{"paper":{"title":"Spectrophotometric properties of galaxies at intermediate redshifts (z ~ 0.2--1.0) I. Sample description, photometric properties and spectral measurements","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"CAUP), Fabrice Lamareille (LATT), IAP), Jarle Brinchmann (MPA, Jean-Fran\\c{c}ois Le Borgne (LATT), Johan Richard (LATT), St\\'ephane Charlot (MPA, Thierry Contini (LATT)","submitted_at":"2005-11-04T15:44:12Z","abstract_excerpt":"We present the spectrophotometric properties of a sample of 141 emission-line galaxies at redshifts in the range $0.2<z<1.0$ with a peak around $z\\in[0.2,0.4]$. The analysis is based on medium resolution ($R\\_{\\mathrm{s}}=500-600$), optical spectra obtained at VLT and Keck. The targets are mostly {} \"Canada-France Redshift Survey\" emission-line galaxies, with the addition of field galaxies randomly selected behind lensing clusters. We complement this sample with galaxy spectra from the {} \"Gemini Deep Deep Survey\" public data release. We have computed absolute magnitudes of the galaxies and me"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0511134","kind":"arxiv","version":3},"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"}