2,852 research outputs found

    Radio Frequency Interference Mitigation

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    Radio astronomy observational facilities are under constant upgradation and development to achieve better capabilities including increasing the time and frequency resolutions of the recorded data, and increasing the receiving and recording bandwidth. As only a limited spectrum resource has been allocated to radio astronomy by the International Telecommunication Union, this results in the radio observational instrumentation being inevitably exposed to undesirable radio frequency interference (RFI) signals which originate mainly from terrestrial human activity and are becoming stronger with time. RFIs degrade the quality of astronomical data and even lead to data loss. The impact of RFIs on scientific outcome is becoming progressively difficult to manage. In this article, we motivate the requirement for RFI mitigation, and review the RFI characteristics, mitigation techniques and strategies. Mitigation strategies adopted at some representative observatories, telescopes and arrays are also introduced. We also discuss and present advantages and shortcomings of the four classes of RFI mitigation strategies, applicable at the connected causal stages: preventive, pre-detection, pre-correlation and post-correlation. The proper identification and flagging of RFI is key to the reduction of data loss and improvement in data quality, and is also the ultimate goal of developing RFI mitigation techniques. This can be achieved through a strategy involving a combination of the discussed techniques in stages. Recent advances in high speed digital signal processing and high performance computing allow for performing RFI excision of large data volumes generated from large telescopes or arrays in both real time and offline modes, aiding the proposed strategy.Comment: 26 pages, 10 figures, Chinese version accepted for publication in Acta Astronomica Sinica; English version to appear in Chinese Astronomy and Astrophysic

    Hitting spheres on hyperbolic spaces

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    For a hyperbolic Brownian motion on the Poincar\'e half-plane H2\mathbb{H}^2, starting from a point of hyperbolic coordinates z=(η,α)z=(\eta, \alpha) inside a hyperbolic disc UU of radius ηˉ\bar{\eta}, we obtain the probability of hitting the boundary ∂U\partial U at the point (ηˉ,αˉ)(\bar \eta,\bar \alpha). For ηˉ→∞\bar{\eta} \to \infty we derive the asymptotic Cauchy hitting distribution on ∂H2\partial \mathbb{H}^2 and for small values of η\eta and ηˉ\bar \eta we obtain the classical Euclidean Poisson kernel. The exit probabilities Pz{Tη1<Tη2}\mathbb{P}_z\{T_{\eta_1}<T_{\eta_2}\} from a hyperbolic annulus in H2\mathbb{H}^2 of radii η1\eta_1 and η2\eta_2 are derived and the transient behaviour of hyperbolic Brownian motion is considered. Similar probabilities are calculated also for a Brownian motion on the surface of the three dimensional sphere. For the hyperbolic half-space Hn\mathbb{H}^n we obtain the Poisson kernel of a ball in terms of a series involving Gegenbauer polynomials and hypergeometric functions. For small domains in Hn\mathbb{H}^n we obtain the nn-dimensional Euclidean Poisson kernel. The exit probabilities from an annulus are derived also in the nn-dimensional case

    Mid-infrared photodetectors operating over an extended wavelength range up to 90 K

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    We report a wavelength threshold extension, from the designed value of 3.1 to 8.9 ÎŒm, in a -type heterostructure photodetector. This is associated with the use of a graded barrier and barrier offset, and arises from hole–hole interactions in the detector absorber. Experiments show that using long-pass filters to tune the energies of incident photons gives rise to changes in the intensity of the response. This demonstrates an alternative approach to achieving tuning of the photodetector response without the need to adjust the characteristic energy that is determined by the band structure

    Parsec-scale jet properties of the gamma-ray quasar 3C 286

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    The quasar 3C~286 is one of two compact steep spectrum sources detected by the {\it Fermi}/LAT. Here, we investigate the radio properties of the parsec(pc)-scale jet and its (possible) association with the Îł\gamma-ray emission in 3C~286. The Very Long Baseline Interferometry (VLBI) images at various frequencies reveal a one-sided core--jet structure extending to the southwest at a projected distance of ∌\sim1 kpc. The component at the jet base showing an inverted spectrum is identified as the core, with a mean brightness temperature of 2.8×1092.8\times 10^{9}~K. The jet bends at about 600 pc (in projection) away from the core, from a position angle of −135∘-135^\circ to −115∘-115^\circ. Based on the available VLBI data, we inferred the proper motion speed of the inner jet as 0.013±0.0110.013 \pm 0.011 mas yr−1^{-1} (ÎČapp=0.6±0.5\beta_{\rm app} = 0.6 \pm 0.5), corresponding to a jet speed of about 0.5 c0.5\,c at an inclination angle of 48∘48^\circ between the jet and the line of sight of the observer. The brightness temperature, jet speed and Lorentz factor are much lower than those of Îł\gamma-ray-emitting blazars, implying that the pc-scale jet in 3C~286 is mildly relativistic. Unlike blazars in which Îł\gamma-ray emission is in general thought to originate from the beamed innermost jet, the location and mechanism of Îł\gamma-ray emission in 3C~286 may be different as indicated by the current radio data. Multi-band spectrum fitting may offer a complementary diagnostic clue of the Îł\gamma-ray production mechanism in this source.Comment: 9 pages, 4 figures, accept for publication in MNRA

    Parkinson’s disease dyskinesias possibly relate to greater dopamine transporter losses in the putamen over time

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    The pathophysiology of levodopa-induced dyskinesias in Parkinson’s disease is incompletely understood. This study was designed to investigate in Parkinson’s patients, whether time-related changes in striatal dopamine transporter availability are associated to the appearance of dyskinesias. 15 Parkinson’s patients had dopamine transporter-specific SPECT imaging with 123I-FP-CIT twice: at baseline (when they were drug naĂŻve) and at follow-up (6.31±2.29 years from baseline), and were followed up clinically every six months. At the end of the study, patients were divided in two groups according to whether they had developed dyskinesias or not. Semi-quantification of 123I-FP-CIT data was performed using the occipital cortex as the reference region. Specific binding ratios were calculated for the putamen and the caudate. During the clinical follow-up, all Parkinson’s patients were treated pharmaceutically. 8 patients developed dyskinesias, while 7 remained nondyskinetic. At baseline, the two groups had similar 123I-FP-CIT specific binding ratio values for the putamen and the caudate (p>0.05). Also, between-group differences in age, disease duration, and Hoehn & Yahr scores were not statistically significant. Over-time, the putaminal 123I-FP-CIT specific binding ratio values in the dyskinetic group decreased significantly (p<0.01). The nondyskinetic patients had smaller reductions (p<0.05) during the same period of time. At follow-up, the dyskinetic patients had significantly higher Hoehn & Yahr scores (p<0.01) and were taking higher levodopa equivalent doses (p<0.001), as compared to the nondyskinetic patients. The development of Parkinson’s dyskinesias is related to a faster progression rate, as reflected by marked putaminal dopamine transporter decreases

    Comparison of chemical profiles and effectiveness between Erxian decoction and mixtures of decoctions of its individual herbs : a novel approach for identification of the standard chemicals

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    Acknowledgements This study was partially supported by grants from the Seed Funding Programme for Basic Research (Project Number 201211159146 and 201411159213), the University of Hong Kong. We thank Mr Keith Wong and Ms Cindy Lee for their technical assistances.Peer reviewedPublisher PD
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