{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2017:6XPQQGK2LFPIIJB2PXPFISDC4R","short_pith_number":"pith:6XPQQGK2","canonical_record":{"source":{"id":"1705.06678","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-05-18T16:29:19Z","cross_cats_sorted":[],"title_canon_sha256":"12090fda16a26052bc718c2e5fc06497b750b2b37623dd1c87524d277df07f25","abstract_canon_sha256":"c2766dcc1da626371fafb840ab25e5b480007cfbc3eaba6c0751055d65e9554c"},"schema_version":"1.0"},"canonical_sha256":"f5df08195a595e84243a7dde544862e47df741b3e6e6acc5ab6f66941403868b","source":{"kind":"arxiv","id":"1705.06678","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1705.06678","created_at":"2026-05-18T00:16:56Z"},{"alias_kind":"arxiv_version","alias_value":"1705.06678v2","created_at":"2026-05-18T00:16:56Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1705.06678","created_at":"2026-05-18T00:16:56Z"},{"alias_kind":"pith_short_12","alias_value":"6XPQQGK2LFPI","created_at":"2026-05-18T12:31:03Z"},{"alias_kind":"pith_short_16","alias_value":"6XPQQGK2LFPIIJB2","created_at":"2026-05-18T12:31:03Z"},{"alias_kind":"pith_short_8","alias_value":"6XPQQGK2","created_at":"2026-05-18T12:31:03Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2017:6XPQQGK2LFPIIJB2PXPFISDC4R","target":"record","payload":{"canonical_record":{"source":{"id":"1705.06678","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-05-18T16:29:19Z","cross_cats_sorted":[],"title_canon_sha256":"12090fda16a26052bc718c2e5fc06497b750b2b37623dd1c87524d277df07f25","abstract_canon_sha256":"c2766dcc1da626371fafb840ab25e5b480007cfbc3eaba6c0751055d65e9554c"},"schema_version":"1.0"},"canonical_sha256":"f5df08195a595e84243a7dde544862e47df741b3e6e6acc5ab6f66941403868b","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:16:56.429282Z","signature_b64":"iE5ce21MmkQ1jIswwDEzgcMYKaWgUd5IRNP6Pxyt0D6ajbeNA2WyONi0apMqpo5wTp+0fNJKz+G1AGcTRdg1Cw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f5df08195a595e84243a7dde544862e47df741b3e6e6acc5ab6f66941403868b","last_reissued_at":"2026-05-18T00:16:56.428464Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:16:56.428464Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1705.06678","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":"2026-05-18T00:16:56Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"MoG/mZ0ybz/Z/YQkhm29Q8LwyG/0Y7bJtkIJxX4p9OB/Vry+NtugbO2egT8h86132aIurhWPy+mZGsTbo0jGDQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-01T21:12:28.144993Z"},"content_sha256":"16b1866b7ce1abbb03a1953b61dfe7ab5d72022658d1251de4368f8f42270c37","schema_version":"1.0","event_id":"sha256:16b1866b7ce1abbb03a1953b61dfe7ab5d72022658d1251de4368f8f42270c37"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2017:6XPQQGK2LFPIIJB2PXPFISDC4R","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"The Keck/OSIRIS Nearby AGN Survey (KONA) I. The Nuclear K-band Properties of Nearby AGN","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"B. Davis, E. K. S. Hicks, F. M\\\"uller-S\\'anchez, M. Malkan, P. C. Yu, R. Davies, S. Shaver","submitted_at":"2017-05-18T16:29:19Z","abstract_excerpt":"We introduce the Keck Osiris Nearby AGN survey (KONA), a new adaptive optics-assisted integral-field spectroscopic survey of Seyfert galaxies. KONA permits at ~0.1\" resolution a detailed study of the nuclear kinematic structure of gas and stars in a representative sample of 40 local bona fide active galactic nucleus (AGN). KONA seeks to characterize the physical processes responsible for the coevolution of supermassive black holes and galaxies, principally inflows and outflows. With these IFU data of the nuclear regions of 40 Seyfert galaxies, the KONA survey will be able to study, for the fir"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1705.06678","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":"2026-05-18T00:16:56Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"VjbTJ+ea9Zw82ZKA3qY9mFt2bBaNpkFi6g+NlIINCx9tfJ2mBeHxXDnFZVTdPCx0f6h/CdPaVWbTNtvVqXJwCw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-01T21:12:28.145353Z"},"content_sha256":"a7408bb9b2231eecd1125201b62b0d6edb85ecb0d195b4a8c0dc3f05ed32382a","schema_version":"1.0","event_id":"sha256:a7408bb9b2231eecd1125201b62b0d6edb85ecb0d195b4a8c0dc3f05ed32382a"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/6XPQQGK2LFPIIJB2PXPFISDC4R/bundle.json","state_url":"https://pith.science/pith