Swift Observations of the Narrow Line Seyfert 1 Galaxy RX J0134.2-4258

In my talk I will present results from Swift and XMM observations of the Narrow Line Seyfert 1 (NLS1) active galactic nuclei RX J0134.2-4258.  Swift monitoring was performed between 2007 and 2015 in X-rays as well as in the Ultraviolet. 
This source was previously observed by the ROSAT satellite in the 1990s, where it had one of the softest spectrums observed by the satellite. It was believed that the small black hole's high accretion rate may have destroyed its corona through radiation-driven outflows, and that the corona would recover over the following years leading up to the beginning of SWIFT's observation of the source. In addition we will also present the X-ray observations performed by XMM in 2008. Possible models to explain the observations will be discussed.