail H. Schaefer, Harold A. McAlister, Jr., Judit Sturmann, Laszlo Sturmann, Lewis C. Roberts, M. Virginia McSwain, Nils H. Turner, Rachel A. Matson, Sergio Simon-Diaz, Stephen J. Williams, Theo A. ten Brummelaar, William I. Hartkopf","submitted_at":"2011-04-25T20:58:15Z","abstract_excerpt":"The star HD 193322 is a remarkable multiple system of massive stars that lies at the heart of the cluster Collinder 419. Here we report on new spectroscopic observations and radial velocities of the narrow-lined component Ab1 that we use to determine its orbital motion around a close companion Ab2 ($P = 312$ d) and around a distant third star Aa ($P = 35$ y).We have also obtained long baseline interferometry of the target in the $K^\\prime$-band with the CHARA Array that we use in two ways. First, we combine published speckle interferometric measurements with CHARA separated fringe packet measu"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1104.4810","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":"2026-05-18T02:02:15Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"C/Y5kckmc4o6Aeh25Wh396JBQGgf/bo0iDqpx2Ujrq4++J10q/m7PnUQwnAHDP7zwVWd/rfhp4LvAMzbS0fLDA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-02T16:30:14.257549Z"},"content_sha256":"cea950417bc44b63e980f8174656281b156d991acda1626ab75aa8b235bb1238","schema_version":"1.0","event_id":"sha256:cea950417bc44b63e980f8174656281b156d991acda1626ab75aa8b235bb1238"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/APE6DYIC47W3BEP57HA3MKD3UK/bundle.json","state_url":"https://pith.science/pith/APE6DYIC47W3BEP57HA3MKD3UK/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/APE6DYIC47W3BEP57HA3MKD3UK/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":"2026-06-02T16:30:14Z","links":{"resolver":"https://pith.science/pith/APE6DYIC47W3BEP57HA3MKD3UK","bundle":"https://pith.science/pith/APE6DYIC47W3BEP57HA3MKD3UK/bundle.json","state":"https://pith.science/pith/APE6DYIC47W3BEP57HA3MKD3UK/state.json","well_known_bundle":"https://pith.science/.well-known/pith/APE6DYIC47W3BEP57HA3MKD3UK/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2011:APE6DYIC47W3BEP57HA3MKD3UK","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":"245aee90305fb0b5cf7f63e2b75b0cd669f6c5497a79f7d7259cad06b6b94a3b","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-04-25T20:58:15Z","title_canon_sha256":"90c8c6750ba98a9e45db653b21edc72c0c73350d77a2031eaec34a62579a7a74"},"schema_version":"1.0","source":{"id":"1104.4810","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1104.4810","created_at":"2026-05-18T02:02:15Z"},{"alias_kind":"arxiv_version","alias_value":"1104.4810v2","created_at":"2026-05-18T02:02:15Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1104.4810","created_at":"2026-05-18T02:02:15Z"},{"alias_kind":"pith_short_12","alias_value":"APE6DYIC47W3","created_at":"2026-05-18T12:26:24Z"},{"alias_kind":"pith_short_16","alias_value":"APE6DYIC47W3BEP5","created_at":"2026-05-18T12:26:24Z"},{"alias_kind":"pith_short_8","alias_value":"APE6DYIC","created_at":"2026-05-18T12:26:24Z"}],"graph_snapshots":[{"event_id":"sha256:cea950417bc44b63e980f8174656281b156d991acda1626ab75aa8b235bb1238","target":"graph","created_at":"2026-05-18T02:02:15Z","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":"The star HD 193322 is a remarkable multiple system of massive stars that lies at the heart of the cluster Collinder 419. Here we report on new spectroscopic observations and radial velocities of the narrow-lined component Ab1 that we use to determine its orbital motion around a close companion Ab2 ($P = 312$ d) and around a distant third star Aa ($P = 35$ y).We have also obtained long baseline interferometry of the target in the $K^\\prime$-band with the CHARA Array that we use in two ways. First, we combine published speckle interferometric measurements with CHARA separated fringe packet measu","authors_text":"Alexander W. Fullerton, Brian D. Mason, Christopher D. Farrington, David P. O'Brien, Douglas R. Gies, Erika D. Grundstrom, Gail H. Schaefer, Harold A. McAlister, Jr., Judit Sturmann, Laszlo Sturmann, Lewis C. Roberts, M. Virginia McSwain, Nils H. Turner, Rachel A. Matson, Sergio Simon-Diaz, Stephen J. Williams, Theo A. ten Brummelaar, William I. Hartkopf","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-04-25T20:58:15Z","title":"An Interferometric and Spectroscopic Analysis of the Multiple Star System HD 193322"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1104.4810","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:bea8eb5a29a22834d60a07dcb3a584fccd6caa0df4ba01d760b7df3e813829ca","target":"record","created_at":"2026-05-18T02:02:15Z","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":"245aee90305fb0b5cf7f63e2b75b0cd669f6c5497a79f7d7259cad06b6b94a3b","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-04-25T20:58:15Z","title_canon_sha256":"90c8c6750ba98a9e45db653b21edc72c0c73350d77a2031eaec34a62579a7a74"},"schema_version":"1.0","source":{"id":"1104.4810","kind":"arxiv","version":2}},"canonical_sha256":"03c9e1e102e7edb091fdf9c1b6287ba2b2cb11b6325d0a511bcdfc027e736c36","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"03c9e1e102e7edb091fdf9c1b6287ba2b2cb11b6325d0a511bcdfc027e736c36","first_computed_at":"2026-05-18T02:02:15.187704Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:02:15.187704Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"ivFNOO3Fm2qHSISMYm9dR4IUR/XDxiw3fDD40A0VcMKDKpmitEPRYPGPvJC/roEIQPzXgZzGF0DivcYU3ieZDQ==","signature_status":"signed_v1","signed_at":"2026-05-18T02:02:15.188468Z","signed_message":"canonical_sha256_bytes"},"source_id":"1104.4810","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:bea8eb5a29a22834d60a07dcb3a584fccd6caa0df4ba01d760b7df3e813829ca","sha256:cea950417bc44b63e980f8174656281b156d991acda1626ab75aa8b235bb1238"],"state_sha256":"8679124d7f2a79b79c288940e3e6b9410785c8b8c7cb264a6a39453a070f28fb"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"GGlOpiRgTGm1SBd39o1bQuPHJkCd61J/86hbJ6LezwzWImtQYFRVbO2BtoQyZkEcFe9k0cHg7yMphdPDl1qwAw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-02T16:30:14.259403Z","bundle_sha256":"c79408a97c4e53085c5eb971d5f1e5fe7e69b5d5189c6e182a827f3d06a07353"}}