{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2017:YKKWRDMFFGUYCNASN7HPVMOTAG","short_pith_number":"pith:YKKWRDMF","canonical_record":{"source":{"id":"1701.01475","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2017-01-05T20:51:33Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"4d5f668aa8fc46b7e69c8ba59d1fda9d86dd4639154ce2cb37c38f5133577d5f","abstract_canon_sha256":"ac83f2e5db863f0b71c28eda5ac60092061bd50ae3791d41135ec07f0af052fd"},"schema_version":"1.0"},"canonical_sha256":"c295688d8529a98134126fcefab1d301ac7a3ce73c6706d64053333c37c863e2","source":{"kind":"arxiv","id":"1701.01475","version":3},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1701.01475","created_at":"2026-05-18T00:48:15Z"},{"alias_kind":"arxiv_version","alias_value":"1701.01475v3","created_at":"2026-05-18T00:48:15Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1701.01475","created_at":"2026-05-18T00:48:15Z"},{"alias_kind":"pith_short_12","alias_value":"YKKWRDMFFGUY","created_at":"2026-05-18T12:31:56Z"},{"alias_kind":"pith_short_16","alias_value":"YKKWRDMFFGUYCNAS","created_at":"2026-05-18T12:31:56Z"},{"alias_kind":"pith_short_8","alias_value":"YKKWRDMF","created_at":"2026-05-18T12:31:56Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2017:YKKWRDMFFGUYCNASN7HPVMOTAG","target":"record","payload":{"canonical_record":{"source":{"id":"1701.01475","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2017-01-05T20:51:33Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"4d5f668aa8fc46b7e69c8ba59d1fda9d86dd4639154ce2cb37c38f5133577d5f","abstract_canon_sha256":"ac83f2e5db863f0b71c28eda5ac60092061bd50ae3791d41135ec07f0af052fd"},"schema_version":"1.0"},"canonical_sha256":"c295688d8529a98134126fcefab1d301ac7a3ce73c6706d64053333c37c863e2","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:48:15.469761Z","signature_b64":"4bY59JwMpb7+Mko8XHuGscxEEIIxdZn339kytKn9nREm+mQ4U6g+lqGvsCCqkIKeSJGz6JhsU+dSxUVzFjXBDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c295688d8529a98134126fcefab1d301ac7a3ce73c6706d64053333c37c863e2","last_reissued_at":"2026-05-18T00:48:15.469031Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:48:15.469031Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1701.01475","source_version":3,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:48:15Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"3pjCAJfxpbRfG2Wg5I9oaz3zpU1qx1vjF8BF/kvLHMqE7sJrx3Pp2cwfhJWPTBZq67kkC2s7Rw1JEGPbf8dxBg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-19T10:15:34.950273Z"},"content_sha256":"e57b343ffbb42e7426914e86ccf2333a21cf51b17bebe990f160ad1611cca417","schema_version":"1.0","event_id":"sha256:e57b343ffbb42e7426914e86ccf2333a21cf51b17bebe990f160ad1611cca417"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2017:YKKWRDMFFGUYCNASN7HPVMOTAG","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Searching for giga-Jansky fast radio bursts from the Milky Way with a global array of low-cost radio receivers","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.IM","authors_text":"Abraham Loeb (Harvard University), Dan Maoz (Tel-Aviv University)","submitted_at":"2017-01-05T20:51:33Z","abstract_excerpt":"If fast radio bursts (FRBs) originate from galaxies at cosmological distances, then their all-sky rate implies that the Milky Way may host an FRB on average once every 30-1500 years. If FRBs repeat for decades or centuies, a local FRB could be active now. A typical Galactic FRB would produce a millisecond radio pulse with ~1 GHz flux density of ~3E10 Jy, comparable to the radio flux levels and frequencies of cellular communication devices (cell phones, Wi-Fi, GPS). We propose to search for Galactic FRBs using a global array of low-cost radio receivers. One possibility is to use the ~1GHz commu"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1701.01475","kind":"arxiv","version":3},"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":"2026-05-18T00:48:15Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"TsA0J2gI0cdnmLios/2M9V+3r5QyfjRX1fXi8cx7wF055YSwq8gjMH9TYssz4cCZJG3m90LY0i/LnmvOJ2CMBg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-19T10:15:34.950628Z"},"content_sha256":"71ea94181ef8bcc7a2f4a7530a1779f1fc25f5085c78f41e300676bdc3b44e79","schema_version":"1.0","event_id":"sha256:71ea94181ef8bcc7a2f4a7530a1779f1fc25f5085c78f41e300676bdc3b44e79"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/YKKWRDMFFGUYCNASN7HPVMOTAG/bundle.json","state_url":"https://pith.science/pith/YKKWRDMFFGUYCNASN7HPVMOTAG/