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19952026
most citedH0LiCOW XIII. A 2.4% measurement of from lensed quasars: tension between early and late-Universe probes

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Showing 2007Show all

8 papers · 1 filter

astro-ph2007★ 51 cited

Simultaneous Estimation of Time Delays and Quasar Structure

Christopher W. Morgan, Michael E. Eyler, C. S. Kochanek +5

We expand our Bayesian Monte Carlo method for analyzing the light curves of gravitationally lensed quasars to simultaneously estimate time delays and quasar structure including the…

astro-ph2007★ 43 cited

ZEN2: A narrow J-band search for z~9 Lya emitting galaxies directed towards three lensing clusters

J. P. Willis, F. Courbin, J. P. Kneib +1

We present the results of a continuing survey to detect Lya emitting galaxies at redshifts z~9: the ZEN ("z equals nine'') survey. We have obtained deep VLT/ISAAC observations in t…

astro-ph2007★ 12 cited

Slit and integral-field optical spectroscopy of the enigmatic quasar HE0450-2958

G. Letawe, P. Magain, F. Courbin

Interest in the quasar HE0450-2958 arose following the publication of the non-detection of its expected massive host, leading to various interpretations. This article investigates…

astro-ph2007★ 67 cited

Microlensing variability in the gravitationally lensed quasar Q2237+0305 = the Einstein Cross, I. Spectrophotometric monitoring with the VLT

A. Eigenbrod, F. Courbin, D. Sluse +2

We present the results of the first long-term (2.2 years) spectroscopic monitoring of a gravitationally lensed quasar, namely the Einstein Cross Q2237+0305. The goal of this paper…

astro-ph2007★ 34 cited

Spatial decomposition of on-nucleus spectra of quasar host galaxies

Knud Jahnke, Lutz Wisotzki, Frederic Courbin +1

In order to study the host galaxies of type 1 (broad-line) quasars, we present a semi-analytic modelling method to decompose the on-nucleus spectra of quasars into nuclear and host…

astro-ph2007★ 2 cited

DECPHOT: an optimal deconvolution-based photometric reduction method

M. Gillon, P. Magain, V. Chantry +5

A high accuracy photometric reduction method is needed to take full advantage of the potential of the transit method for the detection and characterization of exoplanets, especiall…