Hintze Centre for Astrophysical Surveys

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Short-Term Radio-X-ray Correlations of Cygnus X-1

(2003)

Authors:

T Gleissner, J Wilms, GG Pooley, MA Nowak, K Pottschmidt, S Markoff, M Klein-Wolt, RP Fender, R Staubert
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The detailed optical light curve of GRB 030329

(2003)

Authors:

YM Lipkin, EO Ofek, A Gal-Yam, EM Leibowitz, D Poznanski, S Kaspi, D Polishook, SR Kulkarni, DW Fox, E Berger, N Mirabal, J Halpern, M Bureau, K Fathi, PA Price, BA Peterson, A Frebel, B Schmidt, JA Orosz, JB Fitzgerald, JS Bloom, PG van Dokkum, CD Bailyn, MM Buxton, M Barsony
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A Search for Short Time-Scale Optical Variability in the GRB 030329 Afterglow

(2003)

Authors:

N Mirabal, JP Halpern, M Bureau, K Fathi
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SAURON: Observations of E/S0/SA galaxies

Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias 17 (2003) 199

Authors:

H Kuntschner, R Bacon, M Bureau, M Cappellari, Y Copin, RL Davies, E Emsellem, BW Miller, R McDermid, RF Peletier, EK Verolme, PT De Zeeuw

Abstract:

We present results from a new and unique integral-field spectrograph, SAURON. It has a large field of view and high throughput and is primarily built for the study of stellar & gaseous kinematics and stellar populations in galaxies. Its aim is to carry out a systematic survey of the velocity fields, velocity dispersions, and line-strength distributions of nearby ellipticals, lenticular galaxies and spiral bulges.
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Stellar astrophysics in the local group and beyond with the GTC

Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias 16 (2003) 145-149

Abstract:

In this review I discuss the capabilities that the GTC, and in particular the OSIRIS spectrometer, will bring to studying massive stellar populations within Local Group galaxies and even beyond. By observing massive stars in other dwarf irregular and spiral galaxies one can probe star formation and stellar evolution in extreme environments, the wind properties of massive luminous stars, and determine distances to an accuracy of ∼10%.