Integrating adaptive user interface capabilities in enterprise applications

Many existing enterprise applications are at a mature stage in their development and are unable to easily benefit from the usability gains offered by adaptive user interfaces (UIs). Therefore, a method is needed for integrating adaptive UI capabilities into these systems without incurring a high cost or significantly disrupting the way they function. This paper presents a method for integrating adaptive UI behavior in enterprise applications based on CEDAR, a model-driven, service-oriented, and tool-supported architecture for devising adaptive enterprise application UIs. The proposed integration method is evaluated with a case study, which includes establishing and applying technical metrics to measure several of the method’s properties using the open-source enterprise application OFBiz as a test-case. The generality and flexibility of the integration method are also evaluated based on an interview and discussions with practitioners about their real-life projects

Potassium administration increases and potassium deprivation reduces urinary calcium excretion in healthy adults

Potassium administration increases and potassium deprivation reduces urinary calcium excretion in healthy adults. This study was undertaken to evaluate the effects of dietary K intake, independent of whether the accompanying anion is Cl- or HCO3-, on urinary Ca excretion in healthy adults. The effects of KCl, KHCO3, NaCl and NaHCO3 supplements, 90 mmol/day for four days, were compared in ten subjects fed normal constant diets. Using synthetic diets, the effects of dietary KCl-deprivation for five days followed by recovery were assessed in four subjects and of KHCO3-deprivation for five days followed by recovery were assessed in four subjects. On the fourth day of salt administration, daily urinary Ca excretion and fasting UCaV/GFR were lower during the administration of KCl than during NaCl supplements (Δ = -1.11 ± 0.28 SEM mmol/day; P < 0.005 and -0.0077 ± 0.0022 mmol/liter GFR; P < 0.01), and lower during KHCO3 than during control (-1.26 ± 0.29 mmol/day; P < 0.005 and -0.0069 ± 0.0019 mmol/liter GFR; P = 0.005). Both dietary KCl and KHCO3 deprivation (mean reduction in dietary K intake -67 ± 8 mmol/day) were accompanied by an increase in daily urinary Ca excretion and fasting UCaV/GFR that averaged on the fifth day +1.31 ± 0.25 mmol/day (P < 0.005) and +0.0069 ± 0.0012 mmol/liter GFR (P < 0.005) above control. Both daily urinary Ca excretion and fasting UCaV/GFR returned toward or to control at the end of recovery. These observations indicate that: 1) KHCO3 decreases fasting and 24-hour urinary Ca excretion; 2) KCl nor NaHCO3, unlike NaCl, do not increase fasting or 24-hour Ca excretion and 3) K deprivation increases both fasting and 24-hour urinary Ca excretion whether the accompanying anion is Cl- or HCO3-. The mechanisms for this effect of K may be mediated by: 1) alterations in ECF volume, since transient increases in urinary Na and CI excretion and weight loss accompanied KCl or KHCO3 administration, while persistent reductions in urinary Na and Cl excretion and a trend for weight gain accompanied K deprivation; 2) K mediated alterations in renal tubular phosphate transport and renal synthesis of 1, 25-(OH)2-vitamin D, since KCl or KHCO3 administration tended to be accompanied by a rise in fasting serum PO4 and TmPO4 and a fall in fasting UPO4 V/GFR, a fall in serum 1,25-(OH)2-D and a decrease in fasting UCaV/GFR, while dietary KCl or KHCO3 deprivation were accompanied by a reverse sequence

The Swift/UVOT catalogue of NGC4321 star forming sources: A case against density wave theory

We study the star forming regions in the spiral galaxy NGC4321, taking advantage of the spatial resolution (2.5 arcsec FWHM) of the Swift/UVOT camera and the availability of three UV passbands in the region 1600-3000 A, in combination with optical and IR imaging from SDSS, KPNO/Ha and Spitzer/IRAC, to obtain a catalogue of 787 star forming regions out to three disc scale lengths. We determine the properties of the young stellar component and its relationship with the spiral arms. The Ha luminosities of the sources have a strong decreasing radial trend, suggesting more massive star forming regions in the central part of the galaxy. When segregated with respect to NUV-optical colour, blue sources have a significant excess of flux in the IR at 8 micron, revealing the contribution from PAHs, although the overall reddening of these sources stays below E(B-V)=0.2 mag. The distribution of distances to the spiral arms is compared for subsamples selected according to Ha luminosity, NUV-optical colour, or ages derived from a population synthesis model. An offset is expected between these subsamples as a function of radius if the pattern speed of the spiral arm were constant - as predicted by classic density wave theory. No significant offsets are found, favouring instead a mechanism where the pattern speed has a radial dependence.Comment: 12 pages, 11 figures, 4 tables. MNRAS, in pres

