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20112022
most citedDeep Learning in Searching the Spectroscopic Redshift of Quasars

17 citations · 24 across the 4 of their papers we have counts for

collaborators

8 papers

astro-ph.HE202217 cited

Deep Learning in Searching the Spectroscopic Redshift of Quasars

F. Rastegar Nia, M. T. Mirtorabi, R. Moradi +2

Studying the cosmological sources at their cosmological rest-frames is crucial to track the cosmic history and properties of compact objects. In view of the increasing data volume…

astro-ph.GA2021

INT monitoring survey of Local Group dwarf galaxies: star formation history and chemical enrichment

Tahere Parto, Shahrzad Dehghani, Atefeh Javadi +12

The Local Group (LG) hosts many dwarf galaxies with diverse physical characteristics in terms of morphology, mass, star formation, and metallicity. To this end, LG can offer a uniq…

gr-qc2019

Chameleon Mechanism in Inhomogeneous Astrophysical Objects

Noshad Khosravi Largani, Mohammad Taghi Mirtorabi

Observational evidence implying the accelerated expansion of the universe has been the motivation to develop various classes of modified gravity theories. One of them uses the so-c…

astro-ph.SR2018

Linear Polarization Features in the Quiet-Sun Photosphere: Structure and Dynamics

S. Kianfar, S. Jafarzadeh, M. T. Mirtorabi +1

We present detailed characteristics of linear polarization features (LPFs) in the quiet-Sun photosphere from high resolution observations obtained with Sunrise/IMaX. We explore dif…

astro-ph.SR2018

The Delta Scuti star 38 Eri from the ground and from space

M. Paparo, Z. Kollath, R. R. Shobbrook +17

We present and discuss the pulsational characteristics of the Delta Scuti star 38 Eri from photometric data obtained at two widely spaced epochs, partly from the ground (1998) and…

gr-qc2018

Red Giant evolution in Modified Gravity

Sh. Najafi, M. T. Mirtorabi, Z. Ansari +1

In this paper, we study the chameleon profile in inhomogeneous density distributions and find that the fifth force in thin shell near the surface is weaker from what expected in ho…