no code implementations • 27 Jan 2021 • Sanna Gulati, Debbijoy Bhattacharya, Subir Bhattacharyya, Nilay Bhatt, C. S. Stalin, V. K. Agrawal
Based on the cumulative flux distribution of the gamma-ray lightcurve, we identified four distinct activity states and noticed an increase in the baseline flux during the first three states.
High Energy Astrophysical Phenomena
1 code implementation • 23 Oct 2019 • Suvendu Rakshit, C. S. Stalin, Jari Kotilainen
We performed a careful and homogeneous analysis of the SDSS spectra of these sources, to estimate the continuum and line properties of several emission lines such as H${\alpha}$, H${\beta}$, H${\gamma}$, Mg \textsc{ii}, C \textsc{iii]}, C \textsc{iv} and Ly${\alpha}$.
Astrophysics of Galaxies
