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Feedback from active galactic nuclei (AGN) has proven to be a criticalingredient in the current picture of galaxy assembly and growth. However,observational constraints on AGN-driven outflows face technical challenges andas a result, the cold molecular gas outflow properties of type-1 AGN are notwell known. We present new IRAM NOrthern Extended Milimeter Array (NOEMA)observations of CO (1-0) in F07599+6508, Z11598$-$0112, F13342+3932, andPG1440+356, all nearby type-1 AGN and ultraluminous infrared galaxies (ULIRGs).We achieve spatial resolution of 1-3 arcsec corresponding to physical scales of2--8~kpc and spectral resolution of 15-60 km s$^{-1}$ which enables updated CO(1-0) redshifts and a detailed morphological view of the cold molecular gas inthese sources. The CO (1-0) luminosities, $L_{CO}^{\prime}$, are in the range2-12$\times 10^9$ K km s$^{-1}$ pc$^{2}$ and inferred molecular gas masses,$M$(H$_2$), are in the range 2-9$\times 10^9$ M$_{\odot}$. The velocity fieldsand gas distributions do not unambiguously identify any of these sources ashaving outflows. However, Z11598$-$0112 has signs of infalling material andafter the subtraction of a rotating disk model PG 1440+356 shows complexkinematics in the residuals that may indicate an outflow or warped disk.

Properties of cold molecular gas in four type-1 active galaxies hosting outflows