{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:YEMPBCC4GHO24M242C2XTB2CSL","short_pith_number":"pith:YEMPBCC4","schema_version":"1.0","canonical_sha256":"c118f0885c31ddae335cd0b579874292de673952dc716aa31b0a70d8e623aa02","source":{"kind":"arxiv","id":"2407.15412","version":1},"attestation_state":"computed","paper":{"title":"Visible Photonic Lantern integration, characterization and on-sky testing on Subaru/SCExAO","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"Barnaby Norris, Chris Betters, Elsa huby, Guillermo Martin, Guy Perrin, Harry-Dean Kenchington Goldsmith, Jon Lin, Julien Lozi, Kyohoon Ahn, Manon Lallement, Michael P. Fitzgerald, Miles Lucas, Motohide Tamura, Nemanja Jovanovic, Olivier Guyon, Pradip Gatkine, Rodrigo Amezcua-Correa, S\\'ebastien Vievard, Sergio Leon-Saval, Stephanos Yerolatsitis, Steph Sallum, Sylvestre Lacour, Takayuki Kotani, Thayne Currie, Vincent Deo, Yoo-Jung Kim","submitted_at":"2024-07-22T06:39:21Z","abstract_excerpt":"A Photonic Lantern (PL) is a novel device that efficiently converts a multi-mode fiber into several single-mode fibers. When coupled with an extreme adaptive optics (ExAO) system and a spectrograph, PLs enable high throughput spectroscopy at high angular resolution. The Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) system of the Subaru Telescope recently acquired a PL that converts its multi-mode input into 19 single-mode outputs. The single mode outputs feed a R~4,000 spectrograph optimized for the 600 to 760 nm wavelength range. We present here the integration of the PL on SCExAO, an"},"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":"2407.15412","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.IM","submitted_at":"2024-07-22T06:39:21Z","cross_cats_sorted":[],"title_canon_sha256":"379513ec1b62858fc02a4fe2253c18c9ba3733bda276dcc9720a5a5270834c37","abstract_canon_sha256":"731431e052abdc6e212a54cd0520438be404be5e4a1eed06e354b6f476bc9479"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:46:43.546980Z","signature_b64":"1WC5cwqDJ6kLGx+Ts7VRJ1yEA/hfQxdXoYdtVRhPkHW7Nww7gmeKQ+EfgWC1yEg8kQbHzhsZ52SforpCompVBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c118f0885c31ddae335cd0b579874292de673952dc716aa31b0a70d8e623aa02","last_reissued_at":"2026-07-05T08:46:43.546449Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:46:43.546449Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Visible Photonic Lantern integration, characterization and on-sky testing on Subaru/SCExAO","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.IM","authors_text":"Barnaby Norris, Chris Betters, Elsa huby, Guillermo Martin, Guy Perrin, Harry-Dean Kenchington Goldsmith, Jon Lin, Julien Lozi, Kyohoon Ahn, Manon Lallement, Michael P. Fitzgerald, Miles Lucas, Motohide Tamura, Nemanja Jovanovic, Olivier Guyon, Pradip Gatkine, Rodrigo Amezcua-Correa, S\\'ebastien Vievard, Sergio Leon-Saval, Stephanos Yerolatsitis, Steph Sallum, Sylvestre Lacour, Takayuki Kotani, Thayne Currie, Vincent Deo, Yoo-Jung Kim","submitted_at":"2024-07-22T06:39:21Z","abstract_excerpt":"A Photonic Lantern (PL) is a novel device that efficiently converts a multi-mode fiber into several single-mode fibers. When coupled with an extreme adaptive optics (ExAO) system and a spectrograph, PLs enable high throughput spectroscopy at high angular resolution. The Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) system of the Subaru Telescope recently acquired a PL that converts its multi-mode input into 19 single-mode outputs. The single mode outputs feed a R~4,000 spectrograph optimized for the 600 to 760 nm wavelength range. We present here the integration of the PL on SCExAO, an"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2407.15412","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/2407.15412/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":"2407.15412","created_at":"2026-07-05T08:46:43.546506+00:00"},{"alias_kind":"arxiv_version","alias_value":"2407.15412v1","created_at":"2026-07-05T08:46:43.546506+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2407.15412","created_at":"2026-07-05T08:46:43.546506+00:00"},{"alias_kind":"pith_short_12","alias_value":"YEMPBCC4GHO2","created_at":"2026-07-05T08:46:43.546506+00:00"},{"alias_kind":"pith_short_16","alias_value":"YEMPBCC4GHO24M24","created_at":"2026-07-05T08:46:43.546506+00:00"},{"alias_kind":"pith_short_8","alias_value":"YEMPBCC4","created_at":"2026-07-05T08:46:43.546506+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/YEMPBCC4GHO24M242C2XTB2CSL","json":"https://pith.science/pith/YEMPBCC4GHO24M242C2XTB2CSL.json","graph_json":"https://pith.science/api/pith-number/YEMPBCC4GHO24M242C2XTB2CSL/graph.json","events_json":"https://pith.science/api/pith-number/YEMPBCC4GHO24M242C2XTB2CSL/events.json","paper":"https://pith.science/paper/YEMPBCC4"},"agent_actions":{"view_html":"https://pith.science/pith/YEMPBCC4GHO24M242C2XTB2CSL","download_json":"https://pith.science/pith/YEMPBCC4GHO24M242C2XTB2CSL.json","view_paper":"https://pith.science/paper/YEMPBCC4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2407.15412&json=true","fetch_graph":"https://pith.science/api/pith-number/YEMPBCC4GHO24M242C2XTB2CSL/graph.json","fetch_events":"https://pith.science/api/pith-number/YEMPBCC4GHO24M242C2XTB2CSL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YEMPBCC4GHO24M242C2XTB2CSL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YEMPBCC4GHO24M242C2XTB2CSL/action/storage_attestation","attest_author":"https://pith.science/pith/YEMPBCC4GHO24M242C2XTB2CSL/action/author_attestation","sign_citation":"https://pith.science/pith/YEMPBCC4GHO24M242C2XTB2CSL/action/citation_signature","submit_replication":"https://pith.science/pith/YEMPBCC4GHO24M242C2XTB2CSL/action/replication_record"}},"created_at":"2026-07-05T08:46:43.546506+00:00","updated_at":"2026-07-05T08:46:43.546506+00:00"}