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Training Artificial Neural Networks on the Marginal Distribution Estimates of the C index

Inom sjukvården delas patienter ofta in i riskgrupper som avgör vilken behandling som passar varje patient bäst. Företrädesvis ska indelningen baseras på information om patienterna, som till exempel ålder och tumörstorlek, och det är möjligt att använda sig av känd patientinformation för att lära en dator att koppla en given patient till en viss riskgrupp. Detta görs genom att man minimerar någon In this project, we compare two error functions for the purpose of training artificial neural networks on heavily censored data (data where key information is missing). J. Kalderstam et al. has shown that it is possible to train artificial neural networks directly on Harrell's C index \cite{Harrell} using genetic algorithms. He has also investigated the possibilities of improving the performa

The Gaia -ESO Survey : Spectroscopic-asteroseismic analysis of K2 stars in Gaia -ESO

Context. The extensive stellar spectroscopic datasets that are available for studies in Galactic Archeaology thanks to, for example, the Gaia-ESO Survey, now benefit from having a significant number of targets that overlap with asteroseismology projects such as Kepler, K2, and CoRoT. Combining the measurements from spectroscopy and asteroseismology allows us to attain greater accuracy with regard

BIKE STROLLER

According to research from the Municipality of Lund, our travel habits as adults are to 90 percent obtained before the age of 13. Yet, every 4th child in Sweden is given a lift by car to school and day nursery often less than 1000 metres away. These short journeys could easily be replaced by bike. By constantly choosing the car, we adults pass on the attitude of the car being the mean of transport

Galileo observes electromagnetically coupled dust in the Jovian magnetosphere

Measurements of dust coupled to the Jovian magnetosphere have been obtained with the dust detector on board the Galileo spacecraft. We report on data obtained during the first four orbits about Jupiter that had flybys of the Galilean satellites: Ganymede (orbits 1 and 2), Callisto (orbit 3), and Europa (orbit 4). The most prominent features observed are highly time variable dust streams recorded t

The selection function of the RAVE survey

We characterize the selection function of RAdial Velocity Experiment (RAVE) using 2 Micron All Sky Survey (2MASS) as our underlying population, which we assume represents all stars that could have potentially been observed.We evaluate the completeness fraction as a function of position, magnitude and colour in two ways: first, on a field-by-field basis, and second, in equal-size areas on the sky.