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Jy. These observations have been interpreted as a function of evolution by Seymour et al. They embody both star-forming galaxies, which roughly follow the correlation found by Appleton et al., and AGN, which prolong to the top of the plot. Also shown are the stacked data from Boyle et al. 2008). To explore the correlation at even fainter levels, Boyle et al. 2007) stacked ATLAS radio knowledge to indicate that it extends right down to microJy levels. Further exploration has found that this similar consequence can be reproduced by stacking information from the FLS (Norris et al. 0.Eight discovered by Appleton et al.

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Appleton, P. N., et al. 1998, AJ, 115, 1693 de Jong T., Klein,U., Wielebinski,R., Wunderlich,E.,1985, AA, 147, 6 Ekers R. D., Goss W. M., Kotanyi C. G., & Skellern D. J., 1978, A&A, 69, L21 Garn, T., & Alexander, P. 2008, MNRAS, 391, a thousand Jarvis, M. J. 2008, arXiv:0801.4618 Johnston, S., et al. 2004, ApJS, 154, 147 Beswick, R. J., et al., 2008, MNRAS, 385, 1143 Boyle, B., et al., 2007, MNRAS, 376, 1182B Condon, J. J., et al.

ATLAS (Australia Telescope Massive Space Survey) is a wide deep radio survey which is distinguished by its comprehensive multi-wavelength strategy. These and different observations recommend that the AGN activity and star formation develop into increasingly inter-dependent at high redshifts. ATLAS is creating a large dataset of radio-chosen galaxies for studying the evolution and inter-relationship of star-forming and lively galaxies. Radio surveys, once a niche element of those research, are becoming increasingly necessary due to their increasing sensitivity, because they entry giant fields of view, because they are unaffected by dust, and since they’ll detect active galactic nuclei (AGN) as much as the best redshifts. Multiwavelength deep extensive surveys are a key tool for finding out galaxy evolution.

Jy rms. The main science objectives of ATLAS are to help determine how galaxies evolved by means of cosmic time, and help decide the connection between star formation and large black holes. As a result, the ATLAS radio data are accompanied by intensive infrared, and optical knowledge. 2003), around the CDFS and ELAIS-S1 regions, and include the goods and ECDFS areas. The area surveyed by ATLAS has been chosen to overlap that noticed by the Spitzer Wide-area Infrared Extragalactic Survey (SWIRE) program (Lonsdale et al. The facility of deep radio surveys can only be realised by corresponding data at different wavelengths.