Search results for "autocorrelation function"

showing 2 items of 2 documents

All-optical measurements of background, amplitude, and timing jitters for high speed pulse trains or PRBS sequences using autocorrelation function

2008

International audience; We present a simple method for all-optical measurements of background, amplitude, and timing jitters of ultra high speed pulse trains or PRBS sequences using the jitter dependence of the intercorrelation-peak shape. This method is numerically and experimentally demonstrated on a 42.66 Gbit/s PRBS sequence and then applied to measure the jitter growths occurring during the propagation of a 160-GHz pulse train in a classical SMF/DCF dispersion map.

Optical fiberOptical fiberAutocorrelation function02 engineering and technologyTiming and amplitude jitters01 natural sciencesPseudorandom binary sequencelaw.invention010309 optics020210 optoelectronics & photonicsOpticslaw0103 physical sciencesDispersion (optics)0202 electrical engineering electronic engineering information engineeringPulse waveElectrical and Electronic EngineeringInstrumentation40 Gbit/sJitter160 Gbit/sPhysicsHigh bit rate[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]business.industryAutocorrelationAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic MaterialsPulse (physics)AmplitudeControl and Systems EngineeringTelecommunication systembusiness
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Problems of Clustering of Radiogalaxies

2012

We present the preliminary analysis of clustering of a sample of 1157 radio-identified galaxies from Machalski & Condon (1999). We found that for separations $2-15 h^{-1}$Mpc their redshift space autocorrelation function $\xi(s)$ can be approximated by the power law with the correlation length $\sim 3.75h^{-1}$Mpc and slope $\gamma \sim 1.8$. The correlation length for radiogalaxies is found to be lower and the slope steeper than the corresponding parameters of the control sample of optically observed galaxies. Analysis the projected correlation function $\Xi(r)$ displays possible differences in the clustering properties between active galactic nuclei (AGN) and starburst (SB) galaxies.

PhysicsActive galactic nucleusCosmology and Nongalactic Astrophysics (astro-ph.CO)AutocorrelationFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsSpace (mathematics)Power lawGalaxyRedshiftCorrelation function (statistical mechanics)Space and Planetary Scienceautocorrelation functionradiogalaxiesCluster analysisAstrophysics::Galaxy AstrophysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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