Add to ORKGThe ESO Large Programme 185.A-0745 has awarded 10 nights on the VLT-UVES spectrograph for the study of the possible variation in the fine structure constant. We will present the fine-structure measurements from two lines of sight and several absorption systems. We will also present updated systematic error analyses
Aims. We analyze the consistency of different astronomical data of the variation in the fine-structu...
We assess the cosmological variability of the fine-structure constant α from the analysis of an ense...
Cosmological investigations, using high-redshift quasi-stellar object (QSO) absorption spectra, of p...
We present an analysis of 23 absorption systems along the lines of sight towards 18 quasars in the r...
We present a short review of the current quasar (QSO) absorption line constraints on possible variat...
Development of fundamental physics relies on the constancy of various fundamental quantities such as...
Development of fundamental physics relies on the constancy of various fundamental quantities such as...
Development of fundamental physics relies on the constancy of various fundamental quantities such as...
International audienceDevelopment of fundamental physics relies on the constancy of various fundamen...
International audienceDevelopment of fundamental physics relies on the constancy of various fundamen...
International audienceDevelopment of fundamental physics relies on the constancy of various fundamen...
International audienceDevelopment of fundamental physics relies on the constancy of various fundamen...
The fine-structure constant is a fundamental constant of the universe -- and widely thought to have ...
Development of fundamental physics relies on the constancy of various fundamental quantities such as...
Quasar absorption lines provide a precise test of whether the fine-structure constant, α, is the sam...
Aims. We analyze the consistency of different astronomical data of the variation in the fine-structu...
We assess the cosmological variability of the fine-structure constant α from the analysis of an ense...
Cosmological investigations, using high-redshift quasi-stellar object (QSO) absorption spectra, of p...
We present an analysis of 23 absorption systems along the lines of sight towards 18 quasars in the r...
We present a short review of the current quasar (QSO) absorption line constraints on possible variat...
Development of fundamental physics relies on the constancy of various fundamental quantities such as...
Development of fundamental physics relies on the constancy of various fundamental quantities such as...
Development of fundamental physics relies on the constancy of various fundamental quantities such as...
International audienceDevelopment of fundamental physics relies on the constancy of various fundamen...
International audienceDevelopment of fundamental physics relies on the constancy of various fundamen...
International audienceDevelopment of fundamental physics relies on the constancy of various fundamen...
International audienceDevelopment of fundamental physics relies on the constancy of various fundamen...
The fine-structure constant is a fundamental constant of the universe -- and widely thought to have ...
Development of fundamental physics relies on the constancy of various fundamental quantities such as...
Quasar absorption lines provide a precise test of whether the fine-structure constant, α, is the sam...
Aims. We analyze the consistency of different astronomical data of the variation in the fine-structu...
We assess the cosmological variability of the fine-structure constant α from the analysis of an ense...
Cosmological investigations, using high-redshift quasi-stellar object (QSO) absorption spectra, of p...