Flux-density relation for traffic of army ants in a 3-lane bi-directional trail

2021 ◽  
Vol 567 ◽  
pp. 125664
Author(s):  
Smriti Pradhan ◽  
Swayamshree Patra ◽  
Yasar Efe Dai ◽  
Andreas Schadschneider ◽  
Debashish Chowdhury
Keyword(s):  
Flux Density ◽  
Army Ants ◽  
Density Relation

On the Spectral Index-Flux Density Relation for Large Samples of Radio Sources

2003 ◽  
Vol 3 (4) ◽  
pp. 347-358 ◽  
Author(s):  
Xi-Zhen Zhang ◽  
W. Reich ◽  
P. Reich ◽  
R. Wielebinski
Keyword(s):  
Flux Density ◽  
Spectral Index ◽  
Radio Sources ◽  
Large Samples ◽  
Density Relation

scholarly journals New results on the spectral index–flux density relation from the WENSS/NVSS catalogs

2003 ◽  
Vol 404 (1) ◽  
pp. 57-62 ◽  
Author(s):  
X. Zhang ◽  
W. Reich ◽  
P. Reich ◽  
R. Wielebinski
Keyword(s):  
Flux Density ◽  
Spectral Index ◽  
Density Relation

scholarly journals Surveys of Radio Sources at 5 GHz

1977 ◽  
Vol 74 ◽  
pp. 63-74
Author(s):  
I. I. K. Pauliny-Toth
Keyword(s):  
Flux Density ◽  
Radio Astronomy ◽  
Radio Sources ◽  
Astronomy Observatory ◽  
Max Planck ◽  
Radio Astronomy Observatory ◽  
Density Relation ◽  
Strong Source ◽  
Optical Identifications ◽  
5 Ghz

A number of surveys have been carried out at a frequency of 5 GHz at the National Radio Astronomy Observatory (NRAO) and at the Max-Planck-Institut für Radioastronomie (MPIfR), with the aim of determining the number-flux density relation for the sources detected and also of obtaining their radio spectra and optical identifications. The surveys fall into two categories: first, the strong source (S) surveys, which are intended in due course to cover the whole northern sky and to be complete above a flux density of about 0.6 Jy; second, surveys of limited areas of sky down to lower levels of the flux density.

scholarly journals Radio Source Counts at 408 MHz

1973 ◽  
Vol 26 (3) ◽  
pp. 417 ◽  
Author(s):  
BY Mills ◽  
IM Davies ◽  
JG Robertson
Keyword(s):  
Radio Source ◽  
Flux Density ◽  
High Exponent ◽  
Density Relation

Radio source counts at 408 MHz are investigated using the data from the first Molonglo catalogue (MC1) and an all-sky catalogue of strong sources. Earlier results are qualitatively confirmed. Possible explanations of the high exponent of the numberflux density relation between sources of strong and intermediate flux density are discussed briefly, but no firm conclusions seem possible.

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