“Ahamad mehrabi”

Email: 

IPM Positions

Resident Researcher, School of Astronomy


Research Interests

Microlensing structure formation

Research Activities

Kepler satellite provides a high accuracy data and can be used to detect acctivity of stars. In this work we are giong to study acctivity of stars with the data set.

Present Research Project at IPM

Activity of stars with kepler data

Related Papers

1. Hadis. Goodarzi, Ahmad. Mehrabi, Habib. Khosroshahi and Han. He
Flare Activity and Magnetic Feature Analysis of the Flare Stars. II. Subgiant Branch
Astrophysical Journal 906 (2021),   [abstract]
Code: IPM/A-2020/31
2. Hadis . Goodarzi, Ahmad . Mehrabi, Habib . khosroshahi and Han . He
Flare Activity and Magnetic Feature Analysis of the Flare Stars
Astrophysical Journal Supplement Series 244 (2019),   [abstract]
Code: IPM/A-2019/21
3. Ahmad. Mehrabi and Han. He
Magnetic activity properties of M-type kepler stars
ELSEVIER 66 (2019), 31-39  [abstract]
Code: IPM/A-2018/33
4. Han. He, Huaning. Wang, Mei. Zhang, Ahmad. Mehrabi, Yan. Yan and Duo. Yun
Phase difference between long-term magnetic feature activity and flare activity of solar-type stars
IAU 13 (2018), 217-220  [abstract]
Code: IPM/A-2018/35
5. Han. He, Huaning. Wang, Mei. Zhang, Ahmad. Mehrabi, Yan. Yan and Duo. Yun
Activity Analyses for Solar-type Stars Observed with Kepler. II. Magnetic Feature versus Flare Activity
Astrophysical Journal 236 (2018),   [abstract]
Code: IPM/A-2018/34
6. T. Naderi, A. Mehrabi and S. Rahvar
Primordial black hole detection through diffractive microlensing
Int. J. Mod. Phys. D 97 (2018),   [abstract]
Code: IPM/A-2018/20
7. Ahmad . Mehrabi, Han . He and Habib . Khosroshahi
MAGNETIC ACTIVITY ANALYSIS FOR A SAMPLE OF G-TYPE MAIN SEQUENCE KEPLER TARGETS
Astrophysical Journal 834 (2017),   [abstract]
Code: IPM/A-2016/30
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