We explore the possibility to make use of cosmological data to look for signatures of unknown heavy particles whose masses are on the order of the Hubble parameter during the time of inflation. To be more specific we take up the quasi-single field inflation model, in which the isocurvaton $sigma $ is supposed to be the heavy particle. We study correlation functions involving both scalar ($zeta $) and tensor ($gamma $) perturbations and search for imprints of the $sigma$-particle effects. We make use of the technique of the effective field theory for inflation to derive the $zeta sigma $ and $gamma zeta sigma $ couplings. With these couplings we compute the effects due to $sigma $ to the power spectrum $langle zeta zeta rangle $ and correlations $langle gamma^{s} zeta zeta rangle$ and $langle gamma^{s_{1}} gamma ^{s_{2}} zeta zeta rangle $, where $s$, $s_{1}$ and $s_{2}$ are the polarization indices of gravitons. Numerical analyses of the $sigma$-mass effects to these corrlations are presented. It is argued that future precise observations of these correlations could make it possible to measure the $sigma$-mass and the strength of the $zeta sigma$ and $gamma zeta sigma$ couplings. As an extension to the $N$-graviton case we also compute the correlations $langle gamma ^{s_{1}} cdots gamma ^{s_{N}} zeta zeta rangle $ and $langle gamma ^{s_{1}} cdots cdots gamma ^{s_{2N}} zeta zeta rangle $ and their $sigma$-mass effects. It is suggested that larger $N$ correlation functions are useful to probe larger $sigma$-mass .
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