{"paper":{"title":"MIFS: A Mega Integral Field Spectrograph for the VLT","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"B. Guiderdoni, E. Emsellem, E. Pecontal, E. Prieto, F. Combes, G. Adam, G. Gilmore, M. Franx, O. LeFevre, P. Ferruit, P.T. de Zeeuw, P. van der Werf, R. Bacon, R.L. Davies, R. Sharples, S. Cabrit, S. Morris","submitted_at":"2001-09-05T12:08:57Z","abstract_excerpt":"We describe MIFS, a second generation integral-field spectrograph for the VLT, operating in the visible wavelength range. It combines a 1'x1' field of view with the improved spatial resolution provided by multi-conjugate adaptive optics and covers a large simultaneous spectral range (0.6-1.0 microns). A separate mode exploits the highest spatial resolution provided by adaptive optics. With this unique combination of capabilities, MIFS has a wide domain of application and a large discovery potential.\n  The MIFS low-spatial resolution mode (sampled at 0.2\") combined with the initial MCAO capabil"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0109060","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":""},"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"}