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Part of the book series: Eso Astrophysics Symposia ((ESO))

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We describe a concept for a near-infrared (JHK) bulk-optics combiner designed for efficient model-independent imaging of faint sources. Thecombiner is designed to accommodate (through a reconfigurable switchyard) any number of input beams from three to six. The instrument will include its own group-delay fringe tracker in addition to the “science” beam combiner. This will mean that fringe tracking will be possible using baseline “bootstrapping” while science data can be being secured on much longer baselines where the fringe visibility may be very low. We expect that a photon-efficient optical design will allow faint (K ~ 13) science targets to be observed, including AGN. Our proposed instrument will allow the full imaging potential of the VLTI infrastructure to be realised

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© 2007 Springer

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Buscher, D., Baron, F., Coyne, J., Haniff, C., Young, J. (2007). BOBCAT - A Photon-efficient Multi-way Combiner for the VLTI. In: Richichi, A., Delplancke, F., Paresce, F., Chelli, A. (eds) The Power of Optical/IR Interferometry: Recent Scientific Results and 2nd Generation Instrumentation. Eso Astrophysics Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-74256-2_48

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