Table 3
Spectral features identified in the observed spectra.
| λc | Width | ||
| [Å] | [Å] | Species | Transition |
|
|
|||
| 14 877.5 | Mg i |  – |
|
| 15 025.0 | Mg i |  – |
|
| 15 040.2 | * | Mg i | – |
| 15 168.4 | K i | 3d2D3/2– |
|
| 15 740.7 | Mg i |  –4d3D1 |
|
| 15 765.8 | * | Mg i | –4d3D3 |
| 15 888.4 | Si i |  –4p1P1 |
|
| 16 719.0 | Al i |  – |
|
| 16 750.5 | * | Al i |  – |
| 17 110.1 | Mg i | 4s1S0– |
|
Notes.Characteristic photospheric features of late-type stars between 14 500 Å and 18 000 Å. Features between 20 000 and 25 000 Å are listed in Table 2 of Daemgen et al. (2012). Asterisks mark lines that blend with the line with the next shortest wavelength (the previous entry in the list). Transitions selected from Cushing et al. (2005) and the NIST Atomic Spectra Database (http://www.nist.gov/pml/data/asd.cfm).
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