Evaluation methods among corporate travel managers

This study examined whether corporate travel planners performed any kind of evaluation among their clients and in that case what that evaluation revealed about the different air lines\u27 performance. A questionnaire was sent out to 100 members of National Business Travel Association (NBTA) all over the U.S. In this questionnaire the respondents were asked to answer 10 questions about if and how the evaluated the performance of the airlines. In the survey, 25% of the respondents said that they did not perform any evaluation at all. The most commonly used evaluation method was to hand-out questionnaires which was used by 37.5%. Focus groups were used by 11% of the respondents as an evaluation method. When asked why they did not perform focus groups 40% said it was too time consuming. None of the respondents indicated that it was too expensive or that they did not have the knowledge. When conducting focus groups the most commonly used method was to pick out participators from a frequent flier list provided by the airlines. The top issued brought up in their evaluation whether they used focus groups or any other kind of evaluation method, was arrival time of the airlines. The highest rated U. S carrier was USAir followed by United and the highest rated transatlantic carrier was British Airways followed by SAS

Progenitors of Long Gamma-ray Bursts

Pinpointing the progenitors of long duration gamma-ray bursts (LGRBs) remains an extremely important question, although it is now clear that at least a fraction of LGRBs originate in the core collapse of massive stars in type Ic supernovae, the pathways to the production of these stars, and their initial masses, remain uncertain. Rotation is thought to be vital in the creation of LGRBs, and it is likely that black hole creation is also necessary. We suggest that these two constraints can be met if the GRB progenitors are very massive stars (>20 solar masses) and are formed in tight binary systems. Using simple models we compare the predictions of this scenario with observations and find that the location of GRBs on their host galaxies are suggestive of main-sequence masses in excess of 20 solar masses, while 50% of the known compact binary systems may have been sufficiently close to have had the necessary rotation rates for GRB creation. Thus, massive stars in compact binaries are a likely channel for at least some fraction of LGRBs.Comment: To appear in "Gamma-ray bursts: Prospects for GLAST", AIP Conference proceedings 906, Editors M. Axelsson and F Ryd

Use of net cages for fish farming in swedish conditions

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Qubits from Number States and Bell Inequalities for Number Measurements

Bell inequalities for number measurements are derived via the observation that the bits of the number indexing a number state are proper qubits. Violations of these inequalities are obtained from the output state of the nondegenerate optical parametric amplifier.Comment: revtex4, 7 pages, v2: results identical but extended presentation, v3: published versio

β- and α-Cell Dysfunction in Subjects Developing Impaired Glucose Tolerance: Outcome of a 12-Year Prospective Study in Postmenopausal Caucasian Women

OBJECTIVE— This study assessed insulin and glucagon secretion in relation to insulin sensitivity in Caucasian women who develop impaired glucose tolerance (IGT) versus those who maintain normal glucose tolerance (NGT) over a 12-year period

TFAM forces mtDNA to make a U-turn

The mammalian mitochondrial transcription factor A (TFAM) is encoded in the nucleus and imported into mitochondria, where it functions as an activator of mtDNA transcription and packages mtDNA into DNA-protein aggregates called mitochondrial nucleoids. Two X-ray crystallography studies in this issue reveal that TFAM shapes mtDNA into a sharp U-turn, thereby providing a molecular mechanism for its dual roles in the expression and maintenance of mtDNA.VetenskapsrådetPublishe

An adaptive-binning method for generating constant-uncertainty/constant-significance light curves with Fermi-LAT data

We present a method enabling the creation of constant-uncertainty/constant-significance light curves with the data of the Fermi-Large Area Telescope (LAT). The adaptive-binning method enables more information to be encapsulated within the light curve than with the fixed-binning method. Although primarily developed for blazar studies, it can be applied to any sources. This method allows the starting and ending times of each interval to be calculated in a simple and quick way during a first step. The reported mean flux and spectral index (assuming the spectrum is a power-law distribution) in the interval are calculated via the standard LAT analysis during a second step. The absence of major caveats associated with this method has been established by means of Monte-Carlo simulations. We present the performance of this method in determining duty cycles as well as power-density spectra relative to the traditional fixed-binning method.Comment: 17 pages, 13 figures, 5 tables. Submitted to A&