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Swayamtrupta Panda

Researcher at Polish Academy of Sciences

Publications -  97
Citations -  1038

Swayamtrupta Panda is an academic researcher from Polish Academy of Sciences. The author has contributed to research in topics: Quasar & Active galactic nucleus. The author has an hindex of 16, co-authored 77 publications receiving 701 citations. Previous affiliations of Swayamtrupta Panda include Center for Theoretical Physics & Indian Institute of Astrophysics.

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Modeling of the Quasar Main Sequence in the Optical Plane

Swayamtrupta Panda, +6 more
- 18 Oct 2018 - 
TL;DR: In this paper, a physically motivated model was proposed to explain the distribution of quasars in the optical plane, where a hard X-ray power law uniquely tight to the disk at the basis of observational scaling, and the Broad Line Region distance was determined also from observational scaling.
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Failed Radiatively Accelerated Dusty Outflow Model of the Broad Line Region in Active Galactic Nuclei. I. Analytical Solution

Bozena Czerny, +9 more
- 13 Sep 2017 - 
TL;DR: In this paper, the authors adopt a theory-motivated approach to identify the principal mechanism responsible for the complex phenomenon of the Broad Line Region in Active Galactic Nuclei, where the role of dust is essential.
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The Quasar Main Sequence Explained by the Combination of Eddington Ratio, Metallicity, and Orientation

Swayamtrupta Panda, +2 more
- 04 Sep 2019 - 
TL;DR: In this paper, the effect of orientation of the accretion disk plane and the geometry of the broad-line region (BLR) on the distribution of quasars in the optical plane of the quasar main sequence was investigated.
Journal ArticleDOI

Modelling of the quasar main sequence in the optical plane

Swayamtrupta Panda, +6 more
- 22 Jun 2018 - 
TL;DR: In this article, the authors use a physically motivated model to explain the distribution of quasars in the optical plane and conclude that there is no single simple driver behind the sequence, as neither the Eddington ratio nor broad band spectrum shape plays the dominant role.
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Can Reverberation-measured Quasars Be Used for Cosmology?

Mary Loli Martínez-Aldama, +6 more
- 01 Oct 2019 - 
TL;DR: In this article, a correction for the time delay based on the dimensionless accretion rate considering the virial factor anti-correlated with the FWHM of H$\beta was proposed.