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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 clustering and evolution of H-alpha emitters at z~1 from HiZELS

(2009)

Authors:

David Sobral, Philip N Best, James E Geach, Ian Smail, Michele Cirasuolo, Timothy Garn, Gavin B Dalton, Jaron Kurk
More details from the publisher

The HiZELS/UKIRT large area survey for bright Lyman-alpha emitters at z~9

(2009)

Authors:

David Sobral, Philip Best, Jim Geach, Ian Smail, Jaron Kurk, Michele Cirasuolo, Mark Casali, Rob Ivison, Kristen Coppin, Gavin Dalton
More details from the publisher

Obscured star formation at z = 0.84 with HiZELS: the relationship between star formation rate and H-alpha or ultra-violet dust extinction

(2009)

Authors:

Timothy Garn, David Sobral, Philip N Best, James E Geach, Ian Smail, Michele Cirasuolo, Gavin B Dalton, James S Dunlop, Ross J McLure, Duncan Farrah
More details from the publisher

The Herschel ATLAS

(2009)

Authors:

S Eales, L Dunne, D Clements, A Cooray, G De Zotti, S Dye, R Ivison, M Jarvis, G Lagache, S Maddox, M Negrello, S Serjeant, MA Thompson, E Van Kampen, A Amblard, P Andreani, M Baes, A Beelen, GJ Bendo, D Benford, F Bertoldi, J Bock, D Bonfield, A Boselli, C Bridge, V Buat, D Burgarella, R Carlberg, A Cava, P Chanial, S Charlot, N Christopher, P Coles, L Cortese, A Dariush, E Da Cunha, G Dalton, L Danese, H Dannerbauer, S Driver, J Dunlop, L Fan, D Farrah, D Frayer, C Frenk, J Geach, J Gardner, H Gomez, J Gonzalez-Nuevo, E Gonzalez-Solares, M Griffin, M Hardcastle, E Hatziminaoglou, D Herranz, D Hughes, E Ibar, Woong-Seob Jeong, C Lacey, A Lapi, M Lee, L Leeuw, J Liske, M Lopez-Caniego, T Muller, K Nandra, P Panuzzo, A Papageorgiou, G Patanchon, J Peacock, C Pearson, S Phillipps, M Pohlen, C Popescu, S Rawlings, E Rigby, M Rigopoulou, G Rodighiero, A Sansom, B Schulz, D Scott, DJB Smith, B Sibthorpe, I Smail, J Stevens, W Sutherland, T Takeuchi, J Tedds, P Temi, R Tuffs, M Trichas, M Vaccari, I Valtchanov, P Van der Werf, A Verma, J Vieria, C Vlahakis, Glenn J White
More details from the publisher

Bright Lyman-alpha Emitters at z~9: constraints on the luminosity function from HiZELS

Monthly Notices of the Royal Astronomical Society: Letters Blackwell Publishing (2009)

Authors:

D Sobral, PN Best, JE Geach, I Smail, J Kurk, M Cirasuolo, M Casali, RJ Ivison, K Coppin, GB Dalton

Abstract:

New results are presented, as part of the Hi-z Emission Line Survey (HiZELS), from the largest area survey to date (1.4 sq.deg) for Lyman-alpha emitters (LAEs) at z~9. The survey, which is primarily targeting H-alpha emitters at z<3, uses the Wide Field CAMera on the United Kingdom Infrared Telescope and a custom narrow-band filter in the J band and reaches a Lyman-alpha luminosity limit of ~10^43.8 erg/s over a co-moving volume of 1.12x10^6 Mpc^3 at z=8.96+-0.06. Only 2 candidates were found out of 1517 line emitters and those were rejected as LAEs after follow-up observations. The limit on the space density of bright LAEs is improved by 3 orders of magnitude, consistent with suppression of the bright end of the Lyman-alpha luminosity function beyond z~6. Combined with upper limits from smaller but deeper surveys, this rules out some of the most extreme models for high-redshift LAEs. The potential contamination of future narrow-band Lyman-alpha surveys at z>7 by Galactic brown dwarf stars is also examined, leading to the conclusion that such contamination may well be significant for searches at 7.7
Details from ArXiV
More details from the publisher

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