Calibration issues in estimating variability of the fine structure constant (alpha) with cosmic time

Details Calibration issues in estimating variability of the fine structure constant (alpha) with cosmic time Calibration issues in estimating variability of the fine structure constant (alpha) with cosmic time

2009-10-26

arxiv.org/abs/0910.4842v1

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

IAU 2009 JD9 conference proceeding, 4 pages, 2 figures. MmSAI, vol. 80 in press, eds. Paolo Molaro & Elisabeth Vangioni

Scientific paper

Laser Comb Wavelength calibration shows that the ThAr one is locally unreliable with possible deviations of up to 100 m/s within one order range, while delivering an overall 1 m/s accuracy (Wilken et al 2009). Such deviation corresponds to delta alpha/alpha ~ 7E-6 for a FeII-MgII pair. Comparison of line shifts among the 5 FeII lines, with almost identical sensitivity to fine structure constant changes, offers a clean way to directly test the presence of possible local wavelength calibration errors of whatever origin. We analyzed 5 absorption systems, with zabs ranging from 1.15 to 2.19 towards 3 bright QSOs. The results show that while some lines are aligned within 20 m/s, others reveal large deviations reaching 200 m/s or higher and corresponding to a delta alpha/alpha > 1E-5 level. The origin of these deviations is not clearly identified but could be related to the adaptation of wavelength calibration to CCD manufacturing irregularities. These results suggest that to draw conclusions from delta alpha/alpha analysis based on one or only few lines must be done with extreme care.

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