Obscured star formation in the central region of the dwarf galaxy NGC5253

We present HST/NICMOS observations (1.1-2.2micron) and 1.9-4.1micron spectroscopy of the central region of the dwarf galaxy NGC5253. The HST/NICMOS observations reveal the presence of a nuclear double star cluster separated by 0.3-0.4arcsec or 6-8pc (for a distance d=4.1Mpc). The double star cluster, also a bright double source of Pa-alpha emission, appears to be coincident with the double radio nebula detected at 1.3cm. The eastern near-infrared star cluster (C1) is identified with the youngest optical cluster, whereas the western star cluster (C2), although it is almost completely obscured in the optical, becomes the brightest star cluster in the central region of NGC 5253 at wavelengths longer than 2micron. Both clusters are extremely young with ages of approximately 3.5 million years old. C2 is more massive than C1 by a factor of 6 to 20 (M(C2)= 7.7 x 10^5 - 2.6 x 10^6Msun, for a Salpeter IMF in the mass range 0.1-100Msun). Analysis of the circumnuclear spectrum excluding C1 and C2, as well as of a number of other near-infrared selected clusters with a range of (young) ages, suggests that the star formation was triggered across the central regions of the galaxy. We have also modelled the nuclear UV to mid-infrared spectral energy distribution (SED) of NGC5253 and found that the infrared part is well modelled with a highly obscured (A_V= 17mag) young starburst with a stellar mass consistent with our photometric estimates for C1 and C2. The SED model predicts a moderately bright polycyclic aromatic hydrocarbon (PAH) feature at 3.3micron that is not detected in our nuclear L-band spectrum. NGC5253's low metallicity and a top-heavy IMF likely combine to suppress the 3.3micron PAH emission that is commonly seen in more massive starburst systems.Comment: Accepted for publication in ApJ. High quality versions of Figures 1 and 2 are available upon reques

Adaptive model-driven user interface development systems

Adaptive user interfaces (UIs) were introduced to address some of the usability problems that plague many software applications. Model-driven engineering formed the basis for most of the systems targeting the development of such UIs. An overview of these systems is presented and a set of criteria is established to evaluate the strengths and shortcomings of the state-of-the-art, which is categorized under architectures, techniques, and tools. A summary of the evaluation is presented in tables that visually illustrate the fulfillment of each criterion by each system. The evaluation identified several gaps in the existing art and highlighted the areas of promising improvement

Tidal Dwarf Candidates in a Sample of Interacting Galaxies. II. Properties and Kinematics of the Ionized Gas

We present low-resolution spectroscopy of the ionized gas in a sample of optical knots located along the tidal features of 14 interacting galaxies and previously selected as candidates of Tidal Dwarf Galaxies (TDGs). From redshift measurements, we are able to confirm their physical association with the interacting system in almost all cases. For most knots, the oxygen abundance does not depend on the blue luminosity. The average, 12+log(O/H)=8.34+-0.20, is typical of TDGs and comparable to that measured in the outer stellar disk of spirals from which they were formed. A few knots showing low metallicities are probably pre-existing low-mass companions. The estimated Ha luminosity of the TDG candidates is higher than the one of typical individual HII regions in spiral disks and comparable to the global Ha luminosity of dwarf galaxies. We find several instances of velocity gradients with amplitudes apparently larger than 100 km/s in the ionized gas in the tidal knots and discuss various possible origins for the large velocity amplitudes. While we can exclude tidal streaming motions and outflows, we cannot rule out projection effects with the current resolution. The velocity gradients could be indicative of the internal kinematics characteristic of self-gravitating objects. Higher resolution spectra are required to confirm whether the tidal knots in our sample have already acquired their dynamical independence and are therefore genuine Tidal Dwarf Galaxies.Comment: 12 pages, 7 figures, partly color (but printable in greyscale without loss of information). Paper is accepted by A&A. The appendix with images of the galaxies can be downloaded from http://www.uni-sw.gwdg.de/~weilbach/pubs/pub.htm

Swift UV/Optical Telescope Imaging of Star Forming Regions in M81 and Holmberg IX

We present Swift UV/Optical Telescope (UVOT) imaging of the galaxies M81 and Holmberg IX. We combine UVOT imaging in three near-ultraviolet (NUV) filters (uvw2: 1928 Å; uvm2: 2246 Å; uvw1: 2600 Å) with ground-based optical imaging from the Sloan Digital Sky Survey to constrain the stellar populations of both galaxies. Our analysis consists of three different methods. First, we use the NUV imaging to identify UV star-forming knots and then perform spectral energy distribution (SED) modeling on the UV/optical photometry of these sources. Second, we measure surface brightness profiles of the disk of M81 in the NUV and optical. Lastly, we use SED fitting of individual pixels to map the properties of the two galaxies. In agreement with earlier studies, we find evidence for a burst in star formation in both galaxies starting ~200 Myr ago coincident with the suggested time of an M81-M82 interaction. In line with theories of its origin as a tidal dwarf, we find that the luminosity-weighted age of Holmberg IX is a few hundred million years. Both galaxies are best fit by a Milky Way dust extinction law with a prominent 2175 Å bump. In addition, we describe a stacked median filter technique for modeling the diffuse background light within a galaxy and a Markov chain method for cleaning segment maps generated by SExtractor

Lack of effect of salt on the glucose and insulin response to mashed potatoes, white rice, and lima beans.

The effect of 4.25 g of table salt on the insulin and glucose response to three forms of carbohydrate with varying glycemic indices was studied. There was no statistical difference in the peak response or area under the glucose or insulin curves for any of these foods in the presence of salt. It is concluded that salt has no effect on the absorption of starches