The continuous postage stamp problem

For a real set $A$ consider the semigroup $S(A)$, additively generated by $A$; that is, the set of all real numbers representable as a (finite) sum of elements of $A$. If $A \subset (0,1)$ is open and non-empty, then $S(A)$ is easily seen to contain all sufficiently large real numbers, and we let $G(A) := \sup \{u \in R \colon u \notin S(A) \}$. Thus, $G(A)$ is the smallest number with the property that any $u>G(A)$ is representable as indicated above. We show that if the measure of $A$ is large, then $G(A)$ is small; more precisely, writing for brevity \alpha := \mes A we have G(A) \le (1-\alpha) \lfloor 1/\alpha \rfloor \quad &\text{if $0 < \alpha \le 0.1$}, (1-\alpha+\alpha\{1/\alpha\})\lfloor 1/\alpha\rfloor \quad &\text{if $0.1 \le \alpha \le 0.5$}, 2(1-\alpha) \quad &\text{if $0.5 \le \alpha \le 1$}. Indeed, the first and the last of these three estimates are the best possible, attained for $A=(1-\alpha,1)$ and $A=(1-\alpha,1)\setminus\{2(1-\alpha)\}$, respectively; the second is close to the best possible and can be improved by $\alpha \{1/\alpha\} \lfloor 1/\alpha \rfloor \le \{1/\alpha\}$ at most. The problem studied is a continuous analogue of the linear Diophantine problem of Frobenius (in its extremal settings due to Erdos and Graham), also known as the "postage stamp problem" or the "coin exchange problem"

Cost-allocation principles for pipeline capacity and usage

This paper applies principles f rom game theory to the problem o f allocating the cost o f a shared facility, such as a pipeline. The theory o f cooperative games s t r ongl y suggest s t hat no method e x i s t s for allocating costs that wi l l achieve all major policy goals. We apply results from the theory o f cooperative games a n d principles o f cost allocation to assess some c o mmo n l y adopted rules for allocating costs and def i ni ng u n i t charges. Mos t notably, the postage-stamp toll is f o u n d to fail a mi ni mal set o f commonly applied principles.cost allocation; pipeline

GREAT3 results I: systematic errors in shear estimation and the impact of real galaxy morphology

We present first results from the third GRavitational lEnsing Accuracy Testing (GREAT3) challenge, the third in a sequence of challenges for testing methods of inferring weak gravitational lensing shear distortions from simulated galaxy images. GREAT3 was divided into experiments to test three specific questions, and included simulated space- and ground-based data with constant or cosmologically-varying shear fields. The simplest (control) experiment included parametric galaxies with a realistic distribution of signal-to-noise, size, and ellipticity, and a complex point spread function (PSF). The other experiments tested the additional impact of realistic galaxy morphology, multiple exposure imaging, and the uncertainty about a spatially-varying PSF; the last two questions will be explored in Paper II. The 24 participating teams competed to estimate lensing shears to within systematic error tolerances for upcoming Stage-IV dark energy surveys, making 1525 submissions overall. GREAT3 saw considerable variety and innovation in the types of methods applied. Several teams now meet or exceed the targets in many of the tests conducted (to within the statistical errors). We conclude that the presence of realistic galaxy morphology in simulations changes shear calibration biases by $\sim 1$ per cent for a wide range of methods. Other effects such as truncation biases due to finite galaxy postage stamps, and the impact of galaxy type as measured by the S\'{e}rsic index, are quantified for the first time. Our results generalize previous studies regarding sensitivities to galaxy size and signal-to-noise, and to PSF properties such as seeing and defocus. Almost all methods' results support the simple model in which additive shear biases depend linearly on PSF ellipticity.Comment: 32 pages + 15 pages of technical appendices; 28 figures; submitted to MNRAS; latest version has minor updates in presentation of 4 figures, no changes in content or conclusion

Persediaan kerjaya pelajar tahun akhir diploma akauntansi Politeknik dalam melahirkan K-Workes : satu tinjauan

This research was conducted to identify Polytechnic's Diploma in Accountancy final year students' career preparation before enter the working environment to be k-workers. The sample in this study consisted of 48 final year students of Diploma in Accountancy Politeknik Sultan Haji Ahmad Shah (POLISAS), Kuantan. Questionnaire has been chosen as an instrument to get the data. The data was analyzed by using the Statistical Package For Social Sciences (SPSS) package to derive the percentages and mean. The results revealed the Diploma of Accountancy final year students are quite prepared to enter the working environment. Although the students performed very well for their career preparation, there are still dissatisfaction in other two aspects i.e. they lack of information career opportunity and communication in English. Therefore, the career guideline have been proposed to give an exposure for the students to be k-workers in their career in the future

The dependence of intrinsic alignment of galaxies on wavelength using KiDS and GAMA

The outer regions of galaxies are more susceptible to the tidal interactions that lead to intrinsic alignments of galaxies. The resulting alignment signal may therefore depend on the passband if the colours of galaxies vary spatially. To quantify this, we measured the shapes of galaxies with spectroscopic redshifts from the GAMA survey using deep gri imaging data from the KiloDegree Survey. The performance of the moment-based shape measurement algorithm DEIMOS was assessed using dedicated image simulations, which showed that the ellipticities could be determined with an accuracy better than 1% in all bands. Additional tests for potential systematic errors did not reveal any issues. We measure a significant difference of the alignment signal between the g,r and i-band observations. This difference exceeds the amplitude of the linear alignment model on scales below 2 Mpc/h. Separating the sample into central/satellite and red/blue galaxies, we find that that the difference is dominated by red satellite galaxies.Comment: 16 pages, 13 figures, accepted, to appear in A&

The Liberalisation of the Energy Sector in the European Union

The energy sector covers the coal, oil, gas and electricity sector. The European coal and oil sector have already been liberalised in the past. The current debate concerns mainly the electricity and the gas sector. In this paper we will concentrate on the electricity sector for three reasons. First, the sector is more important in terms of value added, secondly it is considered to be more complex and, finally, the opening of the electricity market precedes that of the gas market. Obviously, this does not mean that the gas sector should not be studied as there are many challenges left. In section II, we discuss the institutional background for the liberalisation. Section III then analyses the British experience. This is of interest because the UK has liberalised its market about 10 years ago and this experience has been the subject of extensive economic research. In the sections IV to VII, we focus on the four main problems in the liberalisation of the European electricity market: the stranded costs issue, the cross-subsidies issue, the pricing of transmission and the regulation of the environment. Finally, section VIII concludes.