J-PAS: First identification, physical properties, and ionization efficiency of extreme emission line galaxies

Open Access

Table 2.

Computed emission line quantities for selected galaxies.

Tile ID	Number	Redshift	$ξ_{H α}^{()}$ $\xi_{\mathrm{H}\alpha}^{()}$	$ξ_{H β}^{()}$ $\xi_{\mathrm{H}\beta}^{()}$	F $_{H α}^{(* )}$ $_{\mathrm{H}\alpha}^{(*)}$	F $_{H β}^{(* )}$ $_{\mathrm{H}\beta}^{(*)}$	EW $_{H α}^{(* * )}$ $_{\mathrm{H}\alpha}^{(**)}$	EW $_{H β}^{(* * )}$ $_{\mathrm{H}\beta}^{(**)}$	EW $_{[O III] 5007}^{(* * )}$ $_{\mathrm{[O\,III]}\,5007}^{(**)}$
8838	7985	0.17	24.86 ± 0.42	25.14 ± 0.53	44.89 ± 6.95	22.83 ± 11.79	318.43 ± 49.33	106.25 ± 54.88	288.67 ± 58.11
8838	13110	0.46	–	24.99 ± 0.08	–	83.05 ± 7.71	–	148.55 ± 13.80	572.64 ± 20.79
8838	15288	0.398	–	24.55 ± 0.57	–	3.80 ± 8.82	–	25.09 ± 58.32	468.80 ± 55.12
8838	18374	0.586	–	24.80 ± 0.58	–	8.91 ± 8.25	–	65.80 ± 60.94	420.86 ± 55.43
...	...	...	...	...	...	...	...	...	...

Notes. ^( * ) in Hz erg⁻¹; ^( * *) in 10⁻¹⁹ erg s⁻¹ cm⁻² Å⁻¹; ^{( * * * )} in Å. The entire version of this table for the full sample of EELGs is available at the CDS.

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