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6dFGS gJ190300.3-492201

Observation

Spectrum ID476880179_sp1
Alt nameg1903003-492201
z0.0503
RA, Dec285.7512, -49.3669
MJD60080.73
SNR/Å B/R15.1/21.3
Obs Airmass1.05
SMSS ID476880179
Closest SMSS10.86'', 476880177
SMSS Mean r6"ap16.0 ± 0.1
2MASS Kextnan ± nan

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.047
Power law αν-0.63 ± 0.11
log L5100,AGN43.47 ± 0.02
log HβBr/[O III]-0.38 ± 0.02
log ML5100/M7.82 ± 0.03
log M/M7.25 ± 0.02
log M/M7.67 ± 0.05
log M[O III]/M7.99 ± 0.03

Spatial extraction & sky subtraction region

Spatial plot

Spaxel scale: 1 arcsec² — Flux units: erg s⁻¹ cm⁻² Å⁻¹
Apertures: object (solid), background (dashed)

Spectrum decomposition

Emission line measurements

Linelog L (erg s⁻¹)FWHM (km s⁻¹)σ (km s⁻¹)EW (Å)
Hγ Narrow40.71 ± 0.02235 ± 62172 ± 267.08 ± 0.32
Hγ Broad40.88 ± 0.063834 ± 3221503 ± 5510.20 ± 0.75
[O III] 436440.13 ± 0.07227 ± 6293 ± 251.87 ± 0.17
He II Narrow40.08 ± 0.07227 ± 6293 ± 251.85 ± 0.17
He II Broad40.83 ± 0.065113 ± 1952171 ± 8210.57 ± 0.80
Hβ Narrow41.08 ± 0.01235 ± 62172 ± 2619.36 ± 0.33
Hβ Broad41.31 ± 0.023744 ± 1361400 ± 4331.88 ± 0.74
[O III] 500741.68 ± 0.01235 ± 62172 ± 2680.66 ± 0.37
He I Narrow39.90 ± 0.08227 ± 6293 ± 251.67 ± 0.16
He I Broad40.69 ± 0.042841 ± 1431206 ± 6010.53 ± 0.59
[O I] 630040.35 ± 0.02227 ± 6293 ± 255.08 ± 0.23
Hα Narrow41.56 ± 0.01227 ± 6293 ± 2587.45 ± 0.32
Hα Broad41.89 ± 0.012553 ± 671160 ± 41189.82 ± 1.27
[N II] 658541.02 ± 0.01227 ± 6293 ± 2525.63 ± 0.26
[S II] 671840.84 ± 0.01227 ± 6293 ± 2517.16 ± 0.21
[S II] 673240.73 ± 0.01227 ± 6293 ± 2513.59 ± 0.20

All narrow line widths are tied to narrow [O III] 5007Å. [O III] 5007Å and narrow Hβ include a second narrow component not tied to other narrow lines.

Emission summary

Hα Broad SNR18.74
Hβ Broad SNR5.03
Hγ Broad SNR2.08
AGN frac0.71
Host frac0.29
log L5100,Host43.09
Fe II/Hβ0.26
Fe II/[O III]0.11

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer0
balmer_snr1
hb_width0
balmer_width0

Hα mass estimates from Cho+2023. Remaining mass estimates from R–L relations in Wang & Woo 2024 and zero-points from Amrutha+2026.