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A Submillimetre Survey of the Hubble Deep Field: Unveiling Dust-Enshrouded Star Formation in the Early Universe
David H. Hughes, James Dunlop, Michael Rowan-Robinson +11
The advent of sensitive sub-mm array cameras now allows a proper census of dust-enshrouded massive star-formation in very distant galaxies, previously hidden activity to which even…
The radio luminosity density of star-burst galaxies and co-moving star formation rate
Seb Oliver, Carlotta Gruppioni, Stephen Serjeant
We present a new determination of the co-moving star formation density at redshifts z~<0.35 from the 1.4 GHz luminosity function of sub-mJy star-burst galaxies. Our sample, taken f…
The local star formation rate and radio luminosity density
Stephen Serjeant, Carlotta Gruppioni, Seb Oliver
We present a new determination of the local volume-averaged star formation rate from the 1.4 GHz luminosity function of star forming galaxies. Our sample, taken from the B<=12 Revi…
Unveiling Dust-enshrouded Star Formation in the Early Universe: a Sub-mm Survey of the Hubble Deep Field
David Hughes, Steve Serjeant, James Dunlop +12
The advent of sensitive sub-mm array cameras now allows a proper census of dust-enshrouded massive star-formation in very distant galaxies, previously hidden activity to which even…
IRAS F10214+4724: the inner 100pc
Mark Lacy, Steve Rawlings, Stephen Serjeant
We use new near-infrared spectroscopy and our published optical spectroscopy of the gravitationally-lensed Seyfert-2 galaxy F10214+4724 to study both the links between the starburs…
A spectroscopic study of IRAS F10214+4724
Stephen Serjeant, Steve Rawlings, Mark Lacy +4
The z=2.286 IRAS galaxy F10214+4724 remains one of the most luminous galaxies in the Universe, despite its gravitational lens magnification. We present optical and near-infrared sp…