{ "id": "astro-ph/0407218", "version": "v1", "published": "2004-07-12T09:04:34.000Z", "updated": "2004-07-12T09:04:34.000Z", "title": "Star Formation at Redshift One: Preliminary results from an H-alpha Survey", "authors": [ "M. Doherty", "A. Bunker", "R. Sharp", "G. Dalton", "I. Parry", "I. Lewis", "E. MacDonald", "C. Wolf" ], "comment": "4 pages, 1 figure, to appear in the proceedings of the XXXIXth Rencontres de Moriond \"Exploring the Universe\"", "categories": [ "astro-ph" ], "abstract": "We present the first successful demonstration of multi-object near-infrared spectroscopy on high redshift galaxies. Our objective is to address the true star formation history of the universe at z~1, a crucial epoch which some have suggested is the peak of star formation activity. By using H-alpha -the same robust star formation indicator used at low-z - redshifted into the J- and H-bands, we can trace star formation without the systematic uncertainties of different calibrators, or the extreme dust extinction in the rest-UV, which have plagued previous efforts. We are using the instrument CIRPASS (the Cambridge Infra-Red PAnoramic Survey Spectrograph), in multi-object mode, which has been successfully demonstrated on the Anglo-Australian Telescope (AAT) and the William Herschel Telescope (WHT). CIRPASS has 150 fibres deployable over \\~40arcmin on the AAT and ~15arcmin on the WHT. Here we present preliminary results from one of our fields observed with the WHT: H-alpha detections of z~1 galaxies in the Hubble Deep Field North.", "revisions": [ { "version": "v1", "updated": "2004-07-12T09:04:34.000Z" } ], "analyses": { "keywords": [ "preliminary results", "h-alpha survey", "robust star formation indicator", "cambridge infra-red panoramic survey spectrograph", "true star formation history" ], "note": { "typesetting": "TeX", "pages": 4, "language": "en", "license": "arXiv", "status": "editable", "inspire": 654142, "adsabs": "2004astro.ph..7218D" } } }