{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2011:GVALBV34ECIRHZHO5GZVT7A7YX","short_pith_number":"pith:GVALBV34","canonical_record":{"source":{"id":"1101.5637","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-01-28T22:10:05Z","cross_cats_sorted":[],"title_canon_sha256":"12ed3969c69bc1f5ce3cee7c802a7c8d0d0da3c138695bc47d7440575c038fe2","abstract_canon_sha256":"cccfa7d90e11bbeb923831fae640eb685e73641c802b34e9d5cae870cf62dc12"},"schema_version":"1.0"},"canonical_sha256":"3540b0d77c209113e4eee9b359fc1fc5fba24d5f2ee8b4dd97cafee4e3413ddd","source":{"kind":"arxiv","id":"1101.5637","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1101.5637","created_at":"2026-05-18T02:03:20Z"},{"alias_kind":"arxiv_version","alias_value":"1101.5637v1","created_at":"2026-05-18T02:03:20Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1101.5637","created_at":"2026-05-18T02:03:20Z"},{"alias_kind":"pith_short_12","alias_value":"GVALBV34ECIR","created_at":"2026-05-18T12:26:30Z"},{"alias_kind":"pith_short_16","alias_value":"GVALBV34ECIRHZHO","created_at":"2026-05-18T12:26:30Z"},{"alias_kind":"pith_short_8","alias_value":"GVALBV34","created_at":"2026-05-18T12:26:30Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2011:GVALBV34ECIRHZHO5GZVT7A7YX","target":"record","payload":{"canonical_record":{"source":{"id":"1101.5637","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-01-28T22:10:05Z","cross_cats_sorted":[],"title_canon_sha256":"12ed3969c69bc1f5ce3cee7c802a7c8d0d0da3c138695bc47d7440575c038fe2","abstract_canon_sha256":"cccfa7d90e11bbeb923831fae640eb685e73641c802b34e9d5cae870cf62dc12"},"schema_version":"1.0"},"canonical_sha256":"3540b0d77c209113e4eee9b359fc1fc5fba24d5f2ee8b4dd97cafee4e3413ddd","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:03:20.663027Z","signature_b64":"A4LuDN29s5vdu2IYn17WEoY9jbyQerSzPZaCtPmlCX2593gZI/I6fiDz95D8oenHutOKtA0UYhbYYNZ5r8AsCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3540b0d77c209113e4eee9b359fc1fc5fba24d5f2ee8b4dd97cafee4e3413ddd","last_reissued_at":"2026-05-18T02:03:20.662548Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:03:20.662548Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1101.5637","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":"2026-05-18T02:03:20Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"IlZEOGNF+lROr9+UdbbjoUYNHVgE6LCVEwo0+lQvkHbYr3HV59zOIMQBZuQ3Vmzus6fkwlHZy2yudrb11vPrBg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-18T18:53:32.587045Z"},"content_sha256":"288c0e8d1423e1d2a9607491a5e25b6a8117f029ac41e17798a83efae7b8d7ad","schema_version":"1.0","event_id":"sha256:288c0e8d1423e1d2a9607491a5e25b6a8117f029ac41e17798a83efae7b8d7ad"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2011:GVALBV34ECIRHZHO5GZVT7A7YX","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Multiwavelength Studies of Rotating Radio Transients","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.SR","authors_text":"Andrew Lyne, Evan Keane, Joshua Miller, Kosmas Lazaridis, Maura McLaughlin, Michael Kramer, Nanda Rea, Richard Manchester","submitted_at":"2011-01-28T22:10:05Z","abstract_excerpt":"We describe our studies of the radio and high-energy properties of Rotating Radio Transients (RRATs). We find that the radio pulse intensity distributions are log-normal, with power-law tails evident in two cases. For the three RRATs with coverage over a wide range of frequency, the mean spectral index is -1.7\\pm0.1, roughly in the range of normal pulsars. We do not observe anomalous magnetar-like spectra for any RRATs. Our 94-ks XMM-Newton observation of the high magnetic field RRAT J1819-1458 reveals a blackbody spectrum (kT ~130 eV) with an unusual absorption feature at ~1 keV. We find no e"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1101.5637","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":"2026-05-18T02:03:20Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"00srI0lWT+pMcqEnxT4SgoOasdq3btJiru012Lfs3IHVWgPkuEfjAUEXPLpnUyTykmKJGCpBsKPdxbfSSGMFBQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-18T18:53:32.587603Z"},"content_sha256":"c572f3d808d74642975cf7deac1ae3c637aeb07b628f555c26612fc603ff72b8","schema_version":"1.0","event_id":"sha256:c572f3d808d74642975cf7deac1ae3c637aeb07b628f555c26612fc603ff72b8"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/GVALBV34ECIRHZHO5GZVT7A7YX/bundle.json","state_url":"https://pith.