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1
CIRPASS: Description, performance and astronomical results
Published 2004“…This near-infrared (MR) spectrograph has been used on the 8m Gemini-South Telescope, the 3.9m Anglo-Australian Telescope (AAT) and the 4.2m William Herschel Telescope (WHT). …”
Journal article -
2
Measuring the star formation rate of the universe at z ∼ 1 from Hα with multi-object near-infrared spectroscopy
Published 2006“…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 Flanking Fields, to determine star formation rates (SFRs) using CIRPASS on the WHT. …”
Journal article -
3
Multi-object near-infrared H alpha spectroscopy of z similar to 1 star-forming galaxies in the Hubble Deep Field North
Published 2004“…CIRPASS has been successfully demonstrated in multi-object mode on the Anglo-Australian Telescope (AAT) and the William Herschel Telescope (WHT). …”
Journal article