Measuring the star formation rate of the universe at z ∼ 1 from Hα with multi-object near-infrared spectroscopy

We have demonstrated the first near-infrared multi-object spectrograph, CIRPASS, on the 4.2-m William Herschel Telescope (WHT) and the 3.9-m Anglo-Australian Telescope. We have conducted an H survey of 38 0.77 < z < 1 galaxies over ∼100 arcmin2 of the Hubble Deep Field North and Flanki...

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Bibliografische gegevens
Hoofdauteurs: Bunker, A, Doherty, M, Sharp, R, Parry, I, Dalton, G, Lewis, I
Formaat: Journal article
Taal:English
Gepubliceerd in: 2006