/6XPQQGK2LFPIIJB2PXPFISDC4R/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/6XPQQGK2LFPIIJB2PXPFISDC4R/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":"2026-06-01T21:12:28Z","links":{"resolver":"https://pith.science/pith/6XPQQGK2LFPIIJB2PXPFISDC4R","bundle":"https://pith.science/pith/6XPQQGK2LFPIIJB2PXPFISDC4R/bundle.json","state":"https://pith.science/pith/6XPQQGK2LFPIIJB2PXPFISDC4R/state.json","well_known_bundle":"https://pith.science/.well-known/pith/6XPQQGK2LFPIIJB2PXPFISDC4R/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2017:6XPQQGK2LFPIIJB2PXPFISDC4R","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":"c2766dcc1da626371fafb840ab25e5b480007cfbc3eaba6c0751055d65e9554c","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-05-18T16:29:19Z","title_canon_sha256":"12090fda16a26052bc718c2e5fc06497b750b2b37623dd1c87524d277df07f25"},"schema_version":"1.0","source":{"id":"1705.06678","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1705.06678","created_at":"2026-05-18T00:16:56Z"},{"alias_kind":"arxiv_version","alias_value":"1705.06678v2","created_at":"2026-05-18T00:16:56Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1705.06678","created_at":"2026-05-18T00:16:56Z"},{"alias_kind":"pith_short_12","alias_value":"6XPQQGK2LFPI","created_at":"2026-05-18T12:31:03Z"},{"alias_kind":"pith_short_16","alias_value":"6XPQQGK2LFPIIJB2","created_at":"2026-05-18T12:31:03Z"},{"alias_kind":"pith_short_8","alias_value":"6XPQQGK2","created_at":"2026-05-18T12:31:03Z"}],"graph_snapshots":[{"event_id":"sha256:a7408bb9b2231eecd1125201b62b0d6edb85ecb0d195b4a8c0dc3f05ed32382a","target":"graph","created_at":"2026-05-18T00:16:56Z","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 introduce the Keck Osiris Nearby AGN survey (KONA), a new adaptive optics-assisted integral-field spectroscopic survey of Seyfert galaxies. KONA permits at ~0.1\" resolution a detailed study of the nuclear kinematic structure of gas and stars in a representative sample of 40 local bona fide active galactic nucleus (AGN). KONA seeks to characterize the physical processes responsible for the coevolution of supermassive black holes and galaxies, principally inflows and outflows. With these IFU data of the nuclear regions of 40 Seyfert galaxies, the KONA survey will be able to study, for the fir","authors_text":"B. Davis, E. K. S. Hicks, F. M\\\"uller-S\\'anchez, M. Malkan, P. C. Yu, R. Davies, S. Shaver","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-05-18T16:29:19Z","title":"The Keck/OSIRIS Nearby AGN Survey (KONA) I. The Nuclear K-band Properties of Nearby AGN"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1705.06678","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":"sha256:16b1866b7ce1abbb03a1953b61dfe7ab5d72022658d1251de4368f8f42270c37","target":"record","created_at":"2026-05-18T00:16:56Z","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":"c2766dcc1da626371fafb840ab25e5b480007cfbc3eaba6c0751055d65e9554c","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2017-05-18T16:29:19Z","title_canon_sha256":"12090fda16a26052bc718c2e5fc06497b750b2b37623dd1c87524d277df07f25"},"schema_version":"1.0","source":{"id":"1705.06678","kind":"arxiv","version":2}},"canonical_sha256":"f5df08195a595e84243a7dde544862e47df741b3e6e6acc5ab6f66941403868b","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"f5df08195a595e84243a7dde544862e47df741b3e6e6acc5ab6f66941403868b","first_computed_at":"2026-05-18T00:16:56.428464Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:16:56.428464Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"iE5ce21MmkQ1jIswwDEzgcMYKaWgUd5IRNP6Pxyt0D6ajbeNA2WyONi0apMqpo5wTp+0fNJKz+G1AGcTRdg1Cw==","signature_status":"signed_v1","signed_at":"2026-05-18T00:16:56.429282Z","signed_message":"canonical_sha256_bytes"},"source_id":"1705.06678","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:16b1866b7ce1abbb03a1953b61dfe7ab5d72022658d1251de4368f8f42270c37","sha256:a7408bb9b2231eecd1125201b62b0d6edb85ecb0d195b4a8c0dc3f05ed32382a"],"state_sha256":"7b7d2357a115ceb864cb397ae97b665e6e72a9527536dba2fb31478940faa5be"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"QTcqRRayuBDFIGr/CUfUYn8KUnkFhYCR3ZBaKM2PNTzEVO2luiBHVo+fA8hooOzL2vMnNaZNdAkB0SRn/qr0CQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-01T21:12:28.147468Z","bundle_sha256":"6107b2dc08ddfb3f35adec703b4539c68930276ce554c1f4bd6ecf8addb2be73"}}