We are conducting a survey for distant solar system objects beyond the Kuiper Belt edge ( \sim 50 AU ) with new wide-field cameras on the Subaru and CTIO telescopes . We are interested in the orbits of objects that are decoupled from the giant planet region in order to understand the structure of the outer solar system , including whether a massive planet exists beyond a few hundred AU as first reported in Trujillo and Sheppard ( 2014 ) . In addition to discovering extreme trans-Neptunian objects detailed elsewhere , we have found several objects with high perihelia ( q > 40 AU ) that differ from the extreme and inner Oort cloud objects due to their moderate semi-major axes ( 50 < a < 100 AU ) and eccentricities ( e \lesssim 0.3 ) . Newly discovered objects 2014 FZ71 and 2015 FJ345 have the third and fourth highest perihelia known after Sedna and 2012 VP113 , yet their orbits are not nearly as eccentric or distant . We found several of these high perihelion but moderate orbit objects and observe that they are mostly near Neptune mean motion resonances and have significant inclinations ( i > 20 degrees ) . These moderate objects likely obtained their unusual orbits through combined interactions with Neptune ’ s mean motion resonances and the Kozai resonance , similar to the origin scenarios for 2004 XR190 . We also find the distant 2008 ST291 has likely been modified by the MMR+KR mechanism through the 6:1 Neptune resonance . We discuss these moderately eccentric , distant objects along with some other interesting low inclination outer classical belt objects like 2012 FH84 discovered in our ongoing survey .