SIMBAD references

A collection of the best solar and laboratory spectra in the soft X-rays is used to perform a preliminary benchmark in this wavelength region, by comparing observed with predicted wavelengths and calibrated solar irradiances. The benchmark focuses on the FeIX - FeXIV ions, for which we have recently calculated the relevant atomic data; however, a few other ions have also been benchmarked. The iron ions dominate the soft X-rays, however a large fraction of the strongest soft X-ray lines due to n=4->n=3 transitions were previously unidentified. The strongest transitions are all identified here, in particular the decays from the core-excited levels (3s 3p^l 4s, l= 5,4,3,2,1 for FeX, FeXI, FeXII, FeXIII, and FeXIV, respectively), which are the strongest soft X-ray transitions from these ions. Many new identifications are proposed, some only tentatively. Good agreement in terms of solar irradiances between the soft-Xray and EUV (n=3->n=3) transitions is found, confirming the reliability of the new large-scale calculations. Some of the new atomic data and identifications are particularly important for the Solar Dynamic Observatory (SDO) Atmospheric Imaging Assembly (AIA) 94Å band.