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Jy. These observations have been interpreted as a perform of evolution by Seymour et al. They include both star-forming galaxies, which roughly observe the correlation found by Appleton et al., and AGN, which prolong to the highest of the plot. Additionally shown are the stacked information from Boyle et al. 2008). To explore the correlation at even fainter ranges, Boyle et al. 2007) stacked ATLAS radio information to point out that it extends right down to microJy levels. Additional exploration has found that this same consequence could be reproduced by stacking knowledge from the FLS (Norris et al. 0.8 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, one 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.
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ATLAS (Australia Telescope Giant Area Survey) is a wide deep radio survey which is distinguished by its complete multi-wavelength strategy. These and different observations counsel that the AGN activity and star formation change into increasingly inter-dependent at high redshifts. ATLAS is creating a large dataset of radio-selected galaxies for studying the evolution and inter-relationship of star-forming and active galaxies. Radio surveys, as soon as a distinct segment component of those studies, are becoming more and more necessary because of their rising sensitivity, as a result of they access giant fields of view, as a result of they are unaffected by mud, and because they can detect energetic galactic nuclei (AGN) up to the best redshifts. Multiwavelength deep extensive surveys are a key instrument for learning galaxy evolution.
Jy rms. The main science objectives of ATLAS are to help determine how galaxies evolved by cosmic time, and help determine the relationship between star formation and large black holes. Consequently, the ATLAS radio knowledge are accompanied by intensive infrared, and optical knowledge. 2003), around the CDFS and ELAIS-S1 areas, and embody the products and ECDFS regions. The world surveyed by ATLAS has been chosen to overlap that noticed by the Spitzer Extensive-space Infrared Extragalactic Survey (SWIRE) program (Lonsdale et al. The facility of deep radio surveys can solely be realised by corresponding information at different wavelengths.