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2666892872242400384

Observation

Spectrum ID5182159_sp1
Alt name2666892872242400384
z0.0591
RA, Dec328.4807, -7.1582
MJD60825.8
SNR/Å B/R10.2/18.9
Obs Airmass1.10
SMSS ID5182159
Closest SMSSNone (< 15")
SMSS Mean r6"ap16.5 ± 0.1
2MASS Kext12.9 ± 0.1

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN referenceAllBRICQS2
MW E(B−V)0.035
Power law αν0.29 ± 0.17
log L5100,AGN42.70 ± 0.05
log HβBr/[O III]-0.06 ± 0.02
log ML5100/M8.23 ± 0.04
log M/M7.84 ± 0.02
log M/M8.42 ± 0.04
log M[O III]/M8.60 ± 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 Narrow39.91 ± 0.12275 ± 62172 ± 265.70 ± 1.14
Hγ Broad40.67 ± 0.084102 ± 5411565 ± 4932.58 ± 2.96
[O III] 436439.99 ± 0.08264 ± 62111 ± 256.94 ± 0.69
He II Narrow39.73 ± 0.12264 ± 62111 ± 254.44 ± 0.73
He II Broad40.65 ± 0.064533 ± 901925 ± 3737.25 ± 3.03
Hβ Narrow40.35 ± 0.04275 ± 62173 ± 2620.27 ± 1.29
Hβ Broad41.34 ± 0.028743 ± 2673334 ± 34200.21 ± 4.63
[O III] 500741.41 ± 0.01275 ± 62173 ± 26248.94 ± 1.52
He I Narrow39.05 ± 0.32264 ± 62111 ± 251.58 ± 0.71
He I Broad39.72 ± 0.181351 ± 77573 ± 327.15 ± 1.62
[O I] 630039.93 ± 0.04264 ± 62111 ± 2513.90 ± 0.77
Hα Narrow40.89 ± 0.01264 ± 62111 ± 25138.87 ± 1.27
Hα Broad41.84 ± 0.015227 ± 972208 ± 261236.62 ± 5.43
[N II] 658540.56 ± 0.01264 ± 62111 ± 2565.76 ± 1.17
[S II] 671840.17 ± 0.02264 ± 62111 ± 2528.03 ± 0.96
[S II] 673240.14 ± 0.03264 ± 62111 ± 2526.62 ± 0.97

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 SNR12.43
Hβ Broad SNR3.53
Hγ Broad SNR1.82
AGN frac0.27
Host frac0.73
log L5100,Host43.14
Fe II/Hβ0.19
Fe II/[O III]0.16

Quality flags

spurious_hab/hbb0.0/0
l51001
balmer0
balmer_snr1
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.