ILLUMINATING THE DISK/CORONA/JET CONNECTION IN NLS1 GALAXIES

We propose a 200ks NuSTAR observation of the radioloud narrow line Seyfert 1galaxy PMN J0948+0022, to be executed contemporaneously with an 80ks XMMNewtonobservation. The high accretion rate and rapid variability of NLS1s make themideal candidates in which to observe the disk/corona system, but there are onlya small handful of radioloud members of this population. The broadband Xrayand optical/UV spectra we obtain, along with information from existing Fermi andradio campaigns, will allow us to address some of the key questions regardingthe physics of jet formation in this critical sample, such as the physicalconditions under which a jet can be launched, the relation of the jet to theputative corona in AGN, and correlations with the inner accretion flow. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]