activity
20092023
most citedThe origin of the Broad Line Region in Active Galactic Nuclei

271 citations · 942 across the 30 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

9 papers · 1 filter

astro-ph.CO2016

Tracing dark energy with quasars

J. Średzińska, B. Czerny, M. Bilicki +7

The nature of dark energy, driving the accelerated expansion of the Universe, is one of the most important issues in modern astrophysics. In order to understand this phenomenon, we…

astro-ph.CO2014

Quasars as tracers of cosmic flows

J. Modzelewska, B. Czerny, M. Bilicki +6

Quasars, as the most luminous persistent sources in the Universe, have broad applications for cosmological studies. In particular, they can be employed to directly measure the expa…

astro-ph.CO2014★ 17 cited

SALT long-slit spectroscopy of CTS C30.10: two-component Mg II line

J. Modzelewska, B. Czerny, K. Hryniewicz +7

Quasars can be used as a complementary tool to SN Ia to probe the distribution of dark energy in the Universe by measuring the time delay of the emission line with respect to the c…

astro-ph.CO2013★ 19 cited

SALT long-slit spectroscopy of LBQS 2113-4538: variability of the Mg II and Fe II component

K. Hryniewicz, B. Czerny, W. Pych +4

The Mg II line is of extreme importance in intermediate redshift quasars since it allows us to measure the black hole mass in these sources and to use these sources as probes of th…

astro-ph.CO2013★ 14 cited

Absorption features in the quasar HS 1603+3820 II. Distance to the absorber from photoionisation modelling

A. Rozanska, M. Nikolajuk, B. Czerny +4

We present photoionisation modelling of the intrinsic absorber in the bright quasar HS 1603+3820. We construct spectral energy distribution using optical/UV/X-ray observations as a…

astro-ph.CO2012★ 53 cited

Towards equation of state of dark energy from quasar monitoring: Reverberation strategy

B. Czerny, K. Hryniewicz, I. Maity +3

High redshift quasars can be used to deduce the distribution of dark energy in the Universe, as a complementary tool to SN Ia. The method is based on determination of the size of t…