ACCURATE LABORATORY WAVELENGTHS OF THE 1910 Å Ti II RESONANCE TRANSITIONS RELEVANT TO STUDIES OF POSSIBLE VARIATIONS OF THE FINE-STRUCTURE CONSTANT
- 18 November 2010
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 725 (1), 424-429
- https://doi.org/10.1088/0004-637x/725/1/424
Abstract
No abstract availableThis publication has 29 references indexed in Scilit:
- WAVELENGTH ACCURACY OF THE KECK HIRES SPECTROGRAPH AND MEASURING CHANGES IN THE FINE STRUCTURE CONSTANTThe Astrophysical Journal, 2009
- Precision spectroscopy of thefine-structure doublet inPhysical Review A, 2009
- Laboratory wavelengths for cosmological constraints on varying fundamental constantsPhysica Scripta, 2009
- Accurate laboratory ultraviolet wavelengths for quasar absorption-line constraints on varying fundamental constantsMonthly Notices of the Royal Astronomical Society, 2006
- Frequency metrology on theline for comparison with quasar dataPhysical Review A, 2006
- Probing the cosmological variation of the fine-structure constant: Results based on VLT-UVES sampleAstronomy & Astrophysics, 2004
- Space-Time Variation of Physical Constants and Relativistic Corrections in AtomsPhysical Review Letters, 1999
- Measurement of the refractive index of air and comparison with modified Edl n's formulaeMetrologia, 1998
- Wavelength calibration of Fourier-transform emission spectra with applications to Fe iJournal of the Optical Society of America B, 1988
- High precision fourier transform spectrometry: The critical role of phase correctionsMicrochimica Acta, 1987