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Part of a WEAVE fibre configuration

Part of the WEAVE focal plane showing optical fibres positioned on a set of targets in the telescope focal plane.

Prof Gavin Dalton

Professor of Astrophysics

Research theme

  • Astronomy and astrophysics

Sub department

  • Astrophysics

Research groups

  • Astronomical instrumentation
  • Extremely Large Telescope
Gavin.Dalton@physics.ox.ac.uk
  • About
  • Research
  • Publications

A time delay for the cluster-lensed quasar SDSS J1004+4112

ASTROPHYSICAL JOURNAL 662:1 (2007) 62-71

Authors:

J Fohlmeister, CS Kochanek, EE Falco, J Wambsganss, N Morgan, CW Morgan, EO Ofek, D Maoz, CR Keeton, JC Barentine, G Dalton, J Dembicky, W Ketzeback, R McMillan, CS Peters
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Physics, and faith are worth debating

PHYSICS WORLD 20:12 (2007) 23-23

Authors:

Andrew Briggs, Gavin Dalton, Paul Ewart, Andrew Steane, Justin Wark, William Phillips
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Practical implementation of the complex wavefront modulation model for optical alignment - art. no. 66170N

P SOC PHOTO-OPT INS 6617 (2007) N6170-N6170

Authors:

H Lee, GB Dalton, IAJ Tosh, SW Kim

Abstract:

We discuss the implementation of the complex wavefront modulation model in practical optical alignment procedures and present its interim results. This modulation model describes the relation between the alignment state and the wavefront of a system, both are expressed in mathematical complex quantities. It addresses the importance of the coupled inter-element alignment effect to the resultant system wavefront. We utilise this effect in order to extract the alignment state of a system from measured optical wavefronts. We demonstrate the method's practical applicability to the real optical alignment procedure by showing alignment simulations of a centered three-mirror system.
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Cryogenic mounts for large fused silica lenses

Proceedings of SPIE - The International Society for Optical Engineering 6273 II (2006)

Authors:

TR Froud, IAJ Tosh, RL Edeson, GB Dalton

Abstract:

This paper describes the design and development of an accurate temperature compliant lens mounting technique being used on the camera of the UK-FMOS near infrared spectrograph for operation at the Subaru Telescope in Hawaii. A series of fused silica lenses of up to 4.4kg, 255mm in diameter and operating at temperatures as low as 70K are supported within flexures cut away from stainless steel outer rings. Intermediate low thermal expansion pads are attached to these flexures and in turn bonded to the glass during the alignment process. This mounting method lends itself to the domino chips type of assembly process which can be carried out on a rotary table to maintain accurate axial alignment. A detailed description of the overall design progression including the methods of manufacture, alignment process, adhesive selection, assembly methods and testing is included.
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The UK FMOS spectrograph

Proceedings of SPIE - The International Society for Optical Engineering 6269 II (2006)

Authors:

GB Dalton, IJ Lewis, DG Bonfield, AR Holmes, CB Brooks, H Lee, IAJ Tosh, TR Froud, M Patel, NA Dipper, C Blackburn

Abstract:

We describe the build phase of the UK FMOS spectrograph, a 200 fibre cooled OH Suppression infrared spectrograph being constructed as part of Subaru's Fibre Multi Object Spectroscopy facility. Here we describe recent UK activities within the FMOS programme and the likely schedule for commissioning at Subaru.
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