tokens: T.R. and D.H. are supported by the German Aerospace Center (DLR, grants 05 OR 1507 and 50 OR 1501, respectively). The GAVO project had been supported by the Federal Ministry of Education and Research (BMBF) at Tübingen (05 AC 6 VTB, 05 AC 11 VTB) and is funded at Heidelberg (05 AC 11 VH3). Financial support from the Belgian FRS-FNRS is also acknowledged. PQ is research director of this organization. Some of the data presented in this paper were obtained from the Mikulski Archive for Space Telescopes (MAST). STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. Support for MAST for non-HST data is provided by the NASA Office of Space Science via grant NNX09AF08G and by other grants and contracts. We thank Ralf Napiwotzki for putting the reduced ESO/VLT spectra at our disposal, Monica Raineri who sent us the electronic versions of the Kr iv ( Bredice et al. 2000 ) and Kr v ( Raineri et al. 2012 ) data, and Liang Liang who provided the Kr vii data ( Liang et al. 2013 ). This work used the profile-fitting procedure, OWENS, that was developed by M. Lemoine and the FUSE French Team. This research has made use of NASA’s Astrophysics Data System and the SIMBAD database, operated at CDS, Strasbourg, France. The TheoSSA service ( http://dc.g-vo.org/theossa ) used to retrieve theoretical spectra for this paper and the TOSS service ( http://dc.g-vo.org/TOSS ) that provides weighted oscillator strengths and transition probabilities were constructed as part of the activities of the German Astrophysical Virtual Observatory.
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