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Acknowledgements

The beginnings of this software were developed as part of research funded by the Verbundforschung of the BMBF/DLR under Grant No. 50 OR 9911 1 and by the DFG under Re 353/48. The use of this software in the work listed below (and any work not listed) is gratefully acknowledged. Particular thanks for Martin Wendt for providing feedback and test cases.

Work having used this software

MusE GAs FLOw and Wind (MEGAFLOW) V. The dust/metallicity-anisotropy of the Circum-Galactic Medium.
M. Wendt, F.N. Bouché, J. Zabl, I. Schroetter, S. Muzahid.
Monthly Notices of the Royal Astronomical Society, Advanced Access (2021).
DOI 10.1093/mnras/stab049.

The precision of line position measurements of unresolved quasar absorption lines and its influence on the search for variations of fundamental constants.
N. Prause and D. Reimers.
Astronomy & Astrophysics 555 A88 (2013).
DOI 10.1051/0004-6361/201118373.

Robust limit on a varying proton-to-electron mass ratio from a single H2 system.
M. Wendt and P. Molaro.
Astronomy & Astrophysics 526 A96 (2011).
DOI 10.1051/0004-6361/201014835.

HE 0515-4414: an unusual sub-damped Ly α system revisited. R. Quast, D. Reimers and R. Baade.
Astronomy and Astrophysics 477 (2) 443 (2008).
DOI 10.1051/0004-6361:20054773.

Most precise single redshift bound to Δα/α. S. A. Levshakov, M. Centurión, P. Molaro, et al.
Astronomy and Astrophysics 449 (3) 879 (2006).
DOI 10.1051/0004-6361:20053827.

Evolution strategies applied to the problem of line profile decomposition in QSO spectra. R. Quast, R. Baade and D. Reimers.
Astronomy and Astrophysics 431 (3) 1167 (2005).
DOI 10.1051/0004-6361:20041601.

Probing the variability of the fine-structure constant with the VLT/UVES. R. Quast, D. Reimers and S. A. Levshakov.
Astronomy and Astrophysics 415 (2) L7 (2004).
DOI 10.1051/0004-6361:20040013.

Detection of molecular hydrogen at z = 1.15 toward HE 0515-4414. D. Reimers, R. Baade, R. Quast, S. A. Levshakov.
Astronomy and Astrophysics 410 (3) 785 (2002).
DOI 10.1051/0004-6361:20031313.

Fine-structure diagnostics of neutral carbon toward HE 0515-4414. R. Quast, R. Baade and D. Reimers.
Astronomy and Astrophysics 386 (3) 796 (2002).
DOI 10.1051/0004-6361:20020342.

Data included with this software

Based on observations made with ESO Telescopes at the La Silla or Paranal Observatories under programme ID 066.A-0212.

Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555.