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We present a new web‐tool – N et ‐PSIC o NS – for population synthesis of isolated near‐by cooling neutron stars (NSs). The main aim is to provide an easy test of models of the NS thermal evolution which can be used by groups studying this subject. A user can upload cooling curves for a set of masses, modify the mass spectrum if necessary, change radii to fit the EoS used for cooling curve calculations, and then a population synthesis of close‐by isolated cooling NSs is performed. The output includes the log  N  ‐log  S  distribution confronted with the ROSAT observations and several other sets of data. In this paper, we summarize the idea of the test proposed by Popov et al. (2006), and present a user's manual for the web‐tool (© 2011 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)

A web‐tool for population synthesis of near‐by cooling neutron stars: An on‐line test for cooling curves