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Galaxy clusters at 0.6 < z < 1.4 in the UKIDSS Ultra Deep Survey Early Data Release

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 373:1 (2006) L26-L30

Authors:

C van Breukelen, L Clewley, DG Bonfield, S Rawlings, MJ Jarvis, JM Barr, S Foucaud, O Almaini, M Cirasuolo, G Dalton, JS Dunlop, AC Edge, P Hirst, RJ McLure, MJ Page, K Sekiguchi, C Simpson, I Smail, MG Watson
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Late-type galaxies observed with SAURON:: two-dimensional stellar and emission-line kinematics of 18 spirals

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 367:1 (2006) 46-78

Authors:

K Ganda, J Falcón-Barroso, RF Peletier, M Cappellari, E Emsellem, RM McDermid, PT de Zeeuw, CM Carollo, DR Andersen, RA Swaters
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NGC 7679: an anomalous, composite Seyfert 1 galaxy whose X-ray luminous AGN vanishes at optical wavelengths

ASTRONOMY & ASTROPHYSICS 447:2 (2006) 441-451

Authors:

LM Buson, M Cappellari, EM Corsini, EV Held, J Lim, A Pizzella
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Opto-mechanical design of the KMOS spectrograph module - art. no. 62694G

P SOC PHOTO-OPT INS 6269 (2006) G2694-G2694

Authors:

M Tecza, IJ Lewis, J Lynn, S Yang, NA Thatte, IAJ Tosh, MJ Ferlet

Abstract:

We present the optical and mechanical design of the KMOS spectrograph module together with a detailed analysis of its performance. KMOS is a cryogenic near-infrared multi-object spectrograph being developed as a second-generation instrument for the VLT by a consortium of UK and German institutes. Three identical spectrograph modules provide Nyquist sampled spectra in the wavelength range covering the atmospheric bands z, J, H, and K with a resolving power exceeding 3200. The spectrographs are fully achromatic over the bands and the single mirror collimator and six-element camera, together with six high efficiency gratings provide high throughput. The optical performance analysis includes amongst others the spectral resolving power and variation of the PSF as a function of the pupil illumination.
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Probing the low-luminosity X-ray luminosity function in normal elliptical galaxies

ASTROPHYSICAL JOURNAL 652:2 (2006) 1090-1096

Authors:

D-W Kim, G Fabbiano, V Kalogera, AR King, S Pellegrini, G Trinchieri, SE Zepf, A Zezas, L Angelini, RL Davies, JS Gallagher
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