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Long-term Monitoring with Small and Medium-sized Telescopes on the Ground and in Space

Published online by Cambridge University Press:  20 April 2012

P. A. Charles
Affiliation:
School of Physics & Astronomy, University of Southampton, Southampton, UK email: [email protected] South African Astronomical Observatory, Observatory 7935, South Africa Department of Astronomy, University of Cape Town, Cape Town, South Africa
M. M. Kotze
Affiliation:
South African Astronomical Observatory, Observatory 7935, South Africa Department of Astronomy, University of Cape Town, Cape Town, South Africa
A. Rajoelimanana
Affiliation:
South African Astronomical Observatory, Observatory 7935, South Africa Department of Astronomy, University of Cape Town, Cape Town, South Africa
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Abstract

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The last 20 years have seen revolutionary developments of large-scale synoptic surveys of the sky, both from the ground (e.g., the MACHO and OGLE projects, which were targetted at micro-lensing studies) and in space (e.g., the X-ray All-Sky Monitor onboard RXTE). These utilised small and medium-sized telescopes to search for transient-like events, but they have now built up a huge database of long-term light-curves, thereby enabling archival research on a wide range of objects that has not been possible hitherto. This is illustrated with examples of long time-scale optical and X-ray variability studies from the field of X-ray binary research: the high-mass BeX binaries in the SMC (using MACHO and OGLE), and the bright galactic-bulge X-ray sources (mostly LMXBs, using RXTE/ASM). As such facilities develop greater capabilities in future and at other wavelengths (developments in South Africa will be described), real-time data processing will allow much more rapid follow-up studies with the new generation of queue-scheduled large telescopes such as SALT.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2012

References

Alcock, C., et al. , 1996, ApJ, 461, 84CrossRefGoogle Scholar
Applegate, J. H. & Patterson, J. 1987, ApJ, 322, L99CrossRefGoogle Scholar
Charles, P., Kotze, M., & Rajoelimanana, A. 2010, AIP Conf. Series, 1314, 303Google Scholar
Charles, P. 2011, in: Lasota, J.-P. (ed.), Astronomy at the Frontiers of Science (Dordrecht: Springer), p. 209Google Scholar
Clarkson, W. I., et al. , 2003 MNRAS, 339, 447Google Scholar
Coe, M. J. 2000, ASP Conf. Series, 214, 656Google Scholar
Glass, I. S. & Nagata, T. 2000, MNASSA, 59, 110Google Scholar
Harris, R. J., et al. , 2009 ApJ, 696, 1987CrossRefGoogle Scholar
Hessman, F. V. 2001, ASP Conf.Series, 246, 13Google Scholar
Kato, D., et al. , 2007, PASJ, 59, 615CrossRefGoogle Scholar
Kim, S.-L., et al. , 2010, SPIE, 7733, 107Google Scholar
Kotze, M. M. & Charles, P. A. 2010, MNRAS, 402, L16CrossRefGoogle Scholar
Kotze, M. M. & Charles, P. A. 2011, MNRAS, onlineGoogle Scholar
Kuhn, R., et al. , 2010, BAAS, 42, 288Google Scholar
Levine, A.M., et al. , 1996, ApJ, 469, L33CrossRefGoogle Scholar
McGowan, K. E. & Charles, P. A. 2003, MNRAS, 339, 748CrossRefGoogle Scholar
Ogilvie, G. I. & Dubus, G. 2001, MNRAS, 320, 485CrossRefGoogle Scholar
Rajoelimanana, A. F., Charles, P. A., & Udalski, A. 2011, MNRAS, 413, 1600CrossRefGoogle Scholar
Reig, P. 2011, Ap.Sp.Sci., 332, 1CrossRefGoogle Scholar
Shporer, A., et al. , 2011, in: Sozzetti, A., Lattanzi, M. G. & Boss, A. P. (eds.), The Astrophysics of Planetary Systems, IAU Symp. 276, Cambridge, UK: Cambridge University Press, p. 553Google Scholar
Skelton, P. 2010, in: Basson, I. & Botha, A. E. (eds.), Modelling of Eclipsing Binaries, 55th SAIP Ann. Conf., (Pretoria: CSIR)Google Scholar
Smith, A. M. S., et al. , 2009, MNRAS, 398, 1827CrossRefGoogle Scholar
Udalski, A., Kubiak, M., & Szymanski, M. 1997, Acta Ast., 47, 319Google Scholar