{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2013:SYWLDQ5RCP37XAW4MZCX63I6CP","short_pith_number":"pith:SYWLDQ5R","canonical_record":{"source":{"id":"1310.7588","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-10-28T20:00:07Z","cross_cats_sorted":["astro-ph.GA","astro-ph.HE"],"title_canon_sha256":"3f779ab3ccd332f76ca1c814c216cedee273fda7f948ba825e95845f0cb67757","abstract_canon_sha256":"5fe928a7e638f18a7aca021ddc222ecf8003f16bd316ea1488d927b897804f3f"},"schema_version":"1.0"},"canonical_sha256":"962cb1c3b113f7fb82dc66457f6d1e13ed75a864f677bd9d64025f2738bdef3b","source":{"kind":"arxiv","id":"1310.7588","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1310.7588","created_at":"2026-05-18T01:46:48Z"},{"alias_kind":"arxiv_version","alias_value":"1310.7588v1","created_at":"2026-05-18T01:46:48Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1310.7588","created_at":"2026-05-18T01:46:48Z"},{"alias_kind":"pith_short_12","alias_value":"SYWLDQ5RCP37","created_at":"2026-05-18T12:27:59Z"},{"alias_kind":"pith_short_16","alias_value":"SYWLDQ5RCP37XAW4","created_at":"2026-05-18T12:27:59Z"},{"alias_kind":"pith_short_8","alias_value":"SYWLDQ5R","created_at":"2026-05-18T12:27:59Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2013:SYWLDQ5RCP37XAW4MZCX63I6CP","target":"record","payload":{"canonical_record":{"source":{"id":"1310.7588","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-10-28T20:00:07Z","cross_cats_sorted":["astro-ph.GA","astro-ph.HE"],"title_canon_sha256":"3f779ab3ccd332f76ca1c814c216cedee273fda7f948ba825e95845f0cb67757","abstract_canon_sha256":"5fe928a7e638f18a7aca021ddc222ecf8003f16bd316ea1488d927b897804f3f"},"schema_version":"1.0"},"canonical_sha256":"962cb1c3b113f7fb82dc66457f6d1e13ed75a864f677bd9d64025f2738bdef3b","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:46:48.324860Z","signature_b64":"2xYULHmD+VaJYp6Re7b3b9V2ggrArUhMNakQLfufypmXAsnYLHyipz7FLm6WiG/Hx5WdRRRaO/LiI+mhdLAOCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"962cb1c3b113f7fb82dc66457f6d1e13ed75a864f677bd9d64025f2738bdef3b","last_reissued_at":"2026-05-18T01:46:48.324263Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:46:48.324263Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1310.7588","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":"2026-05-18T01:46:48Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"W4X0q/vX17hzQgLhEFIV4nRG1xUm9Qrv07/zamUbWFGM5flUaGdb0izupx7AnmLqGKdk4c74stuIv/afcVrjAw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T08:56:45.668130Z"},"content_sha256":"0b6abf78c6bf1be35c97e436531d8e5ab3110e82f146d31a9f2e56ec1791a052","schema_version":"1.0","event_id":"sha256:0b6abf78c6bf1be35c97e436531d8e5ab3110e82f146d31a9f2e56ec1791a052"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2013:SYWLDQ5RCP37XAW4MZCX63I6CP","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Detection of a High Brightness Temperature Radio Core in the AGN-Driven Molecular Outflow Candidate NGC 1266","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","astro-ph.HE"],"primary_cat":"astro-ph.CO","authors_text":"J. M. Wrobel, Katherine Alatalo, Kristina Nyland, Lisa M. Young, Martin Bureau, P. T. de Zeeuw, Raffaella Morganti, Susana Deustua, Timothy A. Davis","submitted_at":"2013-10-28T20:00:07Z","abstract_excerpt":"We present new high spatial resolution Karl G. Jansky Very Large Array (VLA) HI absorption and Very Long Baseline Array (VLBA) continuum observations of the Active Galactic Nucleus (AGN)-driven molecular outflow candidate NGC 1266. Although other well-known systems with molecular outflows may be driven by star formation in a central molecular disk, the molecular mass outflow rate reported in Alatalo et al. (2011) in NGC 1266 of 13 M$_{\\odot}$ year$^{-1}$ exceeds star formation rate estimates from a variety of tracers. This suggests that an additional energy source, such as an AGN, may play a s"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1310.7588","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":"2026-05-18T01:46:48Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"7Nro2sSnW21GkWRqvx5zD102qI0Ewp9IXtr1C33LLe9b49zn5jbD9APJN5Yk5YHFDhLU6H8QhlIynY8MG8RKBw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-25T08:56:45.669033Z"},"content_sha256":"5677e0fe6ee20146e8b1ebe87c78f5d6591a086d3567d88fadb3db17051ba2c2","schema_version":"1.0","event_id":"sha256:5677e0fe6ee20146e8b1ebe87c78f5d6591a086d3567d88fadb3db17051ba2c2"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/SYWLDQ5RCP37XAW4MZCX63I6CP/bundle.json","state_url":"https://pith.science/pith/SYWLDQ5RCP