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The University of Sydney is the oldest university in Australia. It was established in Sydney in 1850. It is a member of Australia's "Group of Eight" universities that are highly ranked in terms of their research performance. In 2009, the university had 47,775 students making it the second largest (behind Monash University) in Australia.
More information: http://en.wikipedia.org/wiki/University_of_Sydney
Trade Practices Act and other matters Module 4
Winter Session 2008
Trade Practices Act and other matters Module 4 Winter Session 2008 |
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PSYCHOMETRIC TESTING AT NAB Stephanie Christopher – SHL
Anna Heywood - NAB
PSYCHOMETRIC TESTING AT NAB Stephanie Christopher – SHL Anna Heywood - NAB |
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Hypothesis testing Week 10 Lecture 2
Hypothesis testing Week 10 Lecture 2 |
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Mortgages Cameron Stewart (thanks to Shae McCrystal and Jim Helman)
Mortgages Cameron Stewart (thanks to Shae McCrystal and Jim Helman) |
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Commercial Transactions Module 5-performance and remedies
Winter Session 2010
Commercial Transactions Module 5-performance and remedies Winter Session 20100 |
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Olympiad Training Oscillations & Waves
Olympiad Training Oscillations & Waves |
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Lifelong ambient companions: challenges and steps to overcome them Judy Kay
CHAI: Computer human adapted interaction research group
School of Information Technologies
Lifelong ambient companions: challenges and steps to overcome them Judy Kay CHAI: Computer human adapted interaction research group School of Information Technologies |
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Qualitative Research in Information Technology Liaquat Hossain
School of IT
The University of Sydney
Qualitative Research in Information Technology Liaquat Hossain School of IT The University of Sydney |
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LAW OF TORTS LECTURE 3
Intentional torts to Chattels
Action on the case for Wilful Injury
Defences to Intentional Torts
Greg Young greg.young@lawyer.com
LAW OF TORTS LECTURE 3 Intentional torts to Chattels Action on the case for Wilful Injury Defences to Intentional Torts Greg Young greg.young@lawyer.com |
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Express in Scientific notation
Express in Scientific notationA thousand billionth of a lo 1 thousandth of a pede A billion lo s 1 million n’s |
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Radio-mode feedback in Radio-loud AGN
Radio-mode feedback in Radio-loud AGNBEL - face-on AGN? cold accretion? Abs - hot accretion? NEL - obscured AGN? cold accretion? Figure 1. Colour – redshift plot of radio-loud galaxies and showing where the different populations of radio-loud AGN may lie. Is this figure caused by an evolutionary sequence of radio-loud AGN?? John H. Y. CHING1, Scott Croom1,Elaine Sadler1, 1Sydney Institute for Astronomy, School of Physics, The University of Sydney Andrew Hopkins1 and Helen Johnston1 3. What’s New? A sample of flux-limited radio galaxies has been selected by cross-matching the Faint Images of the Radio Sky at Twenty-Centimeters (FIRST) catalogue with the Sloan Digital Sky Survey (SDSS) photometric catalogue for galaxies within the Galaxy and Mass Assembly (GAMA), WiggleZ, and 2df-SDSS LRG and QSO (2SLAQ) survey regions. Spare-fibres from the GAMA and WiggleZ surveys will allow us to measure the redshifts for those in the sample which have poor or no SDSS spectroscopic redshifts. Covering these large survey regions serves two purposes: 1. it provides us with a parent sample in the same field so we have enough nearby sources to determine the local environment. 2. it provides a large enough redshift range (0.0 < z < 1.1, Figure 2) to measure evolution over almost half the age of the Universe. 4. What I’m Doing? In order to address the questions raised in Figure 1, I will look be looking at the correlation between spectral type and environment, as well as comparing star formation rates. These tests will compare g... |
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Chapter 4: Forces and Motion
Chapter 4: Forces and Motion |
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