Multi-frequency study of the Pavo field

We test the prediction of Hamilton and Helfand (1993ApJ...418...55H) that faint radio selected galaxies are a new class contributing to the diffuse X-ray background (XRB)...我们对Hamilton与Helfand（1993ApJ...418...55H）提出的理论预言进行了检验，该预言指出暗弱射电选星系是一类可贡献弥散X射线背景（diffuse X-ray background，XRB）的新型天体类别。