CONFUSION NOISE AND SOURCE CLUSTERING

被引:40
作者
BARCONS, X [1 ]
机构
[1] UNIV CANTABRIA,INST ESTUDIOS AVANZADO FIS MODERNA & BIOL MOLEC,CSIC,SANTANDER,SPAIN
关键词
METHODS; ANALYTICAL; NUMERICAL; RADIO CONTINUUM; GALAXIES;
D O I
10.1086/171733
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The influence of source clustering on the distribution of fluctuations in integrated background radiations [the P(D) curve] is analyzed. The general framework to model the P(D) curve given the beam profile, the source counts (the log N-log S relation), and the source correlation functions is presented. It is then shown that an account of source clustering in terms of an excess variance [i.e., via the convolution of the model P(D) curves with a Gaussian] is generally inappropriate. Since the correct way to account for source clustering requires all of the n-point source correlation functions, and there is little or no observational information of these quantities for n > 2, simple models with few parameters are presented, namely, a Gaussian clustering model and a shot noise clustering model. To illustrate the effects of source clustering in the determination of source counts via analysis of confusion noise, simulations with the shot noise clustering model and a top-hat beam are generated and P(D) curves subsequently fitted. The amount by which source counts are overestimated if clustering is not properly accounted for is quantified.
引用
收藏
页码:460 / 468
页数:9
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