Exploring the Use of Virtual Worlds as a Scientific Research Platform: The Meta-Institute for Computational Astrophysics (MICA)

We describe the Meta-Institute for Computational Astrophysics (MICA), the first professional scientific organization based exclusively in virtual worlds (VWs). The goals of MICA are to explore the utility of the emerging VR and VWs technologies for scientific and scholarly work in general, and to facilitate and accelerate their adoption by the scientific research community. MICA itself is an experiment in academic and scientific practices enabled by the immersive VR technologies. We describe the current and planned activities and research directions of MICA, and offer some thoughts as to what the future developments in this arena may be.Comment: 15 pages, to appear in the refereed proceedings of "Facets of Virtual Environments" (FaVE 2009), eds. F. Lehmann-Grube, J. Sablating, et al., ICST Lecture Notes Ser., Berlin: Springer Verlag (2009); version with full resolution color figures is available at http://www.mica-vw.org/wiki/index.php/Publication

On World Problems. Facts and Implications - A Hungarian View

This volume of Hungarian studies was compiled as part of the UNESCO Major Programme I (Reflection on World Problems and Future-oriented Studies) within the framework of the contract concluded between UNESCO and IIASA. The subject of the contract was the preparation of a study entitled World Problems and their Perceptions. The study was compiled in coordination with the Hungarian National Member Organization of IIASA. The Report, in addition to the State of the Art part, contains information about the Task Force Meeting which UNESCO and IIASA organized in Budapest, February 1985, on a theme in accordance with the title of the report and the contributions of which will appear later in book form. This Collaborative Paper is part of the background material of the Report. It shows a possible perception and interpretation of a group of problems, and the implications arising therefrom. The Report sets out to show what concealed cultural or professional presuppositions there are behind the weight of the different conceptions of so-called global or world problems and how they differ in relation to each other. In this connection it reflects on the UNESCO Medium-Term Plan: "Whatever the approaches adopted, studies on world problems are inevitably linked, by the very nature of the field they cover -- which is none other than the present and future of societies -- to choices based on presuppositions regarding standards or on systems of values or even on ideological choices. They seem to require, as their necessary complement, an open-minded examination carried out in a context which promotes intellectual cooperation and within which all currents of thought can be freely expressed; and no organization seems to offer such a context more successfully than UNESCO." The Report tries to justify the hypothesis formulated in UNESCO's Medium-Term Plan and make clear the necessary existence of differing cultural and professional world views in this respect. It shows that there is no one correct point of view, that many rational conceptions of equal value to each other exist, and that in relation to these problems only the acceptance of plural rationality can lead to common solutions. While this conception seems trivial, practice shows that in seeking solutions this approach is not unique and not at all self-explanatory. The Report and the Collaborative Paper show how the economic, social and cultural conditions, as well as practice, determine the world view, how wide the differences are, and that they necessarily lead to various problem formulations and action plans. In actual fact these outlined differences and knowledge of their explanation can lead the international organizations to the formulation of fuller and, probably, more successful action programmes than previously. In the Collaborative Paper we offer a selection of Hungarian studies prepared recently in various specialized fields, we give an insight into the workshop debates and results of the Hungarian research teams, and last but not least, we try to show the options formed an different topics by Hungarian researchers. The volume is not a homogeneous-topic selection, but at the same time we endeavored, by examining the facts, to concentrate on different features of the unequal development taking place globally and to indicate the interconnection between the studies. The authors of the studies examine, in a complex way, the world economic. and world political changes of the past years, the present state and tendencies of world factors and draw conclusions as to the expected developments. Naturally, as with all selections, the content of our volume cannot cover the wide range of problems -- also formulated by UNESCO's programmes, even though we plan several selections during the programme period. With this initiative, while wishing to give a sample of the work and opinions of Hungarian researchers, we would also like to encourage other national research teams to make a similar statement of opinion, so that we can contribute directly to the dialogue in the range of topics of the world problems programme being discussed also in international organizations. The range of studies closes with a summary, in which in addition to a summing up of the contents and conclusions of the studies, a sharper formulation is made of those questions to which we want particularly to draw attention at the present stage of the World Problems Programme, covering an extremely wide range of topics

Simultaneous Multicolor Detection of Faint Galaxies in the Hubble Deep Field

We present a novel way to detect objects when multiband images are available. Typically, object detection is performed in one of the available bands or on a somewhat arbitrarily co-added image. Our technique provides an almost optimal way to use all the color information available. We build up a composite image of the N passbands where each pixel value corresponds to the probability that the given pixel is just sky. By knowing the probability distribution of sky pixels (a chi-square distribution with N degrees of freedom), the data can be used to derive the distribution of pixels dominated by object flux. From the two distributions an optimal segmentation threshold can be determined. Clipping the probability image at this threshold yields a mask, where pixels unlikely to be sky are tagged. After using a standard connected-pixel criterion, the regions of this mask define the detected objects. Applying this technique to the Hubble Deep Field data, we find that we can extend the detection limit of the data below that possible using linearly co-added images. We also discuss possible ways of enhancing object detection probabilities for certain well defined classes of objects by using various optimized linear combinations of the pixel fluxes (optimal subspace filtering).Comment: 8 pages, 5 figures (4 postscript, 1 JPEG). To be published in A

