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Michael T. Murphy

Researcher at Swinburne University of Technology

Publications -  369
Citations -  16602

Michael T. Murphy is an academic researcher from Swinburne University of Technology. The author has contributed to research in topics: Quasar & Redshift. The author has an hindex of 67, co-authored 340 publications receiving 14968 citations. Previous affiliations of Michael T. Murphy include University of Cambridge & Virginia Tech.

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Further Evidence for Cosmological Evolution of the Fine Structure Constant

TL;DR: The results of a search for time variability of the fine structure constant alpha using absorption systems in the spectra of distant quasars find no systematic effects which can explain the results.
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Laser Frequency Combs for Astronomical Observations

TL;DR: It is shown that tracking complex, time-varying systematic effects in the spectrograph and detector system is a particular advantage of laser frequency comb calibration, and this technique promises an effective means for modeling and removal of such systematic effects to the accuracy required by future experiments to see direct evidence of the universe's putative acceleration.
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Indications of a Spatial Variation of the Fine Structure Constant

TL;DR: New Very Large Telescope (VLT) data shows an inverse evolution; α increases at high redshift; the combined data set fits a spatial dipole, significant at the 4.2 σ level.
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Further evidence for a variable fine‐structure constant from Keck/HIRES QSO absorption spectra

TL;DR: In this paper, a detailed many-multiplet analysis of a third Keck/HIRES sample containing 78 absorption systems was presented, providing a total of 128 absorption systems over the redshift range 0.2 < zabs < 3.7.
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High‐precision wavelength calibration of astronomical spectrographs with laser frequency combs

TL;DR: In this paper, a new technique for precise wavelength calibration of high-resolution spectrographs using femtosecond-pulsed mode-locked lasers controlled by sta-ble oscillators such as atomic clocks is described.