{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:OOE4WM37WNPYSTWZCTNB7N4GWV","short_pith_number":"pith:OOE4WM37","schema_version":"1.0","canonical_sha256":"7389cb337fb35f894ed914da1fb786b54712406ff7a60de88ebbae3e067b57de","source":{"kind":"arxiv","id":"1604.08215","version":2},"attestation_state":"computed","paper":{"title":"Galaxy-scale gravitational lens candidates from the Hyper Suprime-Cam imaging survey and the Galaxy And Mass Assembly spectroscopic survey","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Anupreeta More, Atsushi J. Nishizawa, Bau-ching Hsieh, Hitoshi Murayama, James H. H. Chan, Jean Coupon, Masamune Oguri, Paul Price, Philip J. Tait, Satoshi Miyazaki, Sherry H. Suyu, Shiang-Yu Wang, Tsuyoshi Terai, Tzihong Chiueh, Yousuke Utsumi, Yutaka Komiyama","submitted_at":"2016-04-27T20:00:10Z","abstract_excerpt":"We present a list of galaxy-scale lens candidates including a highly probable interacting galaxy-scale lens in the Hyper Suprime-Cam (HSC) imaging survey. We combine HSC imaging with the blended-spectra catalog from the Galaxy And Mass Assembly (GAMA) survey to identify lens candidates, and use lens mass modeling to confirm the candidates. We find 46 matches between the HSC S14A_0b imaging data release and the GAMA catalog. Ten of them are probable lens systems according to their morphology and redshifts. There is one system with an interacting galaxy pair, HSC J084928+000949, that has a valid"},"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":"1604.08215","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-04-27T20:00:10Z","cross_cats_sorted":[],"title_canon_sha256":"79151c26b7f2392f55d78f177c29e8060ff8acfdde40736d3cdcce04cc679ce9","abstract_canon_sha256":"5bb1684efffff3c66595c496af6174fddf669fe0f4b8fa50cb4ab021fb3a2e24"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:45:16.141588Z","signature_b64":"Lf93LnvnCUmGRw4pcNszDe8tuxEHM38xS2OHPoxB0MGn/lYt6TVsA2Yw5fOxkZOXme41Aax6tdWTb1AMIAlTCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7389cb337fb35f894ed914da1fb786b54712406ff7a60de88ebbae3e067b57de","last_reissued_at":"2026-05-18T00:45:16.140828Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:45:16.140828Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Galaxy-scale gravitational lens candidates from the Hyper Suprime-Cam imaging survey and the Galaxy And Mass Assembly spectroscopic survey","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Anupreeta More, Atsushi J. Nishizawa, Bau-ching Hsieh, Hitoshi Murayama, James H. H. Chan, Jean Coupon, Masamune Oguri, Paul Price, Philip J. Tait, Satoshi Miyazaki, Sherry H. Suyu, Shiang-Yu Wang, Tsuyoshi Terai, Tzihong Chiueh, Yousuke Utsumi, Yutaka Komiyama","submitted_at":"2016-04-27T20:00:10Z","abstract_excerpt":"We present a list of galaxy-scale lens candidates including a highly probable interacting galaxy-scale lens in the Hyper Suprime-Cam (HSC) imaging survey. We combine HSC imaging with the blended-spectra catalog from the Galaxy And Mass Assembly (GAMA) survey to identify lens candidates, and use lens mass modeling to confirm the candidates. We find 46 matches between the HSC S14A_0b imaging data release and the GAMA catalog. Ten of them are probable lens systems according to their morphology and redshifts. There is one system with an interacting galaxy pair, HSC J084928+000949, that has a valid"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1604.08215","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":""},"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":"1604.08215","created_at":"2026-05-18T00:45:16.140943+00:00"},{"alias_kind":"arxiv_version","alias_value":"1604.08215v2","created_at":"2026-05-18T00:45:16.140943+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1604.08215","created_at":"2026-05-18T00:45:16.140943+00:00"},{"alias_kind":"pith_short_12","alias_value":"OOE4WM37WNPY","created_at":"2026-05-18T12:30:36.002864+00:00"},{"alias_kind":"pith_short_16","alias_value":"OOE4WM37WNPYSTWZ","created_at":"2026-05-18T12:30:36.002864+00:00"},{"alias_kind":"pith_short_8","alias_value":"OOE4WM37","created_at":"2026-05-18T12:30:36.002864+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/OOE4WM37WNPYSTWZCTNB7N4GWV","json":"https://pith.science/pith/OOE4WM37WNPYSTWZCTNB7N4GWV.json","graph_json":"https://pith.science/api/pith-number/OOE4WM37WNPYSTWZCTNB7N4GWV/graph.json","events_json":"https://pith.science/api/pith-number/OOE4WM37WNPYSTWZCTNB7N4GWV/events.json","paper":"https://pith.science/paper/OOE4WM37"},"agent_actions":{"view_html":"https://pith.science/pith/OOE4WM37WNPYSTWZCTNB7N4GWV","download_json":"https://pith.science/pith/OOE4WM37WNPYSTWZCTNB7N4GWV.json","view_paper":"https://pith.science/paper/OOE4WM37","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1604.08215&json=true","fetch_graph":"https://pith.science/api/pith-number/OOE4WM37WNPYSTWZCTNB7N4GWV/graph.json","fetch_events":"https://pith.science/api/pith-number/OOE4WM37WNPYSTWZCTNB7N4GWV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OOE4WM37WNPYSTWZCTNB7N4GWV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OOE4WM37WNPYSTWZCTNB7N4GWV/action/storage_attestation","attest_author":"https://pith.science/pith/OOE4WM37WNPYSTWZCTNB7N4GWV/action/author_attestation","sign_citation":"https://pith.science/pith/OOE4WM37WNPYSTWZCTNB7N4GWV/action/citation_signature","submit_replication":"https://pith.science/pith/OOE4WM37WNPYSTWZCTNB7N4GWV/action/replication_record"}},"created_at":"2026-05-18T00:45:16.140943+00:00","updated_at":"2026-05-18T00:45:16.140943+00:00"}