{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:GGHP6XBEP56MZHIYRJ7RRSVLSH","short_pith_number":"pith:GGHP6XBE","schema_version":"1.0","canonical_sha256":"318eff5c247f7ccc9d188a7f18caab91deb0a1ddc57ab3064f1840a41faf593b","source":{"kind":"arxiv","id":"2506.04570","version":1},"attestation_state":"computed","paper":{"title":"RIDEN pilot survey: broad-band selection of candidate quasars with extended Lyman-$\\alpha$ nebulae using CLAUDS-HSC-SSP-DUNES$^2$ joint data","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Guillaume Desprez, Haruka Kusakabe, Marcin Sawicki, Rhythm Shimakawa, Rieko Momose, Satoshi Kikuta, Stephen Gwyn, Yongming Liang","submitted_at":"2025-06-05T02:44:20Z","abstract_excerpt":"The Vera C. Rubin Observatory will conduct the Legacy Survey of Space and Time (LSST), delivering deep, multi-band ($ugrizy$) imaging data across 18,000 square degrees over the next decade. Before this ultra-wide-field survey, we constructed a broad-band Ly$\\alpha$ imaging toward 483 SDSS/BOSS quasars at $z=$ 1.9-3.0, using deep, wide-field ultraviolet to near-infrared ($u$-to-$K$) data from the Hyper Suprime-Cam Subaru Strategic Survey (HSC-SSP), the CFHT Large Area U-band Deep Survey (CLAUDS), the Deep UKIRT Near-Infrared Steward Survey (DUNES$^2$), and additional public data covering 13 squ"},"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":"2506.04570","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2025-06-05T02:44:20Z","cross_cats_sorted":[],"title_canon_sha256":"dd21ebc4d3643191fe769d5719efe67a3be13d7e7451983eedb426666ec669b6","abstract_canon_sha256":"b79bba74774e39c63007fdf99d57bce760735cea951df72c9eea71f27de22978"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:16:16.856190Z","signature_b64":"T1lHLB0eB+tEpabNk3j3YSGCvR3GtSZ3F7uD56FScTfJ4tHtVRa7+BpdMNVJIY2fM76a+DAGlBC+/ui1IV8dBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"318eff5c247f7ccc9d188a7f18caab91deb0a1ddc57ab3064f1840a41faf593b","last_reissued_at":"2026-07-05T11:16:16.855706Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:16:16.855706Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"RIDEN pilot survey: broad-band selection of candidate quasars with extended Lyman-$\\alpha$ nebulae using CLAUDS-HSC-SSP-DUNES$^2$ joint data","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Guillaume Desprez, Haruka Kusakabe, Marcin Sawicki, Rhythm Shimakawa, Rieko Momose, Satoshi Kikuta, Stephen Gwyn, Yongming Liang","submitted_at":"2025-06-05T02:44:20Z","abstract_excerpt":"The Vera C. Rubin Observatory will conduct the Legacy Survey of Space and Time (LSST), delivering deep, multi-band ($ugrizy$) imaging data across 18,000 square degrees over the next decade. Before this ultra-wide-field survey, we constructed a broad-band Ly$\\alpha$ imaging toward 483 SDSS/BOSS quasars at $z=$ 1.9-3.0, using deep, wide-field ultraviolet to near-infrared ($u$-to-$K$) data from the Hyper Suprime-Cam Subaru Strategic Survey (HSC-SSP), the CFHT Large Area U-band Deep Survey (CLAUDS), the Deep UKIRT Near-Infrared Steward Survey (DUNES$^2$), and additional public data covering 13 squ"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2506.04570","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2506.04570/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":"2506.04570","created_at":"2026-07-05T11:16:16.855772+00:00"},{"alias_kind":"arxiv_version","alias_value":"2506.04570v1","created_at":"2026-07-05T11:16:16.855772+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2506.04570","created_at":"2026-07-05T11:16:16.855772+00:00"},{"alias_kind":"pith_short_12","alias_value":"GGHP6XBEP56M","created_at":"2026-07-05T11:16:16.855772+00:00"},{"alias_kind":"pith_short_16","alias_value":"GGHP6XBEP56MZHIY","created_at":"2026-07-05T11:16:16.855772+00:00"},{"alias_kind":"pith_short_8","alias_value":"GGHP6XBE","created_at":"2026-07-05T11:16:16.855772+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/GGHP6XBEP56MZHIYRJ7RRSVLSH","json":"https://pith.science/pith/GGHP6XBEP56MZHIYRJ7RRSVLSH.json","graph_json":"https://pith.science/api/pith-number/GGHP6XBEP56MZHIYRJ7RRSVLSH/graph.json","events_json":"https://pith.science/api/pith-number/GGHP6XBEP56MZHIYRJ7RRSVLSH/events.json","paper":"https://pith.science/paper/GGHP6XBE"},"agent_actions":{"view_html":"https://pith.science/pith/GGHP6XBEP56MZHIYRJ7RRSVLSH","download_json":"https://pith.science/pith/GGHP6XBEP56MZHIYRJ7RRSVLSH.json","view_paper":"https://pith.science/paper/GGHP6XBE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2506.04570&json=true","fetch_graph":"https://pith.science/api/pith-number/GGHP6XBEP56MZHIYRJ7RRSVLSH/graph.json","fetch_events":"https://pith.science/api/pith-number/GGHP6XBEP56MZHIYRJ7RRSVLSH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GGHP6XBEP56MZHIYRJ7RRSVLSH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GGHP6XBEP56MZHIYRJ7RRSVLSH/action/storage_attestation","attest_author":"https://pith.science/pith/GGHP6XBEP56MZHIYRJ7RRSVLSH/action/author_attestation","sign_citation":"https://pith.science/pith/GGHP6XBEP56MZHIYRJ7RRSVLSH/action/citation_signature","submit_replication":"https://pith.science/pith/GGHP6XBEP56MZHIYRJ7RRSVLSH/action/replication_record"}},"created_at":"2026-07-05T11:16:16.855772+00:00","updated_at":"2026-07-05T11:16:16.855772+00:00"}