91探花

Skip to main content
Department Of Physics text logo
  • Research
    • Our research
    • Our research groups
    • Our research in action
    • Research funding 91探花
    • Summer internships for undergraduates
  • Study
    • Undergraduates
    • Postgraduates
  • Engage
    • For alumni
    • For business
    • For schools
    • For the public
  • Support
91探花
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 Subaru FMOS galaxy redshift survey (FastSound). V. Intrinsic alignments of emission line galaxies at $z\sim 1.4$

(2017)

Authors:

Motonari Tonegawa, Teppei Okumura, Tomonori Totani, Gavin Dalton, Karl Glazebrook, Kiyoto Yabe

Learning from history: adaptive calibration of 'tilting spine' fiber positioners

Astronomical Data Analysis Software and Systems XXV Astronomical Society of the Pacific (2017) 643-646

Authors:

James Gilbert, Gavin Dalton

Abstract:

This paper discusses a new approach for determining the calibration parameters of independently-actuated optical fibers in multi-object astronomical fiber positioning systems. This work comes from the development of a new type of piezoelectric motor intended to enhance the 鈥榯ilting spine' fiber positioning technology originally created by the Australian Astronomical Observatory. Testing has shown that the motor's performance can vary depending on the fiber's location within its accessible field, meaning that an individual fiber is difficult to calibrate with a one-time routine. Better performance has resulted from constantly updating calibration parameters based on the observed movements of the fiber during normal closed-loop positioning. Over time, location-specific historical data is amassed that can be used to better predict the results of a future fiber movement. This is similar to a technique previously proposed by the Australian Astronomical Observatory, but with the addition of location-specific learning. Results from a prototype system are presented, showing a significant reduction in overall positioning error when using this new approach.

CONSTRAINT ON THE INFLOW/OUTFLOW RATES IN STAR-FORMING GALAXIES AT z similar to 1.4 FROM MOLECULAR GAS OBSERVATIONS

ASTROPHYSICAL JOURNAL 833:1 (2016) ARTN 53

Authors:

A Seko, K Ohta, K Yabe, B Hatsukade, M Akiyama, N Tamura, F Iwamuro, G Dalton

Constraint on the inflow/outflow rates in star-forming galaxies at z~1.4 from molecular gas observations

(2016)

Authors:

Akifumi Seko, Kouji Ohta, Kiyoto Yabe, Bunyo Hatsukade, Masayuki Akiyama, Naoyuki Tamura, Fumihide Iwamuro, Gavin Dalton

Developing an integrated concept for the E-ELT Multi-Object Spectrograph (MOSAIC): design issues and trade-offs

(2016)

Authors:

Myriam Rodrigues, Gavin Dalton, Ewan Fitzsimons, Fanny Chemla, Tim Morris, Francois Hammer, Mathieu Puech, Christopher Evans, Pascal Jagourel

Pagination

  • First page First
  • Previous page Prev
  • …
  • Page 11
  • Page 12
  • Page 13
  • Page 14
  • Current page 15
  • Page 16
  • Page 17
  • Page 18
  • Page 19
  • …
  • Next page Next
  • Last page Last

Footer 91探花

  • Contact us
  • Giving to the Dept of Physics
  • Work with us
  • Media

User account menu

  • Log in

Follow us

FIND US

Clarendon Laboratory,

Parks Road,

91探花,

OX1 3PU

CONTACT US

Tel: +44(0)1865272200

Department Of Physics text logo

漏 91探花 - Department of Physics

Cookies | Privacy policy | Accessibility statement

  • Home
  • Research
  • Study
  • Engage
  • Our people
  • News & Comment
  • Events
  • Our facilities & services
  • About us
  • Giving to Physics