{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:W5VE4VND6UZR4ON5OH5URIPAFE","short_pith_number":"pith:W5VE4VND","schema_version":"1.0","canonical_sha256":"b76a4e55a3f5331e39bd71fb48a1e02935f1633d84068f7f7c31093033764219","source":{"kind":"arxiv","id":"1711.04764","version":1},"attestation_state":"computed","paper":{"title":"Nanolensed fast Radio Bursts","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"David Eichler","submitted_at":"2017-11-13T19:00:00Z","abstract_excerpt":"It is suggested that fast radio bursts can probe gravitational lensing by clumpy dark matter objects that range in mass from $10^{-3}M_{\\odot}$ to $10^2 M_{\\odot}$. They may provide a more sensitive probe than observations of lensing of objects in the Magellanic Clouds, and could find or rule out clumpy dark matter with an extended mass spectrum."},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1711.04764","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-11-13T19:00:00Z","cross_cats_sorted":[],"title_canon_sha256":"a14c6209d2c92bb88bc1a89c4746842451cb98ccdd1728f7dd2028f52e314703","abstract_canon_sha256":"d933360e5c5c080eddea4d2a93a7c47557d8d56e06bd1405bbf556a8a38b49d4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:28:10.336103Z","signature_b64":"O3Ocbmqen0Wxg6b8z2pHRNI4yRk1lamQY+mSYYwg4UeRH3nf1UOFmWnJbHmPRP3W3U8qHULHTQJdxWDmYxzWDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b76a4e55a3f5331e39bd71fb48a1e02935f1633d84068f7f7c31093033764219","last_reissued_at":"2026-05-18T00:28:10.335367Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:28:10.335367Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Nanolensed fast Radio Bursts","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"David Eichler","submitted_at":"2017-11-13T19:00:00Z","abstract_excerpt":"It is suggested that fast radio bursts can probe gravitational lensing by clumpy dark matter objects that range in mass from $10^{-3}M_{\\odot}$ to $10^2 M_{\\odot}$. They may provide a more sensitive probe than observations of lensing of objects in the Magellanic Clouds, and could find or rule out clumpy dark matter with an extended mass spectrum."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.04764","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1711.04764","created_at":"2026-05-18T00:28:10.335465+00:00"},{"alias_kind":"arxiv_version","alias_value":"1711.04764v1","created_at":"2026-05-18T00:28:10.335465+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1711.04764","created_at":"2026-05-18T00:28:10.335465+00:00"},{"alias_kind":"pith_short_12","alias_value":"W5VE4VND6UZR","created_at":"2026-05-18T12:31:53.515858+00:00"},{"alias_kind":"pith_short_16","alias_value":"W5VE4VND6UZR4ON5","created_at":"2026-05-18T12:31:53.515858+00:00"},{"alias_kind":"pith_short_8","alias_value":"W5VE4VND","created_at":"2026-05-18T12:31:53.515858+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2407.04097","citing_title":"Simulating FRB Morphologies and Coherent Phase Correlation Signatures from Multi-Plane Astrophysical Lensing","ref_index":15,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/W5VE4VND6UZR4ON5OH5URIPAFE","json":"https://pith.science/pith/W5VE4VND6UZR4ON5OH5URIPAFE.json","graph_json":"https://pith.science/api/pith-number/W5VE4VND6UZR4ON5OH5URIPAFE/graph.json","events_json":"https://pith.science/api/pith-number/W5VE4VND6UZR4ON5OH5URIPAFE/events.json","paper":"https://pith.science/paper/W5VE4VND"},"agent_actions":{"view_html":"https://pith.science/pith/W5VE4VND6UZR4ON5OH5URIPAFE","download_json":"https://pith.science/pith/W5VE4VND6UZR4ON5OH5URIPAFE.json","view_paper":"https://pith.science/paper/W5VE4VND","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1711.04764&json=true","fetch_graph":"https://pith.science/api/pith-number/W5VE4VND6UZR4ON5OH5URIPAFE/graph.json","fetch_events":"https://pith.science/api/pith-number/W5VE4VND6UZR4ON5OH5URIPAFE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/W5VE4VND6UZR4ON5OH5URIPAFE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/W5VE4VND6UZR4ON5OH5URIPAFE/action/storage_attestation","attest_author":"https://pith.science/pith/W5VE4VND6UZR4ON5OH5URIPAFE/action/author_attestation","sign_citation":"https://pith.science/pith/W5VE4VND6UZR4ON5OH5URIPAFE/action/citation_signature","submit_replication":"https://pith.science/pith/W5VE4VND6UZR4ON5OH5URIPAFE/action/replication_record"}},"created_at":"2026-05-18T00:28:10.335465+00:00","updated_at":"2026-05-18T00:28:10.335465+00:00"}