Institution
Swinburne University of Technology
Education•Melbourne, Victoria, Australia•
About: Swinburne University of Technology is a education organization based out in Melbourne, Victoria, Australia. It is known for research contribution in the topics: Galaxy & Population. The organization has 7223 authors who have published 25530 publications receiving 667955 citations. The organization is also known as: Swinburne Technical College & Swinburne College of Technology.
Topics: Galaxy, Population, Redshift, Star formation, Context (language use)
Papers published on a yearly basis
Papers
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University of Western Australia1, University of St Andrews2, Swinburne University of Technology3, Ames Research Center4, Liverpool John Moores University5, University of Nottingham6, University of Sydney7, Australian Astronomical Observatory8, University of Cape Town9, University of Hertfordshire10, University of Oxford11, University of Sussex12, Durham University13, University of Bristol14, University of Melbourne15
TL;DR: In this article, the authors used data from the Galaxy And Mass Assembly (GAMA) survey in the redshift range 0.01 < z < 0.1 (8399 galaxies in g to Ks bands) to derive the stellar mass-half-light radius relations for various divisions of early and late-type samples.
Abstract: We use data from the Galaxy And Mass Assembly (GAMA) survey in the redshift range 0.01 < z < 0.1 (8399 galaxies in g to Ks bands) to derive the stellar mass–half-light radius relations for various divisions of ‘early’- and ‘late’-type samples. We find that the choice of division between early and late (i.e. colour, shape, morphology) is not particularly critical; however, the adopted mass limits and sample selections (i.e. the careful rejection of outliers and use of robust fitting methods) are important. In particular, we note that for samples extending to low stellar mass limits (<1010M⊙) the Sersic index bimodality, evident for high-mass systems, becomes less distinct and no-longer acts as a reliable separator of early- and late-type systems. The final set of stellar mass–half-light radius relations are reported for a variety of galaxy population subsets in 10 bands (ugrizZY JHKs) and are intended to provide a comprehensive low-z benchmark for the many ongoing high-z studies. Exploring the variation of the stellar mass–half-light radius relations with wavelength, we confirm earlier findings that galaxies appear more compact at longer wavelengths albeit at a smaller level than previously noted: at 1010M⊙ both spiral systems and ellipticals show a decrease in size of 13 per cent from g to Ks (which is near linear in log wavelength). Finally, we note that the sizes used in this work are derived from 2D Sersic light profile fitting (using GALFIT3), i.e. elliptical semimajor half-light radii, improving on earlier low-z benchmarks based on circular apertures.
216 citations
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TL;DR: Three-dimensional (3D) micro/nano-structuring of photo-resists is systematically studied at the close-to-dielectric- breakdown irradiance and it is demonstrated that avalanche absorption is playing a major part in free electron generation and chemical bond breaking at these conditions.
Abstract: Three-dimensional (3D) micro/nano-structuring of photo-resists is systematically studied at the close-to-dielectric-breakdown irradiance. It is demonstrated that avalanche absorption is playing a major part in free electron generation and chemical bond breaking at these conditions. The steps of photo-initiation and chemical bond breaking in propagation of polymerization are altered as compared with photo-polymerization at low-irradiance and one-photon stereo-lithography. The avalanche dominates radical generation and promotion of polymerization at tight focusing and a high ~TW/cm2 irradiance. The rates of electron generation by two-photon absorption and avalanche are calculated for the experimental conditions. Simulation results are corroborated by 3D polymerization in three resists with different photo-initiators at two different wavelengths and pulse durations. The smallest feature sizes of 3D polymerized logpile structures are consistent with spectral dependencies of the two photon nonlinearities. Implications of these findings for achieving sub-100 nm resolution in 3D structuring of photo-polymers are presented.
216 citations
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TL;DR: This survey paper looks at emerging research into the application of client-side, server- side, and in-network rate adaptation techniques to support DASH-based content delivery and provides context and motivation for the application.
Abstract: With companies such as Netflix and YouTube accounting for more than 50% of the peak download traffic on North American fixed networks in 2015, video streaming represents a significant source of Internet traffic. Multimedia delivery over the Internet has evolved rapidly over the past few years. The last decade has seen video streaming transitioning from User Datagram Protocol to Transmission Control Protocol-based technologies. Dynamic adaptive streaming over HTTP (DASH) has recently emerged as a standard for Internet video streaming. A range of rate adaptation mechanisms are proposed for DASH systems in order to deliver video quality that matches the throughput of dynamic network conditions for a richer user experience. This survey paper looks at emerging research into the application of client-side, server-side, and in-network rate adaptation techniques to support DASH-based content delivery. We provide context and motivation for the application of these techniques and review significant works in the literature from the past decade. These works are categorized according to the feedback signals used and the end-node that performs or assists with the adaptation. We also provide a review of several notable video traffic measurement and characterization studies and outline open research questions in the field.
216 citations
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TL;DR: A comprehensive Adolescent Risk-Taking Questionnaire (ARQ) was developed using reports of 570 adolescents and was psychometrically evaluated with a sample of 925 adolescents between 11 and 18 years of age as mentioned in this paper.
Abstract: Compared to other life periods, adolescence is characterized by a heightened potential for risky behaviors. This study reports the systematic development and psychometric evaluation of a comprehensive Adolescent Risk-Taking Questionnaire (ARQ). It was developed using reports of 570 adolescents and was psychometrically evaluated with a sample of 925 adolescents between 11 and 18 years of age. Principal components analyses yielded a four-factor risk structure, and these factors were substantiated via a confirmatory factor analysis. One week test-retest and internal consistency indices were demonstrated to be sound. Age and gender differences were found to be consistent with reported trends in accident data. Older adolescents and boys reported lower risk perceptions and a higher frequency of risky behaviors than younger adolescents and girls, respectively, supporting the validity of the ARQ. Furthermore, consistent with past research, perceiving higher levels of risk typically related to lower levels of enga...
215 citations
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TL;DR: In this paper, the dispersion of graphene oxide (GO) in simulated pore solution and cement paste was investigated, and it was found that severe GO aggregation occurred in presence of divalent calcium ions.
215 citations
Authors
Showing all 7390 results
Name | H-index | Papers | Citations |
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Ramachandran S. Vasan | 172 | 1100 | 138108 |
Karl Glazebrook | 132 | 613 | 80150 |
Neville Owen | 127 | 700 | 74166 |
Michael A. Kamm | 124 | 637 | 53606 |
Zidong Wang | 122 | 914 | 50717 |
Christos Pantelis | 120 | 723 | 56374 |
Warrick J. Couch | 109 | 410 | 63088 |
Gao Qing Lu | 108 | 546 | 53914 |
Paul Mulvaney | 106 | 397 | 45952 |
Alexa S. Beiser | 106 | 366 | 47457 |
A. Roodman | 105 | 1087 | 50599 |
Chris Power | 104 | 477 | 45321 |
Murray D. Esler | 104 | 469 | 41929 |
David Coward | 103 | 400 | 67118 |
Hung T. Nguyen | 102 | 1011 | 47693 |