X-ray properties of intermediate-mass black holes in active galaxies

We present a pilot study of the X-ray properties of intermediate-mass (similar to 10(5)-10(6) M-circle dot) black holes in active galaxies using the Chandra X-ray telescope. Eight of the 10 active galaxies are detected with a significance of at least 3 sigma, with X-ray luminosities in the range L0.5-2keV approximate to 10(41)-10(43) ergs s(-1). The optical to X-ray flux ratios are consistent with expectations, given the known correlations between alpha(ox) and ultraviolet luminosity, while a couple of objects appear to be anomalously X-ray weak. The range of 0.5 to 2 keV photon indices we measure, 1 < Gamma(s) < 2.7, is entirely consistent with values found in samples of more luminous sources with more massive black holes. Black hole mass is evidently not a primary driver of soft X-ray spectral index. On the other hand, we do find evidence for a correlation between the X-ray power-law slope and both X-ray luminosity and Eddington ratio, which may suggest that X-ray emission mechanisms weaken at high Eddington ratios. Such a weakening may explain the anomalous X-ray weakness of one of our most optically luminous objects.