{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2018:PAPYDP5EFPZUHRIFF2XO6JQXUT","short_pith_number":"pith:PAPYDP5E","canonical_record":{"source":{"id":"1809.01206","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2018-09-04T19:09:42Z","cross_cats_sorted":[],"title_canon_sha256":"3847d9623ac4a2c43c131aff7292cfaa07a154d3bfd40ab20df3e27b56307afb","abstract_canon_sha256":"3a5e66d0e6ffb362b66ff97f304302867b8143cdc479e8a72aede1af357efc0b"},"schema_version":"1.0"},"canonical_sha256":"781f81bfa42bf343c5052eaeef2617a4db7805c7088464ce627577c2021f107a","source":{"kind":"arxiv","id":"1809.01206","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1809.01206","created_at":"2026-05-18T00:00:45Z"},{"alias_kind":"arxiv_version","alias_value":"1809.01206v1","created_at":"2026-05-18T00:00:45Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1809.01206","created_at":"2026-05-18T00:00:45Z"},{"alias_kind":"pith_short_12","alias_value":"PAPYDP5EFPZU","created_at":"2026-05-18T12:32:43Z"},{"alias_kind":"pith_short_16","alias_value":"PAPYDP5EFPZUHRIF","created_at":"2026-05-18T12:32:43Z"},{"alias_kind":"pith_short_8","alias_value":"PAPYDP5E","created_at":"2026-05-18T12:32:43Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2018:PAPYDP5EFPZUHRIFF2XO6JQXUT","target":"record","payload":{"canonical_record":{"source":{"id":"1809.01206","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2018-09-04T19:09:42Z","cross_cats_sorted":[],"title_canon_sha256":"3847d9623ac4a2c43c131aff7292cfaa07a154d3bfd40ab20df3e27b56307afb","abstract_canon_sha256":"3a5e66d0e6ffb362b66ff97f304302867b8143cdc479e8a72aede1af357efc0b"},"schema_version":"1.0"},"canonical_sha256":"781f81bfa42bf343c5052eaeef2617a4db7805c7088464ce627577c2021f107a","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:00:45.690992Z","signature_b64":"CT3z0e4zdY9+DNjLIHybU/q+UE7xITufAI0cyhwtEvZ0TfhVKDMseZYFiG9IlOLwmP6/HnVeHlG+ie1cRjtyAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"781f81bfa42bf343c5052eaeef2617a4db7805c7088464ce627577c2021f107a","last_reissued_at":"2026-05-18T00:00:45.690567Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:00:45.690567Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1809.01206","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":"2026-05-18T00:00:45Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"S4NiWNjRXtWyV+8cYOxHCTRbotNJ5gJpAJOO78AxNvfk16XOxyhUd+oAp6XB8w66hS4xAffq/SLqPrWVO/3iBw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-22T11:51:40.431532Z"},"content_sha256":"422fd721995f994524bdeb06927b0f56fde3719dd84e5a689198c22cd96d7b6c","schema_version":"1.0","event_id":"sha256:422fd721995f994524bdeb06927b0f56fde3719dd84e5a689198c22cd96d7b6c"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2018:PAPYDP5EFPZUHRIFF2XO6JQXUT","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"MAGNUM survey: A MUSE-Chandra resolved view on ionized outflows and photoionization in the Seyfert galaxy NGC 1365","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Bongiorno, A. Capetti, A. Gallazzi, A. Marconi, B. Balmaverde, C. Cicone, C. Feruglio, E. Nardini, E. Piconcelli, E. Sani, F. Fiore, F. La Franca, F. Mannucci, G. Cresci, G. Risaliti, G. Venturi, K. Matsuoka, M. Brusa, M. Mingozzi, M. Perna, P. Tozzi, R. Maiolino, S. Carniani, S. Ciroi, S. Zibetti, T. Nagao, V. Mainieri","submitted_at":"2018-09-04T19:09:42Z","abstract_excerpt":"Ionized outflows, revealed by broad asymmetric wings of the [OIII] line, are commonly observed in AGN but the low intrinsic spatial resolution of observations has generally prevented a detailed characterization of their properties. The MAGNUM survey aims at overcoming these limitations by focusing on the nearest AGN, including NGC 1365, a nearby Seyfert galaxy (D~17 Mpc), hosting a low-luminosity AGN (Lbol ~ 2x10^43 erg/s). We want to obtain a detailed picture of the ionized gas in the central ~5 kpc of NGC 1365 in terms of physical properties, kinematics, and ionization mechanisms. We also