English

A Concept for an STJ-based Spectrograph

Astrophysics 2009-11-07 v1

Abstract

We describe a multi-order spectrograph concept suitable for 8m-class telescopes, using the intrinsic spectral resolution of Superconducting Tunneling Junction detectors to sort the spectral orders. The spectrograph works at low orders, 1-5 or 1-6, and provides spectral coverage with a resolving power of R~8000 from the atmospheric cutoff at 320 nm to the long wavelength end of the infrared H or K band at 1800 nm or 2400 nm. We calculate that the spectrograph would provide substantial throughput and wavelength coverage, together with high time resolution and sufficient dynamic range. The concept uses currently available technology, or technologies with short development horizons, restricting the spatial sampling to two linear arrays; however an upgrade path to provide more spatial sampling is identified. All of the other challenging aspects of the concept - the cryogenics, thermal baffling and magnetic field biasing - are identified as being feasible.

Keywords

Cite

@article{arxiv.astro-ph/0305057,
  title  = {A Concept for an STJ-based Spectrograph},
  author = {Mark Cropper and M. Barlow and M. A. C. Perryman and Keith Horne and R. Bingham and M. Page and P. Guttridge and A. Smith and A. Peacock and D. Walker and P. Charles},
  journal= {arXiv preprint arXiv:astro-ph/0305057},
  year   = {2009}
}

Comments

Accepted in Monthly Notices of the Royal Astronomical Society, 12 pages with 10 figures