Title: Using quasars as standard clocks for measuring cosmological redshift Authors: De-Chang Dai, Glenn D. Starkman, Branislav Stojkovic, Dejan Stojkovic, Amanda Weltman
We report hitherto unnoticed patterns in quasar light curves. We characterise segments of quasars' light curves with the slopes of the straight lines fit through them. These slopes appear to be directly related to the quasars' redshifts. Alternatively, using only global shifts in time and flux, we are able to find significant overlaps between the light curves of different pairs of quasars by fitting the ratio of their redshifts. We are then able to reliably determine the redshift of one quasar from another. This implies that one can use quasars as standard clocks, as we explicitly demonstrate by constructing two independent methods of finding the redshift of a quasar from its light curve.
The sample of quasars with different redshifts. Time is transformed to the quasar rest frame (i.e. divided by (z +1)). A pattern emerges, some parallel lines (same slopes) appear. We mark them with the thin black lines. A possible shallower, long-term trend is indicated by thick green lines.
Title: A new cosmological distance measure using AGN Authors: D. Watson (1), K. D. Denney (1), M. Vestergaard (1), T. M. Davis (2) ((1) Dark Cosmology Centre, U. Copenhagen, (2) U. Queensland)
Accurate distances to celestial objects are key to establishing the age and energy density of the Universe and the nature of dark energy. A distance measure using active galactic nuclei (AGN) has been sought for more than forty years, as they are extremely luminous and can be observed at very large distances. We report here the discovery of an accurate luminosity distance measure using AGN. We use the tight relationship between the luminosity of an AGN and the radius of its broad line region established via reverberation mapping to determine the luminosity distances to a sample of 38 AGN. All reliable distance measures up to now have been limited to moderate redshift -- AGN will, for the first time, allow distances to be estimated to z~4, where variations of dark energy and alternate gravity theories can be probed.