FIRI - a Far-Infrared Interferometer
arXiv:0707.1822 · doi:10.1007/s10686-008-9100-2
Abstract
Half of the energy ever emitted by stars and accreting objects comes to us in the FIR waveband and has yet to be properly explored. We propose a powerful Far-InfraRed Interferometer mission, FIRI, to carry out high-resolution imaging spectroscopy in the FIR. This key observational capability is essential to reveal how gas and dust evolve into stars and planets, how the first luminous objects in the Universe ignited, how galaxies formed, and when super-massive black holes grew. FIRI will disentangle the cosmic histories of star formation and accretion onto black holes and will trace the assembly and evolution of quiescent galaxies like our Milky Way. Perhaps most importantly, FIRI will observe all stages of planetary system formation and recognise Earth-like planets that may harbour life, via its ability to image the dust structures in planetary systems. It will thus address directly questions fundamental to our understanding of how the Universe has developed and evolved - the very questions posed by ESA's Cosmic Vision.
Proposal developed by a large team of astronomers from Europe, USA and Canada and submitted to the European Space Agency as part of "Cosmic Vision 2015-2025"
References in corpus (8)
- The Demography of Massive Dark Objects in Galaxy Centres
- A Deep Sub-millimeter Survey of Lensing Clusters: A New Window on Galaxy Formation and Evolution
- Submillimeter Galaxies
- Cosmic Microwave Background Anisotropies
- The evolutionary sequence of active galactic nuclei and galaxy formation revealed
- Detection of the Buried AGN in NGC 6240 with the Infrared Spectrograph on The Spitzer Space Telescope
- A filamentary structure of massive star-forming galaxies associated with an X-ray absorbed QSO at z=1.8
- The Space Infrared Interferometric Telescope (SPIRIT): High-resolution imaging and spectroscopy in the far-infrared
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- Far-Infrared double-Fourier interferometers and their spectral sensitivity
- Constraints on the galaxy "main sequence" at z>5: the stellar mass of HDF850.1
- A Fabrication Route for Arrays of Ultra-low-Noise MoAu Transition Edge Sensors on Thin Silicon Nitride for Space Applications
- A Realistic Roadmap to Formation Flying Space Interferometry
- Optical NEP in Hot-Electron Nanobolometers