WE REQUEST SUPPORT FOR AN 80 KS XMM NEWTON AO 15 OBSERVATION OF THE RADIO AND GAMMA RAY LOUD NARROW LINE SEYFERT 1 NLS1 AGN PMN J0948+0022. THIS OBSERVATION WILL BE EXECUTED CONTEMPORANEOUSLY WITH A 200 KS NUSTAR POINTING IN ORDER TO OBTAIN THE HIGHEST POSSIBLE SIGNAL TO NOISE ACROSS A BROAD X RAY BANDPASS AS WELL AS SIMULTANEOUS UV OPTICAL DATA TO ANCHOR SEVERAL COMPETING CONTINUUM AND SOFT EXCESS MODELS. THE HIGH ACCRETION RATE AND RAPID VARIABILITY OF NLS1S MAKE THEM IDEAL CANDIDATES IN WHICH TO OBSERVE THE DISK/CORONA SYSTEM.