8,310 research outputs found
Near-Infrared K and L' Flux Ratios in Six Lensed Quasars
We examine the wavelength dependence of flux ratios for six gravitationally
lensed quasars using K and L' images obtained at the Gemini North 8m telescope.
We select lenses with source redshifts z_s < 2.8 so that K-band images probe
rest-frame optical emission from accretion disks, while L'-band images probe
rest-frame near-infrared flux emitted (in part) from the more extended
surrounding torus. Since the observations correspond to different source sizes,
the K and L' flux ratios are sensitive to structure on different scales and may
be useful for studying small-structure in the lens galaxies. Four of the six
lenses show differences between K and L' flux ratios. In HE 0435$-1223, SDSS
0246-0825, and HE 2149-2745 the differences may be attributable to known
microlensing and/or intrinsic variability. In SDSS 0806+2006 the wavelength
dependence is not easily attributed to known variations, and may indicate the
presence of substructure. By contrast, in Q0142-100 and SBS 0909+523 the K and
L' flux ratios are consistent within the uncertainties. We discuss the utility
of the current data for studying chromatic effects related to microlensing,
dust extinction, and dark matter substructure.Comment: 19 pages, 4 Figures, 4 Tables, AJ accepte
The HST Survey of BL Lac Objects: Gravitational Lens Candidates and Other Unusual Sources
We present HST observations of seven unusual objects from the HST ``snapshot
survey'' of BL Lac objects, of which four are gravitational lens candidates. In
three cases a double point sources is observed: 0033+595, with 1.58 arcsec
separation, and 0502+675 and 1440+122, each with arcsec separation.
The last two also show one or more galaxies, which could be either host or
lensing galaxies. If any are confirmed as lenses, these BL Lac objects are
excellent candidates for measuring H via gravitational time delay because
of their characteristic rapid, high amplitude variability. An additional
advantage is that, like other blazars, they are likely superluminal radio
sources, in which case the source plane is mapped out over a period of years,
providing strong additional constraints on the lensing mass distribution. The
fourth gravitational lens candidate is 1517+656, which is surrounded by three
arclets forming an almost perfect ring of radius 2.4 arcsec. If this is indeed
an Einstein ring, it is most likely a background source gravitationally lensed
by the BL Lac object host galaxy and possibly a surrounding group or cluster.
In the extreme case that all four candidates are true lenses, the derived
frequency of gravitational lensing in this BL Lac sample would be an order of
magnitude higher than in comparable quasar samples.
We also report on three other remarkable BL Lac objects: 0138-097, which is
surrounded by a large number of close companion galaxies; 0806+524, whose host
galaxy contains an uncommon arc-like structure; and 1959+650, which is hosted
by a gas rich elliptical galaxy with a prominent dust lane of .Comment: 29 pages in total, 12 figure
Performance evaluation of NASA/KSC CAD/CAE graphics local area network
This study had as an objective the performance evaluation of the existing CAD/CAE graphics network at NASA/KSC. This evaluation will also aid in projecting planned expansions, such as the Space Station project on the existing CAD/CAE network. The objectives were achieved by collecting packet traffic on the various integrated sub-networks. This included items, such as total number of packets on the various subnetworks, source/destination of packets, percent utilization of network capacity, peak traffic rates, and packet size distribution. The NASA/KSC LAN was stressed to determine the useable bandwidth of the Ethernet network and an average design station workload was used to project the increased traffic on the existing network and the planned T1 link. This performance evaluation of the network will aid the NASA/KSC network managers in planning for the integration of future workload requirements into the existing network
Evolutionary modelling in economics: a survey of methods and building blocks
In this paper we present an overview of methods and components of formal economic models employing evolutionary approaches. This compromises two levels: (1) techniques of evolutionary modelling, including multi-agent modelling, evolutionary algorithms and evolutionary game theory; (2) building blocks or components of formal models classified into core processes and features of evolutionary systems - diversity, innovation and selection - and additional elements, such as bounded rationality, diffusion, path dependency and lock-in, co-evolutionary dynamics, multilevel and group selection, and evolutionary growth. We focus our attention on the characteristics of models and techniques and their underlying assumptions
Automated computation of scattering amplitudes
We review some of the recent advances in the computation of one-loop
scattering amplitudes which led to the construction of efficient and automated
computational tools for NLO predictions. Particular attention is devoted to
unitarity-based methods and integrand-level reduction techniques. Extensions of
one-loop integrand-level techniques to higher orders are also briefly
illustrated.Comment: 13 pages, v2: references corrected. Presented at the "International
Workshop on Advanced Computing and Analysis Techniques in Physics Research"
(ACAT2013), Beijing, China, May 201
ERA distribution of information systems journals
The Excellence in Research for Australia (ERA) initiative being conducted by the Australian Research Council (ARC), mandates a single journal and conference ranking scheme over every academic discipline in Australia. A universal publication outlet ranking list mandated by a government agency is unique and has attracted interest and comment both within Australia and overseas. Equally, the interest shown has come from all sectors involved in academic publishing – authors, reviewers, publishers – and from commercial and open access publishers. This paper investigates the distribution of information systems journals over the various ERA parameters and comments on a claim of bias whereby the ranking of a journal is positively influenced by the number of years it has been in existence in the areas of information systems and business journals. Clear evidence of the diversity of the information systems discipline is observed. The benefits of a multidisciplinary foundation for information systems is also noted. Longer established journals are shown to attract higher rankings and possible reasons for and implications flowing from this are discussed.<br /
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