2010MNRAS.409..808F


Query : 2010MNRAS.409..808F

2010MNRAS.409..808F - Mon. Not. R. Astron. Soc., 409, 808-820 (2010/December-1)

A method of detecting radio transients.

FRIDMAN P.A.

Abstract (from CDS):

Radio transients are sporadic signals, requiring that the backends of radio telescopes be equipped with the appropriate hardware and software for their detection. Observational programmes for detecting transients can be dedicated to that purpose or can rely upon observations made by other programmes. It is the single-dish single-transient (non-periodical) mode which is considered in this paper. Because neither the width of a transient nor the time of its arrival is known, a sequential analysis in the form of a cumulative sum (cusum) algorithm is proposed here. Computer simulations and real observation data processing are included to demonstrate the performance of the cusum. The use of the Hough transform is proposed here for the purpose of non-coherent de-dispersion. It is possible that the detected transients could be radio frequency interferences (RFI), and a procedure is proposed here which can distinguish between celestial signals and man-made RFI. This procedure is based on an analysis of the statistical properties of the signals.

Abstract Copyright: © 2010 The Author. Journal compilation © 2010 RAS

Journal keyword(s): methods: data analysis - methods: miscellaneous - methods: numerical - methods: statistical

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 PSR B0329+54 Psr 03 32 59.3370698592 +54 34 45.028206408           ~ 690 1

Query : 2010MNRAS.409..808F

Basic data :
PSR B0329+54 -- Pulsar
Other object types:
otypes_help
Rad (GB6,MY,...), Psr (PSR,PULS), * (Gaia), NIR (2MASS)
ICRS coord. (ep=J2000) :
03 32 59.3370698592 +54 34 45.028206408 (Optical) [ 0.4683 0.4608 90 ] A 2020yCat.1350....0G
FK4 coord. (ep=B1950 eq=1950) :
03 29 11.0039353995 +54 24 38.968936308 [ 0.4683 0.4608 90 ]
Gal coord. (ep=J2000) :
144.9949679143101 -01.2203063262975 [ 0.4683 0.4608 90 ]
Proper motions mas/yr :
5.020 -2.503 [0.582 0.657 90] A 2020yCat.1350....0G
Parallaxes (mas):
0.209 [0.6583] A 2020yCat.1350....0G
Fluxes (4) :
G 20.136793 [0.006418] C 2020yCat.1350....0G
J 17.093 [0.193] D 2003yCat.2246....0C
H 16.183 [0.203] D 2003yCat.2246....0C
K 15.556 [0.172] D 2003yCat.2246....0C
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Hierarchy : number of linked objects
whatever the membership probability is (see description here ) :

: 1
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Identifiers (16) :
An access of full data is available using the icon Vizier near the identifier of the catalogue

PSR B0329+54 NVSS J033259+543444 TGSSADR J033259.1+543442 WN B0329.1+5424
GB6 B0329+5425 PSR J0332+5434 TIC 316847481 WSTB 32W244
2MASS J03325936+5434448 PULS CP 0329 TXS 0329+544 Gaia DR2 445135392719883904
MY 032910.9+543447.0 PULS CP 0328 WN J0332+5434 Gaia DR3 445135392719883904

References (690 between 1850 and 2026) (Total 690)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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Collections of Measurements Description of Measurements

Distance : 1    Plx : 3    PM : 3   

   


External archives :

Data at NED - NASA/IPAC Extragalactic Database : PSR B0329+54

Link by name to the catalogue in VizieR :

2MASS J03325936+5434448 NVSS J033259+543444 WN J0332+5434 WN B0329.1+5424 Gaia DR2 445135392719883904
Gaia DR3 445135392719883904

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