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341.	H. Firouzjahi, M A. Gorji and A. Hosseini Mansoori, Instabilities in Mimetic Matter Perturbations, JCAP (to appear) [abstract] Code: IPM/A-2017/07

342.	S. Jazayeri, A. Vafaei Sadr and H. Firouzjahi, Primordial anisotropies from cosmic strings during inflation, Phys. Rev. D (to appear) [abstract] Code: IPM/A-2017/06

343.	M. Mosleh, S. Tacchella, A. Renzini, C. M. Carollo, A. Molaeinezhad, M. Onodera, H. G. Khosroshahi and S. Lilly, CONNECTION BETWEEN STELLAR MASS DISTRIBUTIONS WITHIN GALAXIES AND QUENCHING SINCE Z = 2, ApJ (to appear) [abstract] Code: IPM/A-2017/05

344.	CONNECTION BETWEEN STELLAR MASS DISTRIBUTIONS WITHIN GALAXIES AND QUENCHING SINCE Z = 2, arXiv (to appear) [abstract] Code: IPM/A-2017/05

345.	H. Moshafi, A. Sojasi, E. yusofi and M. Mohsenzadeh, Reconstruction of initial Asymptotic-de Sitter mode in light of the Planck data, JCAP (2017), [abstract] Code: IPM/A-2017/04

346.	T. Rostami, A. Karami and H. Firouzjahi, Effective field theory of statistical anisotropies for primordial bispectrum and gravitational waves, JCAP 2017(2017), 31 [abstract] Code: IPM/A-2017/46

347.	A. Molaeinezhad, J. Falcon-Barroso, I. MartÂ´Ä±nez-Valpuesta, H. G. Khosroshahi, A. Vazdekis, F. La Barbera, R. F. Peletier and M. Balcells, The imprints of bars on the vertical stellar population gradients of galactic bulges, MNRAS 467(2017), [abstract] Code: IPM/A-2017/45

348.	M. MOSLEH, S. TACCHELLA, A. RENZINI, C. M. A CAROLLO, A. MOLAEINEZHAD, M. ONODERA, H. G. KHOSROSHAHI and S. LILLY, Connection Between Stellar Mass Distributions Within Galaxies and Quenching Since z =2, ApJ 837(2017), [abstract] Code: IPM/A-2017/01

349.	Valerio. Faraoni, George. F. R. Ellis, Javad. T. Firouzjaee, Alexis. Helou and Ilia. Musco, Foliation dependence of black hole apparent horizons in spherical symmetry, Phys. Rev. D (2017), [abstract] Code: IPM/A-2016/23

350.	V. Vennin, H. Assadullahi, H. Firouzjahi, M. Noorbala and D. Wands, Critical Number of Fields in Stochastic Inflation, Phys. Rev. Lett. (2017), [abstract] Code: IPM/A-2016/12

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