Karuppusamy et al., 2011 - Google Patents
A low frequency study of PSRs B1133+ 16, B1112+ 50, and B0031− 07Karuppusamy et al., 2011
View PDF- Document ID
- 15386092751774518999
- Author
- Karuppusamy R
- Stappers B
- Serylak M
- Publication year
- Publication venue
- Astronomy & Astrophysics
External Links
Snippet
We use the low frequency (110–180 MHz) capabilities of the Westerbork Synthesis Radio Telescope (WSRT) to characterise a large collection of single pulses from three low magnetic field pulsars. Using the Pulsar Machine II (PuMa-II) to acquire and coherently …
- 230000000051 modifying 0 abstract description 19
Classifications
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01S—RADIO DIRECTION-FINDING; RADIO NAVIGATION; DETERMINING DISTANCE OR VELOCITY BY USE OF RADIO WAVES; LOCATING OR PRESENCE-DETECTING BY USE OF THE REFLECTION OR RERADIATION OF RADIO WAVES; ANALOGOUS ARRANGEMENTS USING OTHER WAVES
- G01S7/00—Details of systems according to groups G01S13/00, G01S15/00, G01S17/00
- G01S7/02—Details of systems according to groups G01S13/00, G01S15/00, G01S17/00 of systems according to group G01S13/00
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01N—INVESTIGATING OR ANALYSING MATERIALS BY DETERMINING THEIR CHEMICAL OR PHYSICAL PROPERTIES
- G01N21/00—Investigating or analysing materials by the use of optical means, i.e. using infra-red, visible or ultra-violet light
- G01N21/17—Systems in which incident light is modified in accordance with the properties of the material investigated
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01S—RADIO DIRECTION-FINDING; RADIO NAVIGATION; DETERMINING DISTANCE OR VELOCITY BY USE OF RADIO WAVES; LOCATING OR PRESENCE-DETECTING BY USE OF THE REFLECTION OR RERADIATION OF RADIO WAVES; ANALOGOUS ARRANGEMENTS USING OTHER WAVES
- G01S13/00—Systems using the reflection or reradiation of radio waves, e.g. radar systems; Analogous systems using reflection or reradiation of waves whose nature or wavelength is irrelevant or unspecified
- G01S13/88—Radar or analogous systems specially adapted for specific applications
-
- G—PHYSICS
- G06—COMPUTING; CALCULATING; COUNTING
- G06F—ELECTRICAL DIGITAL DATA PROCESSING
- G06F17/00—Digital computing or data processing equipment or methods, specially adapted for specific functions
- G06F17/10—Complex mathematical operations
- G06F17/18—Complex mathematical operations for evaluating statistical data, e.g. average values, frequency distributions, probability functions, regression analysis
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01M—TESTING STATIC OR DYNAMIC BALANCE OF MACHINES OR STRUCTURES; TESTING STRUCTURES OR APPARATUS NOT OTHERWISE PROVIDED FOR
- G01M11/00—Testing of optical apparatus; Testing structures by optical methods not otherwise provided for
- G01M11/30—Testing of optical devices, constituted by fibre optics or optical waveguides
- G01M11/31—Testing of optical devices, constituted by fibre optics or optical waveguides with a light emitter and a light receiver being disposed at the same side of a fibre or waveguide end-face, e.g. reflectometers
- G01M11/3109—Reflectometers detecting the back-scattered light in the time-domain, e.g. OTDR
- G01M11/3136—Reflectometers detecting the back-scattered light in the time-domain, e.g. OTDR for testing of multiple fibers
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01R—MEASURING ELECTRIC VARIABLES; MEASURING MAGNETIC VARIABLES
- G01R23/00—Arrangements for measuring frequencies; Arrangements for analysing frequency spectra
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01R—MEASURING ELECTRIC VARIABLES; MEASURING MAGNETIC VARIABLES
- G01R13/00—Arrangements for displaying electric variables or waveforms
