11,171 research outputs found

    The magnetic field of the double-lined spectroscopic binary system HD 5550

    Full text link
    (Abridged) In the framework of the BinaMicS project, we have begun a study of the magnetic properties of a sample of intermediate-mass and massive short-period binary systems, as a function of binarity properties. We report in this paper the characterisation of the magnetic field of HD 5550, a double-lined spectroscopic binary system of intermediate-mass, using high-resolution spectropolarimetric Narval observations of HD 5550. We first fit the intensity spectra using Zeeman/ATLAS9 LTE synthetic spectra to estimate the effective temperatures, microturbulent velocities, and the abundances of some elements of both components, as well as the light-ratio of the system. We then fit the least-square deconvolved II profiles to determine the radial and projected rotational velocities of both stars. We then analysed the shape and evolution of the LSD VV profiles using the oblique rotator model to characterise the magnetic fields of both stars. We confirm the Ap nature of the primary, previously reported in the literature, and find that the secondary displays spectral characteristics typical of an Am star. While a magnetic field is clearly detected in the lines of the primary, no magnetic field is detected in the secondary, in any of our observation. If a dipolar field were present at the surface of the Am star, its polar strength must be below 40 G. The faint variability observed in the Stokes VV profiles of the Ap star allowed us to propose a rotation period of 6.840.39+0.616.84_{-0.39}^{+0.61} d, close to the orbital period (\sim6.82 d), suggesting that the star is synchronised with its orbit. By fitting the variability of the VV profiles, we propose that the Ap component hosts a dipolar field inclined with the rotation axis at an angle β=156±17\beta=156\pm17 ^{\circ} and a polar strength Bd=65±20B_{\rm d}=65 \pm 20 G. The field strength is the weakest known for an Ap star.Comment: 13 pages, 12 figures, accepted for publication in Astronomy & Astrophysic

    Exploring Outliers in Crowdsourced Ranking for QoE

    Full text link
    Outlier detection is a crucial part of robust evaluation for crowdsourceable assessment of Quality of Experience (QoE) and has attracted much attention in recent years. In this paper, we propose some simple and fast algorithms for outlier detection and robust QoE evaluation based on the nonconvex optimization principle. Several iterative procedures are designed with or without knowing the number of outliers in samples. Theoretical analysis is given to show that such procedures can reach statistically good estimates under mild conditions. Finally, experimental results with simulated and real-world crowdsourcing datasets show that the proposed algorithms could produce similar performance to Huber-LASSO approach in robust ranking, yet with nearly 8 or 90 times speed-up, without or with a prior knowledge on the sparsity size of outliers, respectively. Therefore the proposed methodology provides us a set of helpful tools for robust QoE evaluation with crowdsourcing data.Comment: accepted by ACM Multimedia 2017 (Oral presentation). arXiv admin note: text overlap with arXiv:1407.763

    Fractal Markets Hypothesis and the Global Financial Crisis: Scaling, Investment Horizons and Liquidity

    Full text link
    We investigate whether fractal markets hypothesis and its focus on liquidity and invest- ment horizons give reasonable predictions about dynamics of the financial markets during the turbulences such as the Global Financial Crisis of late 2000s. Compared to the mainstream efficient markets hypothesis, fractal markets hypothesis considers financial markets as com- plex systems consisting of many heterogenous agents, which are distinguishable mainly with respect to their investment horizon. In the paper, several novel measures of trading activity at different investment horizons are introduced through scaling of variance of the underlying processes. On the three most liquid US indices - DJI, NASDAQ and S&P500 - we show that predictions of fractal markets hypothesis actually fit the observed behavior quite well.Comment: 11 pages, 3 figure

    The Level-0 Muon Trigger for the LHCb Experiment

    Get PDF
    A very compact architecture has been developed for the first level Muon Trigger of the LHCb experiment that processes 40 millions of proton-proton collisions per second. For each collision, it receives 3.2 kBytes of data and it finds straight tracks within a 1.2 microseconds latency. The trigger implementation is massively parallel, pipelined and fully synchronous with the LHC clock. It relies on 248 high density Field Programable Gate arrays and on the massive use of multigigabit serial link transceivers embedded inside FPGAs.Comment: 33 pages, 16 figures, submitted to NIM

