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6dFGS gJ185630.1-285502

Observation

Spectrum ID230101829_sp1
Alt nameg1856301-285502
z0.0992
RA, Dec284.1253, -28.9172
MJD60080.74
SNR/Å B/R11.2/13.6
Obs Airmass1.00
SMSS ID230101829
Closest SMSS8.53'', 230101830
SMSS Mean r6"ap17.1 ± 0.1
2MASS Kext12.9 ± 0.1

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.162
Power law αν-1.49 ± 0.06
log L5100,AGN43.73 ± 0.02
log HβBr/[O III]0.29 ± 0.03
log ML5100/M7.70 ± 0.03
log M/M7.67 ± 0.03
log M/M7.73 ± 0.04
log M[O III]/M7.76 ± 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 Narrow40.18 ± 0.34400 ± 63349 ± 281.32 ± 0.72
Hγ Broad41.53 ± 0.043276 ± 1351068 ± 3528.46 ± 1.03
[O III] 436439.91 ± 0.40368 ± 63156 ± 250.71 ± 0.47
He II Narrow39.84 ± 0.41368 ± 63156 ± 250.62 ± 0.38
He II Broad40.58 ± 0.181180 ± 63501 ± 253.40 ± 0.75
Hβ Narrow40.95 ± 0.06400 ± 63349 ± 288.17 ± 0.77
Hβ Broad41.98 ± 0.022844 ± 1081853 ± 8987.50 ± 2.39
[O III] 500741.69 ± 0.01400 ± 63349 ± 2846.08 ± 0.89
He I Narrow40.50 ± 0.08368 ± 63156 ± 253.20 ± 0.38
He I Broad41.10 ± 0.084915 ± 1312087 ± 5512.71 ± 1.40
[O I] 630039.92 ± 0.29368 ± 63156 ± 250.88 ± 0.40
Hα Narrow41.22 ± 0.03368 ± 63156 ± 2517.95 ± 0.48
Hα Broad42.48 ± 0.012733 ± 671307 ± 46319.54 ± 2.82
[N II] 658541.16 ± 0.03368 ± 63156 ± 2515.50 ± 0.64
[S II] 671840.66 ± 0.06368 ± 63156 ± 254.92 ± 0.51
[S II] 673240.71 ± 0.06368 ± 63156 ± 255.59 ± 0.51

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 SNR20.18
Hβ Broad SNR7.18
Hγ Broad SNR3.86
AGN frac0.61
Host frac0.39
log L5100,Host43.54
Fe II/Hβ0.52
Fe II/[O III]1.00

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer0
balmer_snr0
hb_width1
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.