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01J—MEASUREMENT OF INTENSITY, VELOCITY, SPECTRAL CONTENT, POLARISATION, PHASE OR PULSE CHARACTERISTICS OF INFRA-RED, VISIBLE OR ULTRA-VIOLET LIGHT; COLORIMETRY; RADIATION PYROMETRY
- G01J11/00—Measuring the characteristics of individual optical pulses or of optical pulse trains
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01N—INVESTIGATING OR ANALYSING MATERIALS BY DETERMINING THEIR CHEMICAL OR PHYSICAL PROPERTIES
- G01N29/00—Investigating or analysing materials by the use of ultrasonic, sonic or infrasonic waves; Visualisation of the interior of objects by transmitting ultrasonic or sonic waves through the object
- G01N29/44—Processing the detected response signal, e.g. electronic circuits specially adapted therefor
- G01N29/46—Processing the detected response signal, e.g. electronic circuits specially adapted therefor by spectral analysis, e.g. Fourier analysis or wavelet analysis
Similar Documents
| Publication | Publication Date | Title |
|---|---|---|
| Karuppusamy et al. | Giant pulses from the Crab pulsar-A wide-band study | |
| Osłowski et al. | High signal-to-noise ratio observations and the ultimate limits of precision pulsar timing | |
| Farah et al. | Five new real-time detections of fast radio bursts with UTMOST | |
| Day et al. | High time resolution and polarization properties of ASKAP-localized fast radio bursts | |
| Sánchez-Monge et al. | STATCONT: A statistical continuum level determination method for line-rich sources | |
| Schaefer et al. | The SAMI Galaxy Survey: spatially resolving the environmental quenching of star formation in GAMA galaxies | |
| Ewall-Wice et al. | First limits on the 21 cm power spectrum during the Epoch of X-ray heating | |
| Stewart et al. | LOFAR MSSS: detection of a low-frequency radio transient in 400 h of monitoring of the North Celestial Pole | |
| Geyer et al. | The Thousand-Pulsar-Array programme on MeerKAT–III. Giant pulse characteristics of PSR J0540− 6919 | |
| Leloudas et al. | The properties of SN Ib/c locations | |
| Bilous et al. | A LOFAR census of non-recycled pulsars: extending to frequencies below 80 MHz | |
| Karuppusamy et al. | Crab giant pulses at low frequencies | |
| Karuppusamy et al. | A low frequency study of PSRs B1133+ 16, B1112+ 50, and B0031− 07 | |
| Barnacka et al. | First evidence of a gravitational lensing-induced echo in gamma rays with Fermi LAT | |
| Shannon et al. | Pulse intensity modulation and the timing stability of millisecond pulsars: a case study of PSR J1713+ 0747 | |
| Lindfors et al. | Optical and radio variability of the northern VHE gamma-ray emitting BL Lacertae objects | |
| Hales et al. | ATLAS 1.4 GHz Data Release 2–I. Observations of the CDF-S and ELAIS-S1 fields and methods for constructing differential number counts | |
| Greiner et al. | Probing dust-obscured star formation in the most massive gamma-ray burst host galaxies | |
| Aguilar et al. | Reconstructing the neutrino energy for in-ice radio detectors: A study for the Radio Neutrino Observatory Greenland (RNO-G) | |
| Song et al. | The Thousand-Pulsar-Array programme on MeerKAT–VIII. The subpulse modulation of 1198 pulsars | |
| Jessner et al. | Giant pulses with nanosecond time resolution detected from the Crab pulsar at 8.5 and 15.1 GHz | |
| Liu et al. | Single-pulse and profile-variability study of PSR J1022+ 1001 | |
| Pallavicini et al. | Stellar coronae with EXOSAT-Broad band spectroscopy of nearby coronal sources | |
| Miles et al. | Mode changing in J1909− 3744: the most precisely timed pulsar | |
| CN104266993A (en) | Article characteristic extraction method and device based on terahertz frequency band |