SIMBAD references

The TiO E³Π-X³Δ transition is an important opacity source in the near-infrared spectra of late M dwarfs. The 0-0 band of the ⁴⁸Ti¹⁶O E³Π-X³Δ electronic transition has been reanalyzed using a recently published set of high-resolution, high temperature absorption cross sections. The analysis has been extended to higher J values and an improved set of spectroscopic constants were determined. Calculated high-precision line lists for the 0-0 and 0-1 bands are provided with line strengths based on a previously measured experimental lifetime.