First Science from HerMES: the final starbursts in massive galaxies at 0.5<z<1.0

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Herschel has now successfully launched, and commenced routine operations. The multiple far-IR bands of Herschel, coupled with its ability to deeply survey large areas of sky on rapid timescales, makes it the ideal instrument to resolve some of the key problems in galaxy formation raised by instruments such as SCUBA. In this proposal we aim to take the first steps in exploiting the enormous power of Herschel, by using GMOS to obtain redshifts and spectral diagnostics for some of the most extreme objects that Herschel detects in the HerMES guaranteed time survey. These are rare (1 per square degree) sub-mm bright, optically faint sources at 0.5

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