science/pith/GVALBV34ECIRHZHO5GZVT7A7YX/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/GVALBV34ECIRHZHO5GZVT7A7YX/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":"2026-05-18T18:53:32Z","links":{"resolver":"https://pith.science/pith/GVALBV34ECIRHZHO5GZVT7A7YX","bundle":"https://pith.science/pith/GVALBV34ECIRHZHO5GZVT7A7YX/bundle.json","state":"https://pith.science/pith/GVALBV34ECIRHZHO5GZVT7A7YX/state.json","well_known_bundle":"https://pith.science/.well-known/pith/GVALBV34ECIRHZHO5GZVT7A7YX/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2011:GVALBV34ECIRHZHO5GZVT7A7YX","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":"cccfa7d90e11bbeb923831fae640eb685e73641c802b34e9d5cae870cf62dc12","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-01-28T22:10:05Z","title_canon_sha256":"12ed3969c69bc1f5ce3cee7c802a7c8d0d0da3c138695bc47d7440575c038fe2"},"schema_version":"1.0","source":{"id":"1101.5637","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1101.5637","created_at":"2026-05-18T02:03:20Z"},{"alias_kind":"arxiv_version","alias_value":"1101.5637v1","created_at":"2026-05-18T02:03:20Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1101.5637","created_at":"2026-05-18T02:03:20Z"},{"alias_kind":"pith_short_12","alias_value":"GVALBV34ECIR","created_at":"2026-05-18T12:26:30Z"},{"alias_kind":"pith_short_16","alias_value":"GVALBV34ECIRHZHO","created_at":"2026-05-18T12:26:30Z"},{"alias_kind":"pith_short_8","alias_value":"GVALBV34","created_at":"2026-05-18T12:26:30Z"}],"graph_snapshots":[{"event_id":"sha256:c572f3d808d74642975cf7deac1ae3c637aeb07b628f555c26612fc603ff72b8","target":"graph","created_at":"2026-05-18T02:03:20Z","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 describe our studies of the radio and high-energy properties of Rotating Radio Transients (RRATs). We find that the radio pulse intensity distributions are log-normal, with power-law tails evident in two cases. For the three RRATs with coverage over a wide range of frequency, the mean spectral index is -1.7\\pm0.1, roughly in the range of normal pulsars. We do not observe anomalous magnetar-like spectra for any RRATs. Our 94-ks XMM-Newton observation of the high magnetic field RRAT J1819-1458 reveals a blackbody spectrum (kT ~130 eV) with an unusual absorption feature at ~1 keV. We find no e","authors_text":"Andrew Lyne, Evan Keane, Joshua Miller, Kosmas Lazaridis, Maura McLaughlin, Michael Kramer, Nanda Rea, Richard Manchester","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-01-28T22:10:05Z","title":"Multiwavelength Studies of Rotating Radio Transients"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1101.5637","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":"sha256:288c0e8d1423e1d2a9607491a5e25b6a8117f029ac41e17798a83efae7b8d7ad","target":"record","created_at":"2026-05-18T02:03:20Z","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":"cccfa7d90e11bbeb923831fae640eb685e73641c802b34e9d5cae870cf62dc12","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-01-28T22:10:05Z","title_canon_sha256":"12ed3969c69bc1f5ce3cee7c802a7c8d0d0da3c138695bc47d7440575c038fe2"},"schema_version":"1.0","source":{"id":"1101.5637","kind":"arxiv","version":1}},"canonical_sha256":"3540b0d77c209113e4eee9b359fc1fc5fba24d5f2ee8b4dd97cafee4e3413ddd","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"3540b0d77c209113e4eee9b359fc1fc5fba24d5f2ee8b4dd97cafee4e3413ddd","first_computed_at":"2026-05-18T02:03:20.662548Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:03:20.662548Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"A4LuDN29s5vdu2IYn17WEoY9jbyQerSzPZaCtPmlCX2593gZI/I6fiDz95D8oenHutOKtA0UYhbYYNZ5r8AsCg==","signature_status":"signed_v1","signed_at":"2026-05-18T02:03:20.663027Z","signed_message":"canonical_sha256_bytes"},"source_id":"1101.5637","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:288c0e8d1423e1d2a9607491a5e25b6a8117f029ac41e17798a83efae7b8d7ad","sha256:c572f3d808d74642975cf7deac1ae3c637aeb07b628f555c26612fc603ff72b8"],"state_sha256":"79a82223f69f35e9ae0667b77834217919b7ce605ef4f2d493e7c4798a7ab0cb"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"yvT73gxIU1dpZdJiAEyhjd7M/DyU2YUrv+T5prpGGkBU2mo0c0aHmfjUcDxV2ZbMKXg6zVqRpvZUqyOQoVMXDw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-18T18:53:32.589387Z","bundle_sha256":"a7a55cc1f26fea0137818b377c92bef8733a6a8da8fd4b99e68137d5e235cc1a"}}