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Table 4

Summary of the information included in the released catalogue of classified nebulae.

Identification
index Unique identification number of the region
gal_name Name of the galaxy hosting the region
region_ID Identification number of the region within the galaxy
DIST Distance of the galaxy in Mpc(a)
Position and morphology
ra Right ascension of the Ha luminosity-weighted centre of the region
dec Declination of the Ha luminosity-weighted centre of the region
deproj_dist Deprojected distance from the nucleus of the galaxy (in arcsec)(a)
deproj_phi Deprojected position angle (0–2p)(a)
region_area Area of the region in pixels(b)
region_circ_rad Circularised radius of the region in arcsec
Spectral properties lineid should be replaced with the line ID reported in Table 2
lineid_FLUX Measured line flux in 10-20 erg cm-2 s-1
lineid_FLUX_ERR Measured line flux error in 10-20 erg cm-2 s-1
lineid_SNR S/N of the line
lineid_FLUX_DIG DIG corrected line flux in 10-20 erg cm-2 s-1
lineid_FLUX_ERR_DIG DIG corrected line flux error in 10-20 erg cm-2 s-1
lineid_SNR_DIG S/N of the line after the DIG correction
L_HA Ha luminosity in erg s-1
L_HA_DIG DIG corrected Ha luminosity in erg s-1
Kinematics The kinematics is reported only for the Ha and [N II]?6584 lines.
lineid_SIGMA Velocity dispersion of the line in km s-1 (c)
lineid_SIGMA_ERR Error on the velocity dispersion of the line in km s-1
lineid_VEL Velocity of the line in km s-1
lineid_VEL_ERR Error on the velocity of the line in km s-1
Classification
z_hii Evidence of the H II region models
z_pn Evidence of the PNe models
z_sh Evidence of the shock models
p_hii Probability of the H II region models
p_pn Probability of the PNe models
p_sh Probability of the shock models
c Final classification
Extinction
ebv Balmer decrement E(B - V) from measured fluxes
ebv_dig Balmer decrement E(B - V) from DIG corrected fluxes
ebv_sh E(B - V) estimated by IZI using shock models
ebv_hii E(B - V) estimated by IZI using H II region models
ebv_pn E(B - V) estimated by IZI using PNe models

Notes. (a)Distances from Anand et al. (2021), (b)pixel size: 0.2 arcsec pix−1, (c)corrected for instrumental broadening.

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