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111.	Haidar . Sheikhahmadi, Schwinger-Keldysh mechanism in extended quasi single field inflation, Eur. Phys. J. C 451(2019), [abstract] Code: IPM/A-2019/49

112.	P. Noterdaeme, S. Balashev, J.-K. Krogager, R. Srianand, H. Fathivavsari, P. Petitjean and C. Ledoux, Proximate Molecular Quasar Absorbers: Excess of damped H2 systems at zabs~zQSO in SDSS DR14, Astronomy & Astrophysics 627(2019), [abstract] Code: IPM/A-2019/48

113.	Abolhassan . Mohammadi, Khaled . Saaidi and Haidar . Sheikhahmadi, Constant-roll approach to non-canonical inflation, Phys. Rev. D 100(2019), [abstract] Code: IPM/A-2019/47

114.	Mahdeyeh . Naderi, Ali . Aghamohammadi, Abdollah . Refaei and Haidar . Sheikhahmadi, Intermediate inflation with non-canonical scalar field in the low anisotropy Universe, Mod. Phys. Lett. A 34(2019), [abstract] Code: IPM/A-2019/46

115.	Javad . T. Firouzjaee and Alireza . Allahyari, Black hole shadow with a cosmological constant for cosmological, Eur. Phys. J. C (2019), [abstract] Code: IPM/A-2019/45

116.	Haidar . Sheikhahmadi, Abolhassan . Mohammadi, Ali . Aghamohammadi, Tiberiu . Harko, RamÃ³n. Herrera, Christian . Corda, Amare . Abebe and Khaled . Saaidi, Constraining chameleon field driven warm inflation with Planck 2018 data, Eur. Phys. J. C (2019), [abstract] Code: IPM/A-2019/44

117.	S. Modares Vamegh, M. Haghighat, S. Mahmoudi and R. Mohammadi, Impact of the vector dark matter on polarization of the CMB photon, 100(2019), [abstract] Code: IPM/A-2019/40

118.	Maryam. Torki, Atefeh. Javadi, Jacco Th. van Loon and Hossein. Safari, The star formation history of the M31 galaxy derived from Long-Period-Variable star counts, IAU 14(2019), [abstract] Code: IPM/A-2019/39

119.	Seyed Azim . Hashemi , Atefeh . Javadi and Jacco . Th. van Loon , Recovering the Star Formation History of IC1613 Dwarf Galaxy Using Evolved Stars, IAU 14(2019), [abstract] Code: IPM/A-2019/38

120.	Atefeh . Javadi and Jacco . Th. van Loon , AGB population as probes of galaxy structure and evolution, IAU 14(2019), [abstract] Code: IPM/A-2019/37

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