Extremely Large Telescope

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3D: The new near-infrared field imaging spectrometer

IAU SYMP (1995) 373-373

Authors:

LE TacconiGarman, L Weitzel, M Cameron, S Drapatz, R Genzel, A Krabbe, H Kroker, N Thatte
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AN ULTRAVIOLET FLARE AT THE CENTER OF THE ELLIPTIC GALAXY NGC4552

NATURE 378:6552 (1995) 39-41

Authors:

A RENZINI, L GREGGIO, SD ALIGHIERI, M CAPPELLARI, D BURSTEIN, F BERTOLA
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Automated tuning of the Berkeley-Illinois-Maryland array receivers

P SOC PHOTO-OPT INS 2479 (1995) 289-300

Authors:

N THATTE, RL PLAMBECK, JB LUGTEN, W HOFFMAN, L URRY, D THORNTON, WJ WELCH
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ROGUE - The Rapid Off-axis GUider Experiment

P SOC PHOTO-OPT INS 2475 (1995) 228-235

Authors:

N THATTE, H KROKER, L WEITZEL, LE TACCONIGARMAN, M TECZA, A KRABBE, R GENZEL
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The APM cluster survey: Cluster detection and large-scale structure

MORIOND AST (1995) 249-252

Abstract:

The APM Cluster Survey was based on a modification of Abell's original classification scheme for galaxy clusters. Here we discuss the results of an investigation of the stability of the statistical properties of the cluster catalogue to changes in the selection parameters. For a poor choice of selection parameters we find clear indications of line-of-sight clusters, but there is a wide range of input parameters for which the statistical properties of the catalogue are stable. We conclude that clusters selected in this way are indeed useful as tracers of large-scale structure.
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