ai"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1809.01206","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":"2026-05-18T00:00:45Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"ddvzejQMauACtx/+/hzEHZ6QlKZ/dW+E76h87FTD/8xuQEghZ0Ck0SykG6SUkJIGyrF2vjxYgTOHj3Z3sKzIBA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-22T11:51:40.432205Z"},"content_sha256":"13497672237a4f8bafd1881026b9808cdef2ff2550ac7b225bd7b7cf80949bef","schema_version":"1.0","event_id":"sha256:13497672237a4f8bafd1881026b9808cdef2ff2550ac7b225bd7b7cf80949bef"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/PAPYDP5EFPZUHRIFF2XO6JQXUT/bundle.json","state_url":"https://pith.science/pith/PAPYDP5EFPZUHRIFF2XO6JQXUT/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/PAPYDP5EFPZUHRIFF2XO6JQXUT/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":"2026-05-22T11:51:40Z","links":{"resolver":"https://pith.science/pith/PAPYDP5EFPZUHRIFF2XO6JQXUT","bundle":"https://pith.science/pith/PAPYDP5EFPZUHRIFF2XO6JQXUT/bundle.json","state":"https://pith.science/pith/PAPYDP5EFPZUHRIFF2XO6JQXUT/state.json","well_known_bundle":"https://pith.science/.well-known/pith/PAPYDP5EFPZUHRIFF2XO6JQXUT/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2018:PAPYDP5EFPZUHRIFF2XO6JQXUT","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":"3a5e66d0e6ffb362b66ff97f304302867b8143cdc479e8a72aede1af357efc0b","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2018-09-04T19:09:42Z","title_canon_sha256":"3847d9623ac4a2c43c131aff7292cfaa07a154d3bfd40ab20df3e27b56307afb"},"schema_version":"1.0","source":{"id":"1809.01206","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1809.01206","created_at":"2026-05-18T00:00:45Z"},{"alias_kind":"arxiv_version","alias_value":"1809.01206v1","created_at":"2026-05-18T00:00:45Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1809.01206","created_at":"2026-05-18T00:00:45Z"},{"alias_kind":"pith_short_12","alias_value":"PAPYDP5EFPZU","created_at":"2026-05-18T12:32:43Z"},{"alias_kind":"pith_short_16","alias_value":"PAPYDP5EFPZUHRIF","created_at":"2026-05-18T12:32:43Z"},{"alias_kind":"pith_short_8","alias_value":"PAPYDP5E","created_at":"2026-05-18T12:32:43Z"}],"graph_snapshots":[{"event_id":"sha256:13497672237a4f8bafd1881026b9808cdef2ff2550ac7b225bd7b7cf80949bef","target":"graph","created_at":"2026-05-18T00:00:45Z","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":"Ionized outflows, revealed by broad asymmetric wings of the [OIII] line, are commonly observed in AGN but the low intrinsic spatial resolution of observations has generally prevented a detailed characterization of their properties. The MAGNUM survey aims at overcoming these limitations by focusing on the nearest AGN, including NGC 1365, a nearby Seyfert galaxy (D~17 Mpc), hosting a low-luminosity AGN (Lbol ~ 2x10^43 erg/s). We want to obtain a detailed picture of the ionized gas in the central ~5 kpc of NGC 1365 in terms of physical properties, kinematics, and ionization mechanisms. We also ai","authors_text":"A. Bongiorno, A. Capetti, A. Gallazzi, A. Marconi, B. Balmaverde, C. Cicone, C. Feruglio, E. Nardini, E. Piconcelli, E. Sani, F. Fiore, F. La Franca, F. Mannucci, G. Cresci, G. Risaliti, G. Venturi, K. Matsuoka, M. Brusa, M. Mingozzi, M. Perna, P. Tozzi, R. Maiolino, S. Carniani, S. Ciroi, S. Zibetti, T. Nagao, V. Mainieri","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2018-09-04T19:09:42Z","title":"MAGNUM survey: A MUSE-Chandra resolved view on ionized outflows and photoionization in the Seyfert galaxy NGC 1365"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1809.01206","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":"sha256:422fd721995f994524bdeb06927b0f56fde3719dd84e5a689198c22cd96d7b6c","target":"record","created_at":"2026-05-18T00:00:45Z","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":"3a5e66d0e6ffb362b66ff97f304302867b8143cdc479e8a72aede1af357efc0b","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2018-09-04T19:09:42Z","title_canon_sha256":"3847d9623ac4a2c43c131aff7292cfaa07a154d3bfd40ab20df3e27b56307afb"},"schema_version":"1.0","source":{"id":"1809.01206","kind":"arxiv","version":1}},"canonical_sha256":"781f81bfa42bf343c5052eaeef2617a4db7805c7088464ce627577c2021f107a","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"781f81bfa42bf343c5052eaeef2617a4db7805c7088464ce627577c2021f107a","first_computed_at":"2026-05-18T00:00:45.690567Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:00:45.690567Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"CT3z0e4zdY9+DNjLIHybU/q+UE7xITufAI0cyhwtEvZ0TfhVKDMseZYFiG9IlOLwmP6/HnVeHlG+ie1cRjtyAQ==","signature_status":"signed_v1","signed_at":"2026-05-18T00:00:45.690992Z","signed_message":"canonical_sha256_bytes"},"source_id":"1809.01206","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:422fd721995f994524bdeb06927b0f56fde3719dd84e5a689198c22cd96d7b6c","sha256:13497672237a4f8bafd1881026b9808cdef2ff2550ac7b225bd7b7cf80949bef"],"state_sha256":"567712e9f475bb0c199cf37286921a676efd0fce77b05eafc6b7599d8e9ecb0a"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"8JRtNcwhQ5VoP7AIGn0XGA8O57DurJoWU0L5gLa6XXz5aCZLuar7AnBOVhelT0vz4iWNMFkbuCnmI4NPKJavAw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-22T11:51:40.435765Z","bundle_sha256":"ed0b2bbd2506a19463454cc67d3aae456b5ae4011d7927e437e81ae557dea1a9"}}