ATCA Study of Small Magellanic Cloud Supernova Remnant 1E 0102.2-7219

We present new and archival Australia Telescope Compact Array and Atacama Large Millimeter/submillimeter Array data of the Small Magellanic Cloud supernova remnant 1E 0102.2-7219 at 2100, 5500, 9000, and 108000 MHz; as well as Hi data provided by the Australian Square Kilometre Array Pathfinder. The remnant shows a ring-like morphology with a mean radius of 6.2 pc. The 5500 MHz image reveals a bridge-like structure, seen for the first time in a radio image. This structure is also visible in both optical and X-ray images. In the 9000 MHz image we detect a central feature that has a flux density of 4.3 mJy but rule out a pulsar wind nebula origin, due to the lack of significant polarisation towards the central feature with an upper limit of 4 per cent. The mean fractional polarisation for 1E 0102.2-7219 is 7 +- 1 and 12 +- 2 per cent for 5500 and 9000 MHz, respectively. The spectral index for the entire remnant is -0.61 +- 0.01. We estimate the line-of-sight magnetic field strength in the direction of 1E 0102.2-7219 of ~44 microG with an equipartition field of 65 +- 5 microG. This latter model, uses the minimum energy of the sum of the magnetic field and cosmic ray electrons only. We detect an Hi cloud towards this remnant at the velocity range of ~160-180 km s-1 and a cavity-like structure at the velocity of 163.7-167.6 km s-1. We do not detect CO emission towards 1E 0102.2-7219

Binary blazed reflection gratings

A reflection grating with a binary surface profile is presented that has high diffraction efficiency. The measured intensity for the + 1st diffracted order was 77%. The binary grating is composed of a minilattice with feature sizes comparable with the wavelength of the incident light. The overall structure is designed in such a way that it imitates a conventional blazed grating. The grating also has interesting polarization properties. The main part of the TE-polarized light is diffracted into the 1st diffracted order, and most of the TM-polarized light remains in the 0th diffracted order. The measurements of the grating are compared with rigorous diffraction theory and found to be in reasonable agreement.Other funderDeutsche Forschungsgemeinschaft (German Research Foundation)pe, la, sp, ke, ab - kpw28/10/1

The Returns to Personality Traits Across the Wage Distribution

This paper investigates heterogeneous wage effects of non-cognitive skills across the wage distribution. I develop a model of wage determination under uncertainty with respect to individual productivity based on three components (minimum wages, productivity premiums, bargaining premiums). Based on this model, I expect (i) a larger importance and (ii) larger effects of non-cognitive skills for high-wage employees compared to their low-wage counterparts. I test these hypotheses with unconditional quantile regressions using large-scale survey data from Germany, the UK, and Australia. To test the joint explanatory contribution of multiple variables within a quantile-regression framework, I propose a new statistic that quantifies the rise in explanatory power generated by additional explanatory variables. The findings indicate a rising importance as well as increasing effects of certain personality traits (agreeableness, neuroticism and risk taking) across the wage distribution for full-time employed males and females