Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars - II. Ages, metallicities, detailed elemental abundances, and connections to the Galactic thick disc

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Table 4:

Measured equivalent widths and calculated elemental abundances for each star $^{\dag }$ $\!$ .
			Sun			ob09076		mb09493		mb09133		mb09475		mb99022		mb09489		mb09456		mb09259
El.	$\lambda$	$\chi_{\rm l}$	$W_{\rm\lambda}$	X	flg	$W_{\rm\lambda}$	X	$W_{\rm\lambda}$	X	$W_{\rm\lambda}$	X	$W_{\rm\lambda}$	X	$W_{\rm\lambda}$	X	$W_{\rm\lambda}$	X	$W_{\rm\lambda}$	X	$W_{\rm\lambda}$	X
Al I	6696.023	3.14	38.3	6.51	0	-	-	20.6	5.99	20.4	6.06	-	-	28.6	6.30	37.5	6.45	47.7	6.64	-	-
Al I	6698.673	3.14	20.7	6.47	0	-	-	12.3	6.04	7.5	5.88	-	-	17.3	6.32	20.3	6.39	33.6	6.70	-	-

Notes. $^{(\dagger)}$ For each spectral line we give the lower excitation potential ( $\chi_{\rm l}$ ), measured equivalent widths ( $W_{\rm\lambda}$ ), derived absolute abundance ( $X \equiv \log \epsilon (X)$ ). We have only included the stars that are new to this work. The table is only available in electronic form at the CDS.

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