Measuring the Star Formation Rate of the Universe at z 1 from H-alpha with Multi-Object Near-Infrared Spectroscopy

Details Measuring the Star Formation Rate of the Universe at z 1 from H-alpha with Multi-Object Near-Infrared Spectroscopy Measuring the Star Formation Rate of the Universe at z 1 from H-alpha with Multi-Object Near-Infrared Spectroscopy

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aas...20917108b&link_type=abstract

2007 AAS/AAPT Joint Meeting, American Astronomical Society Meeting 209, #171.08; Bulletin of the American Astronomical Society,

Astronomy and Astrophysics

Astrophysics

Scientific paper

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 Hα survey of 38 0.77 1. This will resolve one of the long-standing puzzles in extragalactic astrophysics the true evolution of the Madau-Lilly diagram of star formation density.

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