← atlas

2MASS J18243062-5112240

Observation

Spectrum ID475504634_sp1
Alt nameg1824306-511224
z0.0784
RA, Dec276.1275, -51.2067
MJD60082.64
SNR/Å B/R6.8/7.9
Obs Airmass1.10
SMSS ID475504634
Closest SMSS14.78'', 475504633
SMSS Mean r6"ap16.1 ± 0.1
2MASS Kext13.1 ± 0.1

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.063
Power law αν0.02 ± 0.22
log L5100,AGN43.98 ± 0.03
log HβBr/[O III]-0.02 ± 0.05
log ML5100/M7.27 ± 0.12
log M/M7.46 ± 0.05
log M/M7.19 ± 0.12
log M[O III]/M7.37 ± 0.12

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 Narrow40.63 ± 0.24363 ± 66151 ± 261.59 ± 0.44
Hγ Broad41.42 ± 0.091289 ± 138454 ± 528.92 ± 0.82
[O III] 436440.67 ± 0.19322 ± 84136 ± 352.06 ± 0.39
He II Narrow40.45 ± 0.27322 ± 84136 ± 351.49 ± 0.40
He II Broad41.01 ± 0.161222 ± 72519 ± 294.53 ± 0.78
Hβ Narrow40.87 ± 0.22363 ± 66151 ± 263.52 ± 0.51
Hβ Broad41.96 ± 0.041537 ± 219558 ± 8337.86 ± 1.00
[O III] 500741.99 ± 0.02363 ± 66151 ± 2649.79 ± 0.64
He I Narrow40.17 ± 0.33322 ± 84136 ± 351.26 ± 0.44
He I Broad41.07 ± 0.121455 ± 138617 ± 588.04 ± 1.03
[O I] 630040.45 ± 0.17322 ± 84136 ± 352.56 ± 0.46
Hα Narrow41.58 ± 0.09322 ± 84136 ± 3533.49 ± 0.90
Hα Broad42.52 ± 0.012074 ± 107754 ± 47287.71 ± 1.86
[N II] 658541.26 ± 0.09322 ± 84136 ± 3516.73 ± 0.81
[S II] 671841.10 ± 0.09322 ± 84136 ± 3512.50 ± 0.89
[S II] 673240.97 ± 0.11322 ± 84136 ± 359.18 ± 0.75

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 SNR16.54
Hβ Broad SNR7.88
Hγ Broad SNR2.96
AGN frac0.84
Host frac0.16
log L5100,Host43.25
Fe II/Hβ0.68
Fe II/[O III]0.55

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer0
balmer_snr1
hb_width0
balmer_width2

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