We found that dust attenuation in star-forming galaxies depends on gas-phase metallicity at intermediate redshift. We analyzed the effect of morphology on dust attenuation, we found that compact objects are more attenuated.

However, we found that environment of galaxies does not play a role in shaping the attenuation of stellar emission. But subtle change in attenuation was observed between edge-on and face-on galaxies.

The complete study is in the PhD thesis of Mahmoud Hamed.

repository: github