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

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

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.

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

SWIFT Image Slicer: large format, compact, low-scatter image slicing - art. no. 62732L

P SOC PHOTO-OPT INS 6273 (2006) L2732-L2732

Authors:

M Tecza, N Thatte, F Clarke, T Goodsall, D Freeman, Y Salaun

Abstract:

We present the SWIFT image slicer and its novel de-magnifying design. It is based on the MPE-3D and SPIFFI image slicers, uses plane mirrors to slice the input field, but achieves a considerable de-magnification through the use of a mosaic of spherical lenses. As only plane and spherical surfaces are used in the design, classical polishing techniques can be applied to achieve very high surface accuracy and quality. This reduces aberrations and scattered light, mandatory for an image slicer working at optical wavelengths and behind an adaptive optics system. Except for the lens mosaic, the SWIFT slicer is built entirely from Zerodur and is assembled using optical contacting. We present a detailed description of the design as well as results of the early stages of its fabrication.