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A direct measurement of the universe's expansion history could be made by observing in real time the evolution of the cosmological redshift of distant objects.
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We thank the Kiepenheuer Institut für Sonnenphysik staff at the Vacuum Tower Telescope and the Instituto de Astrofisica de Canarias (IAC) personnel for their support during the measurements at the VTT. We especially appreciate the efforts of M. Collados (IAC) and F. Kerber (ESO). We thank T. Kippenberg for CW-laser assistance and J. Liske for advice on the manuscript. M.T.M. thanks the Australian Research Council for a QEII Research Fellowship (DP0877998)
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