A Proposed Search for the Detection of Gravitational Waves from Eccentric...
Most of compact binary systems are expected to circularize before the frequency of emitted gravitational waves (GWs) enters the sensitivity band of the ground based interferometric detectors. However,...
View ArticleOptimal design of calibration signals in space borne gravitational wave...
Future space borne gravitational wave detectors will require a precise definition of calibration signals to ensure the achievement of their design sensitivity. The careful design of the test signals...
View ArticleA study on diffuse source detection by HXMT scanning observation [Replacement]
The Hard X-ray Modulation Telescope (HXMT) is a collimated scan X-ray satellite mainly devoted to a sensitive all-sky survey and pointed observations in 1-250 keV. We expect various diffuse sources to...
View ArticleAdvanced Environment for Knowledge Discovery in the VIALACTEA Project...
The VIALACTEA project aims at building a predictive model of star formation in our galaxy. We present the innovative integrated framework and the main technologies and methodologies to reach this...
View ArticleMethod for detection and reconstruction of gravitational wave transients with...
We present a method for detection and reconstruction of the gravitational wave (GW) transients with the networks of advanced detectors. Originally designed to search for transients with the initial GW...
View ArticleObservation of polarised hard X-ray emission from the Crab by the PoGOLite...
We have measured the linear polarisation of hard X-ray emission from the Crab in a previously unexplored energy interval, 20-120 keV. The introduction of two new observational parameters, the...
View ArticleLow Latency transient search of Gravitational Waves for the Advanced...
The reliability of the first detection is one of the most interesting challenges for the gravitational wave community. To increase the detection confidence, the LIGO and Virgo collaborations have...
View ArticleAutomated Detection of Solar Eruptions [Replacement]
Observation of the solar atmosphere reveals a wide range of motions, from small scale jets and spicules to global-scale coronal mass ejections. Identifying and characterizing these motions are...
View ArticleScintillation noise in widefield radio interferometry [Replacement]
In this paper, we consider random phase fluctuations imposed during wave propagation through a turbulent plasma (e.g. ionosphere) as a source of additional noise in interferometric visibilities. We...
View ArticleRelativistic Hydrodynamics with Wavelets
Methods to solve the relativistic hydrodynamic equations are a key computational kernel in a large number of astrophysics simulations and are crucial to understanding the electromagnetic signals that...
View ArticleFast-neutron induced background in LaBr3:Ce detectors [Cross-Listing]
The response of a scintillation detector with a cylindrical 1.5-inch LaBr3:Ce crystal to incident neutrons has been measured in the energy range En = 2-12 MeV. Neutrons were produced by proton...
View Article70 years of Sunspot Observations at Kanzelh\"ohe Observatory: systematic...
Kanzelh\"ohe Observatory (KSO) was founded during World War II by the "Deutsche Luftwaffe" (German Airforces) as one station of a network of observatories, which should provide information on solar...
View ArticleScintillation noise power spectrum and its impact on high redshift 21-cm...
Visibility scintillation resulting from wave propagation through the turbulent ionosphere can be an important sources of noise at low radio frequencies ($\nu\lesssim 200$ MHz). Many low frequency...
View ArticleMethod for detection and reconstruction of gravitational wave transients with...
We present a method for detection and reconstruction of the gravitational wave (GW) transients with the networks of advanced detectors. Originally designed to search for transients with the initial GW...
View ArticleLow Latency transient search of Gravitational Waves for the Advanced...
The reliability of the first detection is one of the most interesting challenges for the gravitational wave community. To increase the detection confidence, the LIGO and Virgo collaborations have...
View Article"Asymptotic Parabola" Fits for Smoothing Generally Asymmetric Light Curves
A computer program is introduced, which allows to determine statistically optimal approxi-mation using the "Asymptotic Parabola" fit, or, in other words, the spline consisting of polynomials of order...
View ArticleLOFAR MSSS: Detection of a low-frequency radio transient in 400 hrs of...
We present the results of a four-month campaign searching for low-frequency radio transients near the North Celestial Pole with the Low-Frequency Array (LOFAR), as part of the Multifrequency Snapshot...
View ArticleWavelet-Based Techniques for the Gamma-Ray Sky
We demonstrate how the image analysis technique of wavelet decomposition can be applied to the gamma-ray sky to separate emission on different angular scales. New structures on scales that differ from...
View ArticleCTA telescopes as deep-space lasercom ground receivers
The amount of scientific data to be transmitted from deep-space probes is very limited due to RF-communications constraints. Free-space optical communication can alleviate this bottleneck, increasing...
View ArticleWavelet-Based Techniques for the Gamma-Ray Sky [Cross-Listing]
We demonstrate how the image analysis technique of wavelet decomposition can be applied to the gamma-ray sky to separate emission on different angular scales. New structures on scales that differ from...
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