J-PLUS: Tools to identify compact planetary nebulae in the Javalambre and southern photometric local Universe surveys

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Volume 633 (January 2020)

A&A, 633 (2020) A123

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Table 2

Emission line fluxes of J-PLUS PN candidate.

Line	λ_rest (Å)	λ_Obs(Å)	F^(a)	I^(a)
[O II]^(b)	3727.0	3734.3	290.6	357.8
Hδ	4101.7	4108.4	24.8	28.7
Hγ	4340.5	4347.3	41.7	46.2
Hβ	4861.4	4869.1	100.0	100.0 O III>O III

	4958.9	4966.8	67.9	66.6 O III>O III

	5006.8	5014.8	199.4	193.7 He I>He I

	5875.6	5888.9	29.6	24.9
H α	6562.8	6573.5	373.7	288.5 N II>N II

	6583.4	6594.4	22.3	17.2 S II>S II

	6716.4	6727.3	53.2	40.3 S II>S II

	6730.8	6742.0	30.4	23.1

F(Hβ)^(c)	−	−	3.246	−

Notes. The five columns show, respectively, the line identification, the rest frame and observed central wavelengths, the observed fluxes, and the extinction corrected intensities. ^(a)In units of Hβ = 100. ^(b) Blended line. ^(c) In units of 10⁻¹⁵ erg cm⁻² s⁻¹.

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