activity
20172026
most citedThe CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics

299 citations · 1.6k across the 115 of their papers we have counts for

collaborators
Showing 2019Show all

13 papers · 1 filter

astro-ph.HE2019

FeII emission in NLS1s -- originating from denser regions with higher abundances?

Swayamtrupta Panda, Paola Marziani, Bożena Czerny

The interpretation of the main sequence of quasars has become a frontier subject in the last years. The consider the effect of a highly flattened, axially symmetric geometry for th…

astro-ph.HE2019

FeII strength in NLS1s -- dependence on the viewing angle and FWHM

Swayamtrupta Panda, Paola Marziani, Bożena Czerny

We address the effect of orientation of the accretion disk plane and the geometry of the broad-line region (BLR) in the context of understanding the distribution of quasars along t…

astro-ph.HE2019

Generating AGN spectra for LSST: First steps

Swayamtrupta Panda, Bożena Czerny

In the near future, the arrival of new surveys promises a significant increment in the number of quasars (QSO) at large redshift ranges. This will help to constrain the dark energy…

astro-ph.HE2019

Explaining the Broad-line Region through photoionisation modelling

Swayamtrupta Panda

Broad-line regions (BLR) are one of the main components that constitute the phenomenological picture of active galaxies near the vicinity of the accreting supermassive black holes.…

astro-ph.GA2019★ 2 cited

A catalogue of 108 extended planetary nebulae observed by GALEX

Ananta C. Pradhan, Swayamtrupta Panda, Mudumba Parthasarathy +2

We present the ultraviolet (UV) imaging observation of planetary nebulae (PNe) using archival data of Galaxy Evolution Explorer (GALEX). We found 358 PNe detected by GALEX in near-…

astro-ph.GA2019★ 2 cited

Quasars from LSST as dark energy tracers: first steps

Mary Loli Martínez-Aldama, Swayamtrupta Panda, Bożena Czerny +1

In the near future, new surveys promise a significant increase in the number of quasars (QSO) at large redshifts. This will help to constrain the dark energy models using quasars.…