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FLEX (The First Light Explorer)—The Science Case for a Fully OH Suppressed IFU Spectrograph

  • Simon Ellis
  • Joss Bland-Hawthorn
  • Anthony Horton
  • Roger Haynes
Part of the Astrophysics and Space Science Proceedings book series (ASSSP)

The ability to achieve deep near infrared spectroscopy is of great importance to the future of astronomy. Our understanding of the early Universe depends on our ability to observe highly redshifted spectroscopic diagnostic features. Observations of H-α at wavelengths 0.9≤λ≤1.8 μm would allow accurate star-formation rates to be measured over the period 0.4≤z≤1.7—a crucial period in the formation of galaxies. Observations of Lyman-α at the same wavelengths would probe 6≤z≤13—the epoch at which the Universe underwent a major (and poorly understood) phase change from neutral to ionised. Similarly our understanding of low mass stars and unbound planets relies on NIR spectroscopy, since these objects emit most of their light at NIR wavelengths.

Keywords

Fibre Bragg Grating Near Infrared Spectroscopy Crucial Period Large Core Diameter Excite Hydroxyl Radical 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer Science + Business Media B.V. 2009

Authors and Affiliations

  • Simon Ellis
    • 1
  • Joss Bland-Hawthorn
  • Anthony Horton
  • Roger Haynes
  1. 1.AAOEppingAustralia

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