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All Outputs (6)

Multiple Integral Field Spectroscopy (2002)
Presentation / Conference Contribution
Wright, G., Ivison, R., Hastings, P., Wells, M., Sharples, R., Allington-Smith, J., & Content, R. (2002). Multiple Integral Field Spectroscopy.

A Million Element Integral Field Unit (MEIFU) (2002)
Presentation / Conference Contribution
Morris, S., Content, R., Sharples, R., Bower, R., Davies, R., & Baugh, C. (2002). A Million Element Integral Field Unit (MEIFU). In Scientific Drivers for ESO Future VLT/VLTI Instrumentation: Proceedings of the ESO Workshop Held in Garching, Germany, 11-15 June 2001 (99-107). https://doi.org/10.1007/10857019_16

We describe an instrument concept that will provide simultaneous spectra for a million spatial samples on the sky. With the proposed field of view and spectral resolution, it will be able to measure redshifts and line strengths for around 2-4000 z∼∼3... Read More about A Million Element Integral Field Unit (MEIFU).

Integral field spectroscopy with the Gemini Multiobject Spectrograph. I. design, construction, and testing (2002)
Journal Article
Allington-Smith, J., Murray, G., Content, R., Dodsworth, G., Davies, R., Miller, B., …Murowinski, R. (2002). Integral field spectroscopy with the Gemini Multiobject Spectrograph. I. design, construction, and testing. Publications of the Astronomical Society of the Pacific, 114(798), 892-912

The Gemini Multiobject Spectrograph (GMOS) installed on the Gemini-North telescope has a facility for integral field spectroscopy over the wavelength range 0.4-1.0 mum. GMOS is converted to this mode by the remote insertion of an integral field unit... Read More about Integral field spectroscopy with the Gemini Multiobject Spectrograph. I. design, construction, and testing.

The origin of [FeII] emission in NGC 4151 (2002)
Journal Article
Turner, J., Allington-Smith, J., Chapman, S., Content, R., Done, C., Haynes, R., …Morris, S. (2002). The origin of [FeII] emission in NGC 4151. Monthly Notices of the Royal Astronomical Society, 331(2), 284-292. https://doi.org/10.1046/j.1365-8711.2002.05214.x

The centre of NGC 4151 has been observed in the J band with the SMIRFS integral field unit (IFU) on the UK Infrared Telescope. A map of [Fe ii] emission is derived, and compared with the distributions of the optical narrow-line region and radio jet.... Read More about The origin of [FeII] emission in NGC 4151.