{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:G4224A2YT2JQ4GNIIXSJ4MCOSV","short_pith_number":"pith:G4224A2Y","schema_version":"1.0","canonical_sha256":"3735ae03589e930e19a845e49e304e957c7ea66bc9eeed3c61ea272345630253","source":{"kind":"arxiv","id":"2307.11407","version":2},"attestation_state":"computed","paper":{"title":"Line-of-sight structure of troughs identified in Subaru Hyper Suprime-Cam Year 3 weak lensing mass maps","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Atsushi J. Nishizawa, Ken Osato, Masamune Oguri, Rhythm Shimakawa, Takumi Shimasue","submitted_at":"2023-07-21T08:05:41Z","abstract_excerpt":"We perform the weak lensing mass mapping analysis to identify troughs, which are defined as local minima in the mass map. Since weak lensing probes projected matter along the line-of-sight, these troughs can be produced by single voids or multiple voids projected along the line-of-sight. To scrutinise the origins of the weak lensing troughs, we systematically investigate the line-of-sight structure of troughs selected from the latest Subaru Hyper Suprime-Cam (HSC) Year 3 weak lensing data covering $433.48 \\, \\mathrm{deg}^2$. From a curved sky mass map constructed with the HSC data, we identify"},"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":"2307.11407","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2023-07-21T08:05:41Z","cross_cats_sorted":[],"title_canon_sha256":"5c56c447c7e945ad961c468c491d92829b913ceb797c90c76ee89ca8c0bb3766","abstract_canon_sha256":"714359cd13c1d86b9c98d18960e964689289a6db5015e08f3cb6f7a33c6e1ba7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:13:24.210470Z","signature_b64":"Eorq8IMhDR+UABmaT+us/8n4I9JFufCcWG9Oju9PMWWyDh+1ey9kQxo8dpHwlW3c/HMcEVzCtTqZoxsJLj6uAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3735ae03589e930e19a845e49e304e957c7ea66bc9eeed3c61ea272345630253","last_reissued_at":"2026-07-05T07:13:24.209980Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:13:24.209980Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Line-of-sight structure of troughs identified in Subaru Hyper Suprime-Cam Year 3 weak lensing mass maps","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Atsushi J. Nishizawa, Ken Osato, Masamune Oguri, Rhythm Shimakawa, Takumi Shimasue","submitted_at":"2023-07-21T08:05:41Z","abstract_excerpt":"We perform the weak lensing mass mapping analysis to identify troughs, which are defined as local minima in the mass map. Since weak lensing probes projected matter along the line-of-sight, these troughs can be produced by single voids or multiple voids projected along the line-of-sight. To scrutinise the origins of the weak lensing troughs, we systematically investigate the line-of-sight structure of troughs selected from the latest Subaru Hyper Suprime-Cam (HSC) Year 3 weak lensing data covering $433.48 \\, \\mathrm{deg}^2$. From a curved sky mass map constructed with the HSC data, we identify"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2307.11407","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2307.11407/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2307.11407","created_at":"2026-07-05T07:13:24.210040+00:00"},{"alias_kind":"arxiv_version","alias_value":"2307.11407v2","created_at":"2026-07-05T07:13:24.210040+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2307.11407","created_at":"2026-07-05T07:13:24.210040+00:00"},{"alias_kind":"pith_short_12","alias_value":"G4224A2YT2JQ","created_at":"2026-07-05T07:13:24.210040+00:00"},{"alias_kind":"pith_short_16","alias_value":"G4224A2YT2JQ4GNI","created_at":"2026-07-05T07:13:24.210040+00:00"},{"alias_kind":"pith_short_8","alias_value":"G4224A2Y","created_at":"2026-07-05T07:13:24.210040+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.24939","citing_title":"Primordial Physics in the Nonlinear Universe: Revealing the oscillating halo bias from cosmological collider models","ref_index":27,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/G4224A2YT2JQ4GNIIXSJ4MCOSV","json":"https://pith.science/pith/G4224A2YT2JQ4GNIIXSJ4MCOSV.json","graph_json":"https://pith.science/api/pith-number/G4224A2YT2JQ4GNIIXSJ4MCOSV/graph.json","events_json":"https://pith.science/api/pith-number/G4224A2YT2JQ4GNIIXSJ4MCOSV/events.json","paper":"https://pith.science/paper/G4224A2Y"},"agent_actions":{"view_html":"https://pith.science/pith/G4224A2YT2JQ4GNIIXSJ4MCOSV","download_json":"https://pith.science/pith/G4224A2YT2JQ4GNIIXSJ4MCOSV.json","view_paper":"https://pith.science/paper/G4224A2Y","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2307.11407&json=true","fetch_graph":"https://pith.science/api/pith-number/G4224A2YT2JQ4GNIIXSJ4MCOSV/graph.json","fetch_events":"https://pith.science/api/pith-number/G4224A2YT2JQ4GNIIXSJ4MCOSV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/G4224A2YT2JQ4GNIIXSJ4MCOSV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/G4224A2YT2JQ4GNIIXSJ4MCOSV/action/storage_attestation","attest_author":"https://pith.science/pith/G4224A2YT2JQ4GNIIXSJ4MCOSV/action/author_attestation","sign_citation":"https://pith.science/pith/G4224A2YT2JQ4GNIIXSJ4MCOSV/action/citation_signature","submit_replication":"https://pith.science/pith/G4224A2YT2JQ4GNIIXSJ4MCOSV/action/replication_record"}},"created_at":"2026-07-05T07:13:24.210040+00:00","updated_at":"2026-07-05T07:13:24.210040+00:00"}