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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

The HETDEX Instrumentation: Hobby-Eberly Telescope Wide Field Upgrade and VIRUS

(2021)

Authors:

Gary J Hill, Hanshin Lee, Phillip J MacQueen, Andreas Kelz, Niv Drory, Brian L Vattiat, John M Good, Jason Ramsey, Herman Kriel, Trent Peterson, DL DePoy, Karl Gebhardt, JL Marshall, Sarah E Tuttle, Svend M Bauer, Taylor S Chonis, Maximilian H Fabricius, Cynthia Froning, Marco Haeuser, Briana L Indahl, Thomas Jahn, Martin Landriau, Ron Leck, Francesco Montesano, Travis Prochaska, Jan M Snigula, Gregory R Zeimann, Randy Bryant, George Damm, JR Fowler, Steven Janowiecki, Jerry Martin, Emily Mrozinski, Stephen Odewahn, Sergey Rostopchin, Matthew Shetrone, Renny Spencer, Erin Mentuch Cooper, Taft Armandroff, Ralf Bender, Gavin Dalton, Ulrich Hopp, Eiichiro Komatsu, Harald Nicklas, Lawrence W Ramsey, Martin M Roth, Donald P Schneider, Chris Sneden, Matthias Steinmetz
More details from the publisher
Details from ArXiV

The Hobby-Eberly Telescope Dark Energy Experiment (HETDEX) Survey Design, Reductions, and Detections

(2021)

Authors:

Karl Gebhardt, Erin Mentuch Cooper, Robin Ciardullo, Viviana Acquaviva, Ralf Bender, William P Bowman, Barbara G Castanheira, Gavin Dalton, Dustin Davis, Roelof S de Jong, DL DePoy, Yaswant Devarakonda, Sun Dongsheng, Niv Drory, Maximilian Fabricius, Daniel J Farrow, John Feldmeier, Steven L Finkelstein, Cynthia S Froning, Eric Gawiser, Caryl Gronwall, Laura Herold, Gary J Hill, Ulrich Hopp, Lindsay R House, Steven Janowiecki, Matthew Jarvis, Donghui Jeong, Shardha Jogee, Ryota Kakuma, Andreas Kelz, W Kollatschny, Eiichiro Komatsu, Mirko Krumpe, Martin Landriau, Chenxu Liu, Maja Lujan Niemeyer, Phillip MacQueen, Jennifer Marshall, Ken Mawatari, Emily M McLinden, Shiro Mukae, Gautam Nagaraj, Yoshiaki Ono, Masami Ouchi, Casey Papovich, Nao Sakai, Shun Saito, Donald P Schneider, Andreas Schulze, Khavvia Shanmugasundararaj, Matthew Shetrone, Chris Sneden, Jan Snigula, Matthias Steinmetz, Benjamin P Thomas, Brianna Thomas, Sarah Tuttle, Tanya Urrutia, Lutz Wisotzki, Isak Wold, Gregory Zeimann, Yechi Zhang
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Details from ArXiV

Wide-Field Near Infrared Imaging

Chapter in , World Scientific Publishing (2021) 175-185
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MOSAIC on the ELT: high-multiplex spectroscopy to unravel the physics of stars and galaxies from the dark ages to the present-day

The ESO Messenger (2021)

Authors:

F Hammer, S Morris, Jg Cuby, L Kaper, M Steinmetz, J Afonso, B Barbuy, E Bergin, A Finogenov, J Gallego, S Kassin, L Penterricci, D Schaerer, B Ziegler, K Dohlen, M Dubbeldam, K El Hadi, A Janssen, A Kelz, M Larrieu, I Lewis, M MacIntosh, T Morris, R Navarro, W Seifert

Abstract:

The powerful combination of the cutting-edge multi-object spectrograph MOSAIC with the world largest telescope, the ELT, will allow us to probe deeper into the Universe than was possible. MOSAIC is an extremely efficient instrument in providing spectra for the numerous faint sources in the Universe, including the very first galaxies and sources of cosmic reionization. MOSAIC has a high multiplex in the NIR and in the VIS, in addition to multi-Integral Field Units (Multi-IFUs) in NIR. As such it is perfectly suited to carry out an inventory of dark matter (from rotation curves) and baryons in the cool-warm gas phases in galactic haloes at z=3-4. MOSAIC will enable detailed maps of the intergalactic medium at z=3, the evolutionary history of dwarf galaxies during a Hubble time, the chemistry directly measured from stars up to several Mpc. Finally, it will measure all faint features seen in cluster gravitational lenses or in streams surrounding nearby galactic halos, providing MOSAIC to be a powerful instrument with an extremely large space of discoveries. The preliminary design of MOSAIC is expected to begin next year, and its level of readiness is already high, given the instrumental studies made by the team.
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Details from ORA
Details from ArXiV

Fibre links for the WEAVE instrument: the making of

Society of Photo-optical Instrumentation Engineers (2020) 114502F

Authors:

Shan Mignot, Piercarlo Bonifacio, Gilles Fasola, Gavin Dalton, Ian Lewis

Abstract:

The WEAVE instrument nearing completion for the William Herschel Telescope is a fiber-fed spectrograph operating in three different modes. Two comprise deployable fibers at the prime focus for point-like objects and small integral field units (IFU), the third is a large IFU placed at the center of the field. Three distinct fiber systems support these modes and route the photons to the spectrograph located on the Nasmyth platform 33m away: the first features 960+940 fibers and is duplicated to allow configuring the fibers on one plate while observation is carried out on the other, the second has 20 hexagonal IFUs featuring 37 fibers each, the third is a large array of 609 fibers with twice the former’s diameter. The large number of fibers and the diversity of their instantiation have made procurement of the parts and assembly of the custom cables a challenge. They involve project partners in France, the UK and the Netherlands and industrial partners in France, Canada, the USA and China to combine know-how and compress the schedule by parallelizing assembly of the cables. Besides the complex management that this induces, it has called for revising the fibers’ handling to relax tolerances and for a rigorous assessment of the conformity of the products. This paper tells the story of the making of the fiber links, presents the overall organization of the procurement and assembly chains together with the inspection and testing allowing for assessing the conformance of the hardware delivered.
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