{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:TK7PGD3NQLA3USFQ7EN3MEN66S","short_pith_number":"pith:TK7PGD3N","schema_version":"1.0","canonical_sha256":"9abef30f6d82c1ba48b0f91bb611bef4b05f971abfc7272318be853dc3868f1e","source":{"kind":"arxiv","id":"1605.06334","version":2},"attestation_state":"computed","paper":{"title":"The impact of JWST broad-band filter choice on photometric redshift estimation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Koekemoer, H. U. N{\\o}rgaard-Nielsen, J. Pye, K. I. Caputi, L. Bisigello, L. Colina, N. Grogin, O. Ilbert, O. Le F\\`evre, P. G. P\\'erez-Gonz\\'alez, P. van der Werf","submitted_at":"2016-05-20T12:53:31Z","abstract_excerpt":"The determination of galaxy redshifts in James Webb Space Telescope (JWST)'s blank-field surveys will mostly rely on photometric estimates, based on the data provided by JWST's Near-Infrared Camera (NIRCam) at 0.6-5.0 {\\mu}m and Mid Infrared Instrument (MIRI) at {\\lambda}>5.0 {\\mu}m. In this work we analyse the impact of choosing different combinations of NIRCam and MIRI broad-band filters (F070W to F770W), as well as having ancillary data at {\\lambda}<0.6 {\\mu}m, on the derived photometric redshifts (zphot) of a total of 5921 real and simulated galaxies, with known input redshifts z=0-10. We "},"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":"1605.06334","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-05-20T12:53:31Z","cross_cats_sorted":[],"title_canon_sha256":"8d504ccea453eba5e872b019550ab7b75ddb9e557d93d3390c1ffb423318b6bf","abstract_canon_sha256":"3341a2e64d060529ba322a635012f7f1f56b909368e3692acca07958f495500c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:55:13.739736Z","signature_b64":"GA/Yr2703lBFER4bZjD7vtXWhl01ah8wXJd7UwH22xn09BN3QTI1pZpFfyiInO5v+vkiJkhB6xB+rlhmqL9hBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9abef30f6d82c1ba48b0f91bb611bef4b05f971abfc7272318be853dc3868f1e","last_reissued_at":"2026-05-18T00:55:13.739356Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:55:13.739356Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The impact of JWST broad-band filter choice on photometric redshift estimation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"A. Koekemoer, H. U. N{\\o}rgaard-Nielsen, J. Pye, K. I. Caputi, L. Bisigello, L. Colina, N. Grogin, O. Ilbert, O. Le F\\`evre, P. G. P\\'erez-Gonz\\'alez, P. van der Werf","submitted_at":"2016-05-20T12:53:31Z","abstract_excerpt":"The determination of galaxy redshifts in James Webb Space Telescope (JWST)'s blank-field surveys will mostly rely on photometric estimates, based on the data provided by JWST's Near-Infrared Camera (NIRCam) at 0.6-5.0 {\\mu}m and Mid Infrared Instrument (MIRI) at {\\lambda}>5.0 {\\mu}m. In this work we analyse the impact of choosing different combinations of NIRCam and MIRI broad-band filters (F070W to F770W), as well as having ancillary data at {\\lambda}<0.6 {\\mu}m, on the derived photometric redshifts (zphot) of a total of 5921 real and simulated galaxies, with known input redshifts z=0-10. We "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1605.06334","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":"1605.06334","created_at":"2026-05-18T00:55:13.739416+00:00"},{"alias_kind":"arxiv_version","alias_value":"1605.06334v2","created_at":"2026-05-18T00:55:13.739416+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1605.06334","created_at":"2026-05-18T00:55:13.739416+00:00"},{"alias_kind":"pith_short_12","alias_value":"TK7PGD3NQLA3","created_at":"2026-05-18T12:30:44.179134+00:00"},{"alias_kind":"pith_short_16","alias_value":"TK7PGD3NQLA3USFQ","created_at":"2026-05-18T12:30:44.179134+00:00"},{"alias_kind":"pith_short_8","alias_value":"TK7PGD3N","created_at":"2026-05-18T12:30:44.179134+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/TK7PGD3NQLA3USFQ7EN3MEN66S","json":"https://pith.science/pith/TK7PGD3NQLA3USFQ7EN3MEN66S.json","graph_json":"https://pith.science/api/pith-number/TK7PGD3NQLA3USFQ7EN3MEN66S/graph.json","events_json":"https://pith.science/api/pith-number/TK7PGD3NQLA3USFQ7EN3MEN66S/events.json","paper":"https://pith.science/paper/TK7PGD3N"},"agent_actions":{"view_html":"https://pith.science/pith/TK7PGD3NQLA3USFQ7EN3MEN66S","download_json":"https://pith.science/pith/TK7PGD3NQLA3USFQ7EN3MEN66S.json","view_paper":"https://pith.science/paper/TK7PGD3N","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1605.06334&json=true","fetch_graph":"https://pith.science/api/pith-number/TK7PGD3NQLA3USFQ7EN3MEN66S/graph.json","fetch_events":"https://pith.science/api/pith-number/TK7PGD3NQLA3USFQ7EN3MEN66S/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TK7PGD3NQLA3USFQ7EN3MEN66S/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TK7PGD3NQLA3USFQ7EN3MEN66S/action/storage_attestation","attest_author":"https://pith.science/pith/TK7PGD3NQLA3USFQ7EN3MEN66S/action/author_attestation","sign_citation":"https://pith.science/pith/TK7PGD3NQLA3USFQ7EN3MEN66S/action/citation_signature","submit_replication":"https://pith.science/pith/TK7PGD3NQLA3USFQ7EN3MEN66S/action/replication_record"}},"created_at":"2026-05-18T00:55:13.739416+00:00","updated_at":"2026-05-18T00:55:13.739416+00:00"}