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The 2dF Galaxy Redshift Survey: stochastic relative biasing between galaxy populations

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 356:1 (2005) 247-269

Authors:

V Wild, JA Peacock, O Lahav, E Conway, S Maddox, IK Baldry, CM Baugh, J Bland-Hawthorn, T Bridges, R Cannon, S Cole, M Colless, C Collins, W Couch, G Dalton, R De Propris, SP Driver, G Efstathiou, RS Ellis, CS Frenk, K Glazebrook, C Jackson, I Lewis, S Lumsden, D Madgwick, P Norberg, BA Peterson, W Sutherland, K Taylor
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The 2dF Galaxy Redshift Survey: luminosity functions by density environment and galaxy type

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 356:3 (2005) 1155-1167

Authors:

DJ Croton, GR Farrar, P Norberg, M Colless, JA Peacock, IK Baldry, CM Baugh, J Bland-Hawthorn, T Bridges, R Cannon, S Cole, C Collins, W Couch, G Dalton, R De Propris, SP Driver, G Efstathiou, RS Ellis, CS Frenk, K Glazebrook, C Jackson, O Lahav, I Lewis, S Lumsden, S Maddox, D Madgwick, BA Peterson, W Sutherland, K Taylor
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The [O II]λ3727/Hα ratio of emission-line galaxies in the 2dF galaxy redshift survey

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 362:4 (2005) 1143-1156

Authors:

M Mouhcine, I Lewis, B Jones, F Lamareille, SJ Maddox, T Contini
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Novel coating and photo-fabrication techniques for astronomy

Proceedings of SPIE - The International Society for Optical Engineering 5494 (2004) 562-565

Authors:

IJ Lewis, GB Dalton, C Band, C Goodwin, D Bonfield

Abstract:

In this paper we describe two coating and fabrication techniques we have developed applicable to astronomical instrumentation with particular emphasis on the FMOS instrument for the Subaru telescope.
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KMOS: An infrared multiple object integral field spectrograph for the ESO VLT

Proceedings of SPIE - The International Society for Optical Engineering 5492:PART 3 (2004) 1179-1186

Authors:

RM Sharples, R Bender, M Lehnert, SKR Howat, MN Bremer, RL Davies, R Genzel, R Hofmann, RJ Ivison, R Saglia, NA Thatte

Abstract:

We describe the design of a 2nd generation instrument for the ESO VLT which will deliver a unique multiple deployable integral field capability in the near-infrared (1-2.5μm). The science drivers for the instrument are presented and linked to the functional specification. The baseline instrument concept is described with emphasis on technological innovations. Detailed discussions of specific technologies, and ongoing prototype studies, are described in separate papers.
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