← atlas

6dFGS gJ182452.5-432858

Observation

Spectrum ID203556779_sp1
Alt nameg1824525-432858
z0.0718
RA, Dec276.2189, -43.4828
MJD59019.57
SNR/Å B/R23.3/35.5
Obs Airmass1.04
SMSS ID203556779
Closest SMSS3.99'', 203556778
SMSS Mean r6"ap16.2 ± 0.1
2MASS Kext12.6 ± 0.1

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.069
Power law αν-0.23 ± 0.07
log L5100,AGN43.89 ± 0.01
log HβBr/[O III]0.61 ± 0.02
log ML5100/M8.08 ± 0.03
log M/M7.80 ± 0.03
log M/M8.05 ± 0.03
log M[O III]/M7.93 ± 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 Narrow40.41 ± 0.12355 ± 63377 ± 301.26 ± 0.27
Hγ Broad41.49 ± 0.023711 ± 1341158 ± 4015.09 ± 0.40
[O III] 436439.67 ± 0.34329 ± 63139 ± 250.23 ± 0.13
He II Narrow39.98 ± 0.18329 ± 63139 ± 250.53 ± 0.14
He II Broad41.57 ± 0.037943 ± 2493373 ± 10520.68 ± 0.70
Hβ Narrow40.74 ± 0.05355 ± 63377 ± 303.31 ± 0.30
Hβ Broad42.00 ± 0.014093 ± 1261644 ± 4059.53 ± 0.62
[O III] 500741.39 ± 0.01355 ± 63378 ± 3015.55 ± 0.34
He I Narrow39.99 ± 0.11329 ± 63139 ± 250.82 ± 0.15
He I Broad41.37 ± 0.025529 ± 1502348 ± 6319.74 ± 0.53
[O I] 630040.24 ± 0.05329 ± 63139 ± 251.67 ± 0.14
Hα Narrow41.14 ± 0.01329 ± 63139 ± 2514.11 ± 0.21
Hα Broad42.51 ± 0.013113 ± 641436 ± 25328.95 ± 0.86
[N II] 658540.88 ± 0.02329 ± 63139 ± 257.71 ± 0.20
[S II] 671840.67 ± 0.02329 ± 63139 ± 255.02 ± 0.19
[S II] 673240.53 ± 0.03329 ± 63139 ± 253.64 ± 0.18

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 SNR36.67
Hβ Broad SNR12.68
Hγ Broad SNR5.47
AGN frac0.71
Host frac0.29
log L5100,Host43.51
Fe II/Hβ0.16
Fe II/[O III]0.65

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer0
balmer_snr0
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.