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CLOVER: The CMB Polarization Observer

EAS Publications Series EDP Sciences 14 (2005) 251-256

Authors:

B Maffei, PAR Ade, C Calderon, AD Challinor, P De Bernardis, L Dunlop, WK Gear, Y Giraud-Héraud, DJ Goldie, KJB Grainge, KG Isaak, B Johnson, ME Jones, AN Lasenby, PD Mauskopf, SJ Melhuish, A Orlando, L Piccirillo, G Pisano, AC Taylor, S Withington, G Yassin
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The 2dF QSO Redshift Survey - XIV. Structure and evolution from the two-point correlation function

Monthly Notices of the Royal Astronomical Society 356 (2005) 415-438

Authors:

L Miller, Boyle, B.J., Croom, S.M., Shanks, T.
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The SCUBA half-degree extragalactic survey -: I.: Survey motivation, design and data processing

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 363:2 (2005) 563-580

Authors:

AMJ Mortier, S Serjeant, JS Dunlop, SE Scott, P Ade, D Alexander, O Almaini, I Aretxaga, C Baugh, AJ Benson, PN Best, A Blain, J Bock, C Borys, A Bressan, C Carilli, EL Chapin, S Chapman, DL Clements, K Coppin, M Crawford, M Devlin, S Dicker, L Dunne, SA Eales, AC Edge, D Farrah, M Fox, C Frenk, E Gaztañaga, WK Gear, E Gonzales-Solares, GL Granato, TR Greve, JA Grimes, J Gundersen, M Halpern, P Hargrave, DH Hughes, RJ Ivison, MJ Jarvis, T Jenness, R Jimenez, E van Kampen, A King, C Lacey, A Lawrence, K Lepage, RG Mann, G Marsden, P Mauskopf, B Netterfield, S Oliver, L Olmi, MJ Page, JA Peacock, CP Pearson, WJ Percival, A Pope, RS Priddey, S Rawlings, N Roche, MR Robinson, D Scott, K Sekiguchi, M Seigar, L Silva, C Simpson, I Smail, JA Stevens, T Takagi, G Tucker, C Vlahakis, I Waddington, J Wagg, M Watson, C Willott, M Vaccari
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Towards simulating star formation in the interstellar medium

Monthly Notices of the Royal Astronomical Society 356 (2005) 737-752

Authors:

AD Slyz, Julien Devriendt, Greg Bryan, Joseph Silk
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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

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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