{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:VXAWZFRCSRC7YLDBWLO73LAKFI","short_pith_number":"pith:VXAWZFRC","schema_version":"1.0","canonical_sha256":"adc16c96229445fc2c61b2ddfdac0a2a0bcc6f3bfd56f8b9f347be0aa2f25eac","source":{"kind":"arxiv","id":"2606.13781","version":2},"attestation_state":"computed","paper":{"title":"CANUCS/Technicolor Data Release 2: A Catalogue of Galaxy Structural Parameters in up to 29 HST+JWST bands and a Multi-Wavelength Exploration of the Galaxy Size-Mass Relation at $0.6 < z \\leq 4$","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Adam Muzzin, Chris J. Willott, Danilo Marchesini, Gabriel B. Brammer, Ga\\\"el Noirot, Georgios E. Magdis, Ghassan T. E. Sarrouh, Gregor Rihtar\\v{s}i\\v{c}, Guillaume Desprez, Jacqueline Antwi-Danso, Jon Jude\\v{z}, Kartheik G. Iyer, Katherine Myers, Lamiya A. Mowla, Luke Robbins, Marcin Sawicki, Maru\\v{s}a Brada\\v{c}, Maya Merchant, Natalie Allen, Nicholas S. Martis, Roberto Abraham, Rosa M. M\\'erida, Sunna Withers, Visal Sok, Westley Brown, Yoshihisa Asada","submitted_at":"2026-06-11T18:00:02Z","abstract_excerpt":"We present James Webb Space Telescope (JWST) results of a morphological study of galaxies in the CAnadian NIRISS Unbiased Cluster (CANUCS) and Technicolor surveys, observed in 19 medium- and broadband NIRCam filters in five CANUCS NIRCam Flanking Fields with rest-frame wavelength coverage between $\\sim 0.2 - 3.2\\mu m$. Using GALFIT, we measure the morphological parameters of $\\sim$ 4,100 star-forming galaxies at $0.6 < z \\leq 4$ with stellar masses of $8.5 < \\text{log}(M_*/M_\\odot) \\leq 11.5$. This enables us to concurrently examine how galaxy size varies as a function of stellar mass, redshif"},"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":"2606.13781","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2026-06-11T18:00:02Z","cross_cats_sorted":[],"title_canon_sha256":"56149b021e2fec4938ea1c6c2d3d8117e7a50ba7889b2a5b52e5064cf137a67c","abstract_canon_sha256":"4517378afc7b19731fba1a48f314cf2a0ffa8e5f353e846b4fecb8b0115c26c2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-06-19T16:10:56.044145Z","signature_b64":"a6V6Wt191LrRRmhtfjAqak/x/TUZENAi8VxCZg2UZmzDktQ/3PcGc6HppUvJjP2OiKsDNzU/NsB3h68CDSp6CQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"adc16c96229445fc2c61b2ddfdac0a2a0bcc6f3bfd56f8b9f347be0aa2f25eac","last_reissued_at":"2026-06-19T16:10:56.043747Z","signature_status":"signed_v1","first_computed_at":"2026-06-19T16:10:56.043747Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"CANUCS/Technicolor Data Release 2: A Catalogue of Galaxy Structural Parameters in up to 29 HST+JWST bands and a Multi-Wavelength Exploration of the Galaxy Size-Mass Relation at $0.6 < z \\leq 4$","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Adam Muzzin, Chris J. Willott, Danilo Marchesini, Gabriel B. Brammer, Ga\\\"el Noirot, Georgios E. Magdis, Ghassan T. E. Sarrouh, Gregor Rihtar\\v{s}i\\v{c}, Guillaume Desprez, Jacqueline Antwi-Danso, Jon Jude\\v{z}, Kartheik G. Iyer, Katherine Myers, Lamiya A. Mowla, Luke Robbins, Marcin Sawicki, Maru\\v{s}a Brada\\v{c}, Maya Merchant, Natalie Allen, Nicholas S. Martis, Roberto Abraham, Rosa M. M\\'erida, Sunna Withers, Visal Sok, Westley Brown, Yoshihisa Asada","submitted_at":"2026-06-11T18:00:02Z","abstract_excerpt":"We present James Webb Space Telescope (JWST) results of a morphological study of galaxies in the CAnadian NIRISS Unbiased Cluster (CANUCS) and Technicolor surveys, observed in 19 medium- and broadband NIRCam filters in five CANUCS NIRCam Flanking Fields with rest-frame wavelength coverage between $\\sim 0.2 - 3.2\\mu m$. Using GALFIT, we measure the morphological parameters of $\\sim$ 4,100 star-forming galaxies at $0.6 < z \\leq 4$ with stellar masses of $8.5 < \\text{log}(M_*/M_\\odot) \\leq 11.5$. This enables us to concurrently examine how galaxy size varies as a function of stellar mass, redshif"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2606.13781","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/2606.13781/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":"2606.13781","created_at":"2026-06-19T16:10:56.043805+00:00"},{"alias_kind":"arxiv_version","alias_value":"2606.13781v2","created_at":"2026-06-19T16:10:56.043805+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2606.13781","created_at":"2026-06-19T16:10:56.043805+00:00"},{"alias_kind":"pith_short_12","alias_value":"VXAWZFRCSRC7","created_at":"2026-06-19T16:10:56.043805+00:00"},{"alias_kind":"pith_short_16","alias_value":"VXAWZFRCSRC7YLDB","created_at":"2026-06-19T16:10:56.043805+00:00"},{"alias_kind":"pith_short_8","alias_value":"VXAWZFRC","created_at":"2026-06-19T16:10:56.043805+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/VXAWZFRCSRC7YLDBWLO73LAKFI","json":"https://pith.science/pith/VXAWZFRCSRC7YLDBWLO73LAKFI.json","graph_json":"https://pith.science/api/pith-number/VXAWZFRCSRC7YLDBWLO73LAKFI/graph.json","events_json":"https://pith.science/api/pith-number/VXAWZFRCSRC7YLDBWLO73LAKFI/events.json","paper":"https://pith.science/paper/VXAWZFRC"},"agent_actions":{"view_html":"https://pith.science/pith/VXAWZFRCSRC7YLDBWLO73LAKFI","download_json":"https://pith.science/pith/VXAWZFRCSRC7YLDBWLO73LAKFI.json","view_paper":"https://pith.science/paper/VXAWZFRC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2606.13781&json=true","fetch_graph":"https://pith.science/api/pith-number/VXAWZFRCSRC7YLDBWLO73LAKFI/graph.json","fetch_events":"https://pith.science/api/pith-number/VXAWZFRCSRC7YLDBWLO73LAKFI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VXAWZFRCSRC7YLDBWLO73LAKFI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VXAWZFRCSRC7YLDBWLO73LAKFI/action/storage_attestation","attest_author":"https://pith.science/pith/VXAWZFRCSRC7YLDBWLO73LAKFI/action/author_attestation","sign_citation":"https://pith.science/pith/VXAWZFRCSRC7YLDBWLO73LAKFI/action/citation_signature","submit_replication":"https://pith.science/pith/VXAWZFRCSRC7YLDBWLO73LAKFI/action/replication_record"}},"created_at":"2026-06-19T16:10:56.043805+00:00","updated_at":"2026-06-19T16:10:56.043805+00:00"}