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Table 2:

NIR spectroscopy. Emission lines are represented with the laboratory $(\lambda _{0})$ and fitted $(\lambda _{{\rm fit}})$ wavelengths.
    March 5 March 12
Identification $\lambda_{0}$ $\lambda_{{\rm fit}}$ Flux EW FWHM $\lambda_{{\rm fit}}$ Flux EW FWHM
  $\mu$m $\mu$m arbitrary Å Å $\mu$m arbitrary Å Å
[S III] 0.9531 - - - - 0.9911(1) $2724\pm226$ $-23\pm2$ $35\pm3$
He I/Pa $\gamma$ 1.0830/1.0935 1.1292(6) $1418\pm96$ $-168\pm11$ $222\pm18$ 1.1293(2) $19513\pm341$ $-155\pm3$ $182\pm4$
Pa $\beta$ 1.2820 - - - - 1.3330(5) $8621\pm531$ $-59\pm4$ $183\pm15$
Pa $\alpha$ 1.8751 1.9466(8) $1120\pm56$ $-170\pm8$ $279\pm21$ 1.9473(2) $12993\pm167$ ${-}120\pm1$ $269\pm4$

Source LaTeX | All tables | In the text