BASIS: Bayfordbury single-object integral field spectrograph
Author
Richards, S.
Martin, Bill
Campbell, D.
Jones, H.R.A.
Bland-Hawthorn, J.
Lawrence, J.
Brinks, E.
Bryant, J.J.
Fogarty, L.
Gallaway, M.
Goodwin, M.
Leon-Saval, S.
Sarzi, M.
Smith, Daniel
Attention
2299/13046
Abstract
We present an inexpensive (<US$500) and easily replicable integral field unit for use on small aperture telescopes. Based on a commercial small spectrograph (SBIG Self-Guiding Spectrograph) and a 37 optical fibre bundle integral field unit with each fibre having 50μm cores and a pitch of 125μm. It has an overall field-of-view of 40 arc seconds (2.6arcsec/core), a resolution of 9Å from 3995Å to 7170Å and an average system efficiency of 9%, yielding a signal-tonoise ratio of 10 for a 20min exposure of a 13mag/arcsec2 source. Still in commissioning, we present first light observations of Vega and M57. © (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). [Downloading of the abstract is permitted for personal use only]