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LEDA 622139

Observation

Spectrum ID488201165_sp1
Alt nameg2112449-373012
z0.0430
RA, Dec318.1870, -37.5033
MJD60085.8
SNR/Å B/R17.4/25.2
Obs Airmass1.01
SMSS ID488201165
Closest SMSSNone (< 15")
SMSS Mean r6"ap15.9 ± 0.1
2MASS Kext12.4 ± 0.1

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.036
Power law αν-0.35 ± 0.14
log L5100,AGN43.34 ± 0.02
log HβBr/[O III]0.59 ± 0.02
log ML5100/M7.41 ± 0.03
log M/M6.89 ± 0.04
log M/M7.37 ± 0.04
log M[O III]/M7.23 ± 0.04

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 Narrow40.06 ± 0.09390 ± 63168 ± 252.05 ± 0.24
Hγ Broad40.95 ± 0.032482 ± 121917 ± 4316.15 ± 0.57
[O III] 436439.63 ± 0.20388 ± 63165 ± 250.78 ± 0.19
He II Narrow39.60 ± 0.17388 ± 63165 ± 250.80 ± 0.19
He II Broad41.15 ± 0.0310654 ± 1684524 ± 7129.04 ± 1.04
Hβ Narrow40.54 ± 0.03390 ± 63168 ± 257.32 ± 0.26
Hβ Broad41.45 ± 0.012467 ± 681425 ± 4761.63 ± 0.84
[O III] 500740.87 ± 0.01390 ± 63168 ± 2516.59 ± 0.29
He I Narrow39.80 ± 0.08388 ± 63165 ± 251.85 ± 0.19
He I Broad40.81 ± 0.034259 ± 1071809 ± 4419.09 ± 0.63
[O I] 630039.57 ± 0.11388 ± 63165 ± 251.24 ± 0.21
Hα Narrow41.14 ± 0.01388 ± 63165 ± 2549.06 ± 0.36
Hα Broad41.82 ± 0.011762 ± 71882 ± 25232.03 ± 0.77
[N II] 658540.87 ± 0.01388 ± 63165 ± 2526.27 ± 0.34
[S II] 671840.39 ± 0.02388 ± 63165 ± 258.93 ± 0.25
[S II] 673240.28 ± 0.02388 ± 63165 ± 256.97 ± 0.24

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 SNR33.87
Hβ Broad SNR13.03
Hγ Broad SNR5.87
AGN frac0.76
Host frac0.24
log L5100,Host42.84
Fe II/Hβ0.55
Fe II/[O III]2.14

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer0
balmer_snr0
hb_width1
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.