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3XMM J011127.5-380500

Observation

Spectrum ID9264736_sp1
Alt nameNGC424
z0.0120
RA, Dec17.8646, -38.0835
MJD60650.59
SNR/Å B/R3.2/6.1
Obs Airmass1.53
SMSS ID9264736
Closest SMSS6.29'', 2015330919
SMSS Mean r6"ap14.7 ± 0.1
2MASS Kext9.1 ± 0.0

AGN Properties

Spectrum TypeSy 1.8
Quality Flaggood
AGN referenceS7
MW E(B−V)0.013
Power law αν-0.91 ± 0.47
log L5100,AGN42.09 ± 0.19
log HβBr/[O III]-0.65 ± 0.13
log ML5100/M6.38 ± 0.10
log M/M6.42 ± 0.06
log M/M6.48 ± 0.08
log M[O III]/M6.91 ± 0.06

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 Narrow39.76 ± 0.29368 ± 151248 ± 7622.25 ± 6.62
Hγ Broad40.25 ± 0.181201 ± 65422 ± 2556.16 ± 8.75
[O III] 436439.67 ± 0.24243 ± 125102 ± 5316.56 ± 3.96
He II Narrow39.55 ± 0.25243 ± 125102 ± 5314.16 ± 3.29
He II Broad40.06 ± 0.161247 ± 84529 ± 3543.43 ± 7.18
Hβ Narrow39.98 ± 0.24368 ± 151248 ± 7645.13 ± 6.02
Hβ Broad40.57 ± 0.101402 ± 71523 ± 34136.83 ± 8.23
[O III] 500741.22 ± 0.08368 ± 151248 ± 76677.89 ± 8.61
He I Narrow39.16 ± 0.30243 ± 125102 ± 537.17 ± 2.86
He I Broad39.50 ± 0.311238 ± 85525 ± 3515.24 ± 6.23
[O I] 630039.48 ± 0.22243 ± 125102 ± 5315.12 ± 2.80
Hα Narrow39.99 ± 0.29243 ± 125102 ± 5358.33 ± 5.24
Hα Broad41.32 ± 0.021465 ± 80542 ± 291107.79 ± 9.12
[N II] 658540.05 ± 0.19243 ± 125102 ± 5360.11 ± 4.26
[S II] 671839.91 ± 0.19243 ± 125102 ± 5342.48 ± 2.95
[S II] 673239.88 ± 0.20243 ± 125102 ± 5343.73 ± 2.92

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 SNR14.10
Hβ Broad SNR3.54
Hγ Broad SNR2.19
AGN frac0.20
Host frac0.80
log L5100,Host42.69
Fe II/Hβ1.13
Fe II/[O III]0.24

Quality flags

spurious_hab/hbb0.0/0
l51002
balmer0
balmer_snr1
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.