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6dFGS gJ140125.6-491314

Observation

Spectrum ID322999424_sp1
Alt nameg1401256-491314
z0.0723
RA, Dec210.3565, -49.2206
MJD60379.76
SNR/Å B/R9.1/13.5
Obs Airmass1.09
SMSS ID322999424
Closest SMSS13.25'', 322999423
SMSS Mean r6"ap17.2 ± 0.1
2MASS Kext12.4 ± 0.1

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.193
Power law αν-1.75 ± 0.21
log L5100,AGN42.59 ± 0.25
log HβBr/[O III]0.03 ± 0.02
log ML5100/M7.46 ± 0.12
log M/M7.80 ± 0.02
log M/M7.75 ± 0.04
log M[O III]/M7.88 ± 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 Narrow39.72 ± 0.33317 ± 63218 ± 276.70 ± 3.77
Hγ Broad41.07 ± 0.051897 ± 3601161 ± 70149.78 ± 8.37
[O III] 436439.34 ± 0.40301 ± 63127 ± 252.79 ± 2.26
He II Narrow39.93 ± 0.15301 ± 63127 ± 2511.19 ± 1.95
He II Broad39.96 ± 0.301348 ± 75572 ± 3111.54 ± 4.32
Hβ Narrow40.33 ± 0.07317 ± 63218 ± 2728.23 ± 3.50
Hβ Broad41.47 ± 0.023798 ± 1011436 ± 30383.57 ± 7.72
[O III] 500741.44 ± 0.01317 ± 63218 ± 27363.05 ± 3.95
He I Narrow39.87 ± 0.23301 ± 63127 ± 2510.12 ± 2.96
He I Broad40.90 ± 0.065118 ± 1022173 ± 43110.03 ± 8.64
[O I] 630040.02 ± 0.09301 ± 63127 ± 2514.62 ± 1.90
Hα Narrow40.98 ± 0.02301 ± 63127 ± 25136.54 ± 2.37
Hα Broad42.08 ± 0.014167 ± 831659 ± 251720.33 ± 9.78
[N II] 658540.98 ± 0.01301 ± 63127 ± 25134.87 ± 2.34
[S II] 671840.41 ± 0.04301 ± 63127 ± 2536.93 ± 2.28
[S II] 673240.41 ± 0.04301 ± 63127 ± 2536.91 ± 2.15

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 SNR15.30
Hβ Broad SNR5.54
Hγ Broad SNR3.75
AGN frac0.12
Host frac0.88
log L5100,Host43.46
Fe II/Hβ0.15
Fe II/[O III]0.16

Quality flags

spurious_hab/hbb0.0/0
l51002
balmer0
balmer_snr0
hb_width0
balmer_width1

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