37XAW4MZCX63I6CP/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/SYWLDQ5RCP37XAW4MZCX63I6CP/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":"2026-05-25T08:56:45Z","links":{"resolver":"https://pith.science/pith/SYWLDQ5RCP37XAW4MZCX63I6CP","bundle":"https://pith.science/pith/SYWLDQ5RCP37XAW4MZCX63I6CP/bundle.json","state":"https://pith.science/pith/SYWLDQ5RCP37XAW4MZCX63I6CP/state.json","well_known_bundle":"https://pith.science/.well-known/pith/SYWLDQ5RCP37XAW4MZCX63I6CP/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2013:SYWLDQ5RCP37XAW4MZCX63I6CP","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":"5fe928a7e638f18a7aca021ddc222ecf8003f16bd316ea1488d927b897804f3f","cross_cats_sorted":["astro-ph.GA","astro-ph.HE"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-10-28T20:00:07Z","title_canon_sha256":"3f779ab3ccd332f76ca1c814c216cedee273fda7f948ba825e95845f0cb67757"},"schema_version":"1.0","source":{"id":"1310.7588","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1310.7588","created_at":"2026-05-18T01:46:48Z"},{"alias_kind":"arxiv_version","alias_value":"1310.7588v1","created_at":"2026-05-18T01:46:48Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1310.7588","created_at":"2026-05-18T01:46:48Z"},{"alias_kind":"pith_short_12","alias_value":"SYWLDQ5RCP37","created_at":"2026-05-18T12:27:59Z"},{"alias_kind":"pith_short_16","alias_value":"SYWLDQ5RCP37XAW4","created_at":"2026-05-18T12:27:59Z"},{"alias_kind":"pith_short_8","alias_value":"SYWLDQ5R","created_at":"2026-05-18T12:27:59Z"}],"graph_snapshots":[{"event_id":"sha256:5677e0fe6ee20146e8b1ebe87c78f5d6591a086d3567d88fadb3db17051ba2c2","target":"graph","created_at":"2026-05-18T01:46:48Z","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 present new high spatial resolution Karl G. Jansky Very Large Array (VLA) HI absorption and Very Long Baseline Array (VLBA) continuum observations of the Active Galactic Nucleus (AGN)-driven molecular outflow candidate NGC 1266. Although other well-known systems with molecular outflows may be driven by star formation in a central molecular disk, the molecular mass outflow rate reported in Alatalo et al. (2011) in NGC 1266 of 13 M$_{\\odot}$ year$^{-1}$ exceeds star formation rate estimates from a variety of tracers. This suggests that an additional energy source, such as an AGN, may play a s","authors_text":"J. M. Wrobel, Katherine Alatalo, Kristina Nyland, Lisa M. Young, Martin Bureau, P. T. de Zeeuw, Raffaella Morganti, Susana Deustua, Timothy A. Davis","cross_cats":["astro-ph.GA","astro-ph.HE"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-10-28T20:00:07Z","title":"Detection of a High Brightness Temperature Radio Core in the AGN-Driven Molecular Outflow Candidate NGC 1266"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1310.7588","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":"sha256:0b6abf78c6bf1be35c97e436531d8e5ab3110e82f146d31a9f2e56ec1791a052","target":"record","created_at":"2026-05-18T01:46:48Z","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":"5fe928a7e638f18a7aca021ddc222ecf8003f16bd316ea1488d927b897804f3f","cross_cats_sorted":["astro-ph.GA","astro-ph.HE"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2013-10-28T20:00:07Z","title_canon_sha256":"3f779ab3ccd332f76ca1c814c216cedee273fda7f948ba825e95845f0cb67757"},"schema_version":"1.0","source":{"id":"1310.7588","kind":"arxiv","version":1}},"canonical_sha256":"962cb1c3b113f7fb82dc66457f6d1e13ed75a864f677bd9d64025f2738bdef3b","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"962cb1c3b113f7fb82dc66457f6d1e13ed75a864f677bd9d64025f2738bdef3b","first_computed_at":"2026-05-18T01:46:48.324263Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:46:48.324263Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"2xYULHmD+VaJYp6Re7b3b9V2ggrArUhMNakQLfufypmXAsnYLHyipz7FLm6WiG/Hx5WdRRRaO/LiI+mhdLAOCQ==","signature_status":"signed_v1","signed_at":"2026-05-18T01:46:48.324860Z","signed_message":"canonical_sha256_bytes"},"source_id":"1310.7588","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:0b6abf78c6bf1be35c97e436531d8e5ab3110e82f146d31a9f2e56ec1791a052","sha256:5677e0fe6ee20146e8b1ebe87c78f5d6591a086d3567d88fadb3db17051ba2c2"],"state_sha256":"c96379ba2949c0f7b91f9353668155980dedeb14236a2f7980266801b553c4f5"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"xsZ59Fh3dvJvIpG9oOsMxSLhq0NepI6CAg5+DQB4t+EYetsucvSJi1qwG5NY2rDT6zz3x0NqGVKEIP+v0PZgCQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-25T08:56:45.672353Z","bundle_sha256":"b09f943684681365db45270803f62773bc3d60259012b4bf4b99ff17e31c9be4"}}