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211.	I. Heywood, M. J. Jarvis, C. L. Hale, I. H. Whittam, H. L. Bester, B. Hugo, J. S. Kenyon, M. Prescott, O. M. Smirnov, C. Tasse, J. M. Afonso, P. N. Best, J. D. Collier, R. P. Deane, B. S. Frank, M. J. Hardcastle, K. Knowles, N. Maddox, E. J. Murphy, I. Prandoni, S. M. Randriamampandry, M. G. Santos, S. Sekhar, F. Tabatabaei, A. R. Taylor and K. Thorat, MIGHTEE: Total intensity radio continuum imaging and the COSMOS / XMM-LSS Early Science fields, MNRAS (2021), [abstract] Code: IPM/A-2021/17

212.	M. Khodadi, U. Kumar Dey and G. Lambiase, Strongly magnetized hot QCD matter and stochastic gravitational wave background, Phys. Rev. D 104(2021), 17 [abstract] Code: IPM/A-2021/16

213.	M. Khodadi, G. Lambiase and D. F. Mota, No-hair theorem in the wake of Event Horizon Telescope, JCAP (2021), [abstract] Code: IPM/A-2021/15

214.	Y. Tavakoli, Cosmological Particle Production in Quantum Gravity, Universe 7(2021), [abstract] Code: IPM/A-2021/14

215.	H. Firouzjahi, M A. Gorji, Sh. Mukohyama and B. Salehian, Dark photon dark matter from charged inflaton, Journal of High Energy Physics (JHEP) (2021), [abstract] Code: IPM/A-2021/13

216.	M H. Zhoolideh Haghighi, S. Rahvar and M R. Rahimi Tabar, Phase Transition in Modified Newtonian Dynamics (MONDian) Self-Gravitating Systems, Entropy 23(2021), [abstract] Code: IPM/A-2021/12

217.	M. Heydarzadeh, M. mohsenzadeh, M. Abbasian-Motlaq and E. Yusofi, Asymptotic de Sitter inflation in different geometric backgrounds, Int. J. Geom. Methods Mod. Phys. (2021), [abstract] Code: IPM/A-2021/11

218.	M M. Motiei, M. Hosseinirad and Sh. Abbassi, Gravitational instability of non-isothermal filamentary molecular clouds, in presence of external pressure, MNRAS 502(2021), [abstract] Code: IPM/A-2020/43

219.	M. Roshan, I. Banik, N. Ghafourian, I. Thies, B. Famaey, E. Asencio and P. Kroupa, Barred spiral galaxies in modified gravity theories, MNRAS 503(2021), [abstract] Code: IPM/A-2020/42

220.	M . Trevisan, G A . Mamon and H . G Khosroshahi, Erratum: Do the stellar populations of the brightest two group galaxies depend on the magnitude gap, MNRAS 503(2021), [abstract] Code: IPM/A-2021/10

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