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/YKKWRDMFFGUYCNASN7HPVMOTAG/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":"2026-05-19T10:15:34Z","links":{"resolver":"https://pith.science/pith/YKKWRDMFFGUYCNASN7HPVMOTAG","bundle":"https://pith.science/pith/YKKWRDMFFGUYCNASN7HPVMOTAG/bundle.json","state":"https://pith.science/pith/YKKWRDMFFGUYCNASN7HPVMOTAG/state.json","well_known_bundle":"https://pith.science/.well-known/pith/YKKWRDMFFGUYCNASN7HPVMOTAG/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2017:YKKWRDMFFGUYCNASN7HPVMOTAG","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":"ac83f2e5db863f0b71c28eda5ac60092061bd50ae3791d41135ec07f0af052fd","cross_cats_sorted":["astro-ph.CO"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2017-01-05T20:51:33Z","title_canon_sha256":"4d5f668aa8fc46b7e69c8ba59d1fda9d86dd4639154ce2cb37c38f5133577d5f"},"schema_version":"1.0","source":{"id":"1701.01475","kind":"arxiv","version":3}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1701.01475","created_at":"2026-05-18T00:48:15Z"},{"alias_kind":"arxiv_version","alias_value":"1701.01475v3","created_at":"2026-05-18T00:48:15Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1701.01475","created_at":"2026-05-18T00:48:15Z"},{"alias_kind":"pith_short_12","alias_value":"YKKWRDMFFGUY","created_at":"2026-05-18T12:31:56Z"},{"alias_kind":"pith_short_16","alias_value":"YKKWRDMFFGUYCNAS","created_at":"2026-05-18T12:31:56Z"},{"alias_kind":"pith_short_8","alias_value":"YKKWRDMF","created_at":"2026-05-18T12:31:56Z"}],"graph_snapshots":[{"event_id":"sha256:71ea94181ef8bcc7a2f4a7530a1779f1fc25f5085c78f41e300676bdc3b44e79","target":"graph","created_at":"2026-05-18T00:48:15Z","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":"If fast radio bursts (FRBs) originate from galaxies at cosmological distances, then their all-sky rate implies that the Milky Way may host an FRB on average once every 30-1500 years. If FRBs repeat for decades or centuies, a local FRB could be active now. A typical Galactic FRB would produce a millisecond radio pulse with ~1 GHz flux density of ~3E10 Jy, comparable to the radio flux levels and frequencies of cellular communication devices (cell phones, Wi-Fi, GPS). We propose to search for Galactic FRBs using a global array of low-cost radio receivers. One possibility is to use the ~1GHz commu","authors_text":"Abraham Loeb (Harvard University), Dan Maoz (Tel-Aviv University)","cross_cats":["astro-ph.CO"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2017-01-05T20:51:33Z","title":"Searching for giga-Jansky fast radio bursts from the Milky Way with a global array of low-cost radio receivers"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1701.01475","kind":"arxiv","version":3},"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:e57b343ffbb42e7426914e86ccf2333a21cf51b17bebe990f160ad1611cca417","target":"record","created_at":"2026-05-18T00:48:15Z","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":"ac83f2e5db863f0b71c28eda5ac60092061bd50ae3791d41135ec07f0af052fd","cross_cats_sorted":["astro-ph.CO"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2017-01-05T20:51:33Z","title_canon_sha256":"4d5f668aa8fc46b7e69c8ba59d1fda9d86dd4639154ce2cb37c38f5133577d5f"},"schema_version":"1.0","source":{"id":"1701.01475","kind":"arxiv","version":3}},"canonical_sha256":"c295688d8529a98134126fcefab1d301ac7a3ce73c6706d64053333c37c863e2","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"c295688d8529a98134126fcefab1d301ac7a3ce73c6706d64053333c37c863e2","first_computed_at":"2026-05-18T00:48:15.469031Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:48:15.469031Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"4bY59JwMpb7+Mko8XHuGscxEEIIxdZn339kytKn9nREm+mQ4U6g+lqGvsCCqkIKeSJGz6JhsU+dSxUVzFjXBDg==","signature_status":"signed_v1","signed_at":"2026-05-18T00:48:15.469761Z","signed_message":"canonical_sha256_bytes"},"source_id":"1701.01475","source_kind":"arxiv","source_version":3}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:e57b343ffbb42e7426914e86ccf2333a21cf51b17bebe990f160ad1611cca417","sha256:71ea94181ef8bcc7a2f4a7530a1779f1fc25f5085c78f41e300676bdc3b44e79"],"state_sha256":"9f36f8ebb505eb8ff74b42ecfa255416e3d9ff2b970e3cd24683866c6cd04b6f"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Gehp7GSX5gxbPBIz+FwV6YpkX0WW6u2LV3KfGeLprevyRgx1MHVA/Kov20ieONH4zXUHJVWONvyhwdFawrOBDw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-19T10:15:34.952144Z","bundle_sha256":"289c026fe3ae1bb73d3aa2430a7a7eee6d640cf1fcdfc8733d9908c6fb7b415a"}}