activity
19972010
most citedCosmic dynamics in the era of Extremely Large Telescopes

258 citations · 590 across the 14 of their papers we have counts for

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Showing 2005Show all

7 papers · 1 filter

astro-ph2005

Most precise single redshift bound to the variability of the fine-structure constant

S. A. Levshakov, M. Centurion, P. Molaro +4

Verification of theoretical predictions of an oscillating behavior of the fine-structure constant, alpha, with cosmic time requires high precision measurements at individual redshi…

astro-ph2005

Most precise single redshift bound to Delta alpha/alpha

S. A. Levshakov, M. Centurion, P. Molaro +4

Verification of theoretical predictions of an oscillating behavior of the fine-structure constant alpha with cosmic time requires high precision Delta alpha/alpha measurements at i…

astro-ph2005

Spectral shape of the UV ionizing background and OVI absorbers at z ~ 1.5 towards HS0747+4259

D. Reimers, I. I. Agafonova, S. A. Levshakov +5

We report on high resolution spectra of the bright QSO HS0747+4259 (zem = 1.90, V = 15.8) observed to search for intermediate redshift OVI absorption systems. The spectra were obta…

astro-ph2005

Nitrogen-deficient and iron-rich associated absorbers with oversolar metallicities towards the quasar HE0141-3932

S. A. Levshakov, I. I. Agafonova, D. Reimers +3

HE0141-3932 (zem=1.80) is a bright blue radio-quite quasar which reveals an emission line spectrum with an unusually weak Ly-alpha line. In addition, large redshift differences (De…

astro-ph2005

Spectral energy distribution of the metagalactic ionizing radiation field from QSO absorption spectra

I. I. Agafonova, M. Centurion, S. A. Levshakov +1

A computational procedure is presented to estimate the spectral shape of the ionizing background between 1 and 10 Ryd by analyzing optically thin absorption systems in the spectra…

astro-ph2005

VLT/UVES shows no cosmological variability of alpha

P. Molaro, M. Centurion, S. D'Odorico +1

The cosmological variability of alpha is probed from individual observations of pairs of FeII lines. This procedure allows a better control of the systematics and avoids the influe…