    Microstructure Effects on Daily Return Volatility in Financial Markets

    Full text link
    We simulate a series of daily returns from intraday price movements initiated by microstructure elements. Significant evidence is found that daily returns and daily return volatility exhibit first order autocorrelation, but trading volume and daily return volatility are not correlated, while intraday volatility is. We also consider GARCH effects in daily return series and show that estimates using daily returns are biased from the influence of the level of prices. Using daily price changes instead, we find evidence of a significant GARCH component. These results suggest that microstructure elements have a considerable influence on the return generating process.Comment: 15 pages, as presented at the Complexity Workshop in Aix-en-Provenc

    Charge Transport in Non-Irradiated and Irradiated Silicon Diodes

    Get PDF
    A model describing the transport of charge carriers generated in silicon detectors (standard planar float zone and MESA diodes) by ionizing particles is presented. The current pulse response induced by α\alpha and β\beta particles in non-irradiated detectors and detectors irradiated up to fluences Φ31014\Phi \approx 3 \cdot 10^{14} particles/cm2^2 is reproduced through this model: i) by adding a small n-type region 15 μ\mum deep on the p+p^+ side for the standard planar float zone detectors at fluences beyond the n to p-type inversion and ii) for the MESA detectors, by considering one dead layer 14 μ\mum deep (observed experimentally) on each side, and introducing a second (delayed) component. For both types of detectors, the model gives mobilities decreasing linearily up to fluences of about 510135 \cdot 10^{13} particles/cm2^2 and converging, beyond, to saturation values of about 1000 cm2^2/Vs and 455 cm2^2/Vs for electrons and holes, respectively. At a fluence Φ1014\Phi \approx 10^{14} particles/cm2^2, charge collection deficits of about 13\% for β\beta particles, 25\% for α\alpha particles incident on the front and 35\% for α\alpha particles incident on the back of the detector are found for both type of diodes

    Study of charge Transport in Silicon Detectors: Non-Irradiated and Irradiated

    Get PDF
    The electrical characteristics of silicon detectors (standard planar float zone and MESA detectors) as a function of the particle fluence can be extracted by the application of a model describing the transport of charge carriers generated in the detectors by ionizing particles. The current pulse response induced by α\alpha and β\beta particles in non-irradiated detectors and detectors irradiated up to fluences Φ31014\Phi \approx 3 \cdot 10^{14} particles/cm2^2 is reproduced via this model: i) by adding a small n-type region 15 μ\mum deep on the p+p^+ side for the detectors at fluences beyond the n to p-type inversion and ii) for the MESA detectors, by considering one additional dead layer of 14 μ\mum (observed experimentally) on each side of the detector, and introducing a second (delayed) component to the current pulse response. For both types of detectors, the model gives mobilities decreasing linearily up to fluences of about 510135 \cdot 10^{13} particles/cm2^2 and converging, beyond, to saturation values of about 1050 cm2^2/Vs and 450 cm2^2/Vs for electrons and holes, respectively. At a fluence Φ1014\Phi \approx 10^{14} particles/cm2^2 (corresponding to about ten years of operation at the CERN-LHC), charge collection deficits of about 14\% for β\beta particles, 25\% for α\alpha particles incident on the front and 35\% for α\alpha particles incident on the back of the detector are found for both type of detectors

    Optimizing a Certified Proof Checker for a Large-Scale Computer-Generated Proof

    Full text link
    In recent work, we formalized the theory of optimal-size sorting networks with the goal of extracting a verified checker for the large-scale computer-generated proof that 25 comparisons are optimal when sorting 9 inputs, which required more than a decade of CPU time and produced 27 GB of proof witnesses. The checker uses an untrusted oracle based on these witnesses and is able to verify the smaller case of 8 inputs within a couple of days, but it did not scale to the full proof for 9 inputs. In this paper, we describe several non-trivial optimizations of the algorithm in the checker, obtained by appropriately changing the formalization and capitalizing on the symbiosis with an adequate implementation of the oracle. We provide experimental evidence of orders of magnitude improvements to both runtime and memory footprint for 8 inputs, and actually manage to check the full proof for 9 inputs.Comment: IMADA-preprint-c
    corecore