Reconstructing Galaxy Spectral Energy Distributions from Broadband Photometry

We present a novel approach to photometric redshifts, one that merges the advantages of both the template fitting and empirical fitting algorithms, without any of their disadvantages. This technique derives a set of templates, describing the spectral energy distributions of galaxies, from a catalog with both multicolor photometry and spectroscopic redshifts. The algorithm is essentially using the shapes of the templates as the fitting parameters. From simulated multicolor data we show that for a small training set of galaxies we can reconstruct robustly the underlying spectral energy distributions even in the presence of substantial errors in the photometric observations. We apply these techniques to the multicolor and spectroscopic observations of the Hubble Deep Field building a set of template spectra that reproduced the observed galaxy colors to better than 10%. Finally we demonstrate that these improved spectral energy distributions lead to a photometric-redshift relation for the Hubble Deep Field that is more accurate than standard template-based approaches.Comment: 23 pages, 8 figures, LaTeX AASTeX, accepted for publication in A

Linear Matrix Inequality-based Robust Controller design for Type-1 Diabetes Model

This paper investigates the capabilities of a sophisticate d robust nonlinear controller designed directly for a widely known and used high-order non linear type 1 diabetes (T1DM) model to lessen the dependency from patient compliance and t o answer practical requirements such as avoiding hypoglycaemia. The resulting controller c an perform adequately in nominal conditions, but expected to keep this performance even in ex treme situations, e.g. high carbohydrate intake, rejecting hypoglycaemic episodes

All degree six local unitary invariants of k qudits

We give explicit index-free formulae for all the degree six (and also degree four and two) algebraically independent local unitary invariant polynomials for finite dimensional k-partite pure and mixed quantum states. We carry out this by the use of graph-technical methods, which provides illustrations for this abstract topic.Comment: 18 pages, 6 figures, extended version. Comments are welcom

Sensor Drift Compensation Using Fuzzy Interference System and Sparse-Grid Quadrature Filter in Blood Glucose Control

Diabetes mellitus is a serious chronic condition of the human metabolism. The development of an automated treatment has reached clinical phase in the last few years. The goal is to keep the blood glucose concentration within a certain region with minimal interaction required by the patient or medical personnel. However, there are still several prac- tical problems to solve. One of these would be that the available sensors have significant noise and drift. The latter is rather difficult to manage, because the deviating signal can cause the controller to drive the glu- cose concentration out of the safe region even in the case of frequent calibration. In this study a linear-quadratic-Gaussian (LQG) controller is employed on a widely used diabetes model and enhanced with an ad- vanced Sparse-grid quadratic filter and a fuzzy interference system-based calibration supervisor

Probabilistic Cross-Identification of Astronomical Sources

We present a general probabilistic formalism for cross-identifying astronomical point sources in multiple observations. Our Bayesian approach, symmetric in all observations, is the foundation of a unified framework for object matching, where not only spatial information, but physical properties, such as colors, redshift and luminosity, can also be considered in a natural way. We provide a practical recipe to implement an efficient recursive algorithm to evaluate the Bayes factor over a set of catalogs with known circular errors in positions. This new methodology is crucial for studies leveraging the synergy of today's multi-wavelength observations and to enter the time-domain science of the upcoming survey telescopes.Comment: Accepted for publication in the Astrophysical Journal, 8 pages, 1 figure, emulateapj w/ apjfont

A comparison of estimators for the two-point correlation function

Nine of the most important estimators known for the two-point correlation function are compared using a predetermined, rigorous criterion. The indicators were extracted from over 500 subsamples of the Virgo Hubble Volume simulation cluster catalog. The ``real'' correlation function was determined from the full survey in a 3000Mpc/h periodic cube. The estimators were ranked by the cumulative probability of returning a value within a certain tolerance of the real correlation function. This criterion takes into account bias and variance, and it is independent of the possibly non-Gaussian nature of the error statistics. As a result for astrophysical applications a clear recommendation has emerged: the Landy & Szalay (1993) estimator, in its original or grid version Szapudi & Szalay (1998), are preferred in comparison to the other indicators examined, with a performance almost indistinguishable from the Hamilton (1993) estimator.Comment: aastex, 10 pages, 1 table, 1 figure, revised version, accepted in ApJ