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NVSS J042938-210942

Observation

Spectrum ID22460749_sp1
Alt nameg0429383-210944
z0.0702
RA, Dec67.4096, -21.1621
MJD60939.77
SNR/Å B/R12.8/25.0
Obs Airmass1.02
SMSS ID22460749
Closest SMSS10.93'', 22460748
SMSS Mean r6"ap15.4 ± 0.2
2MASS Kext11.9 ± 0.1

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.021
Power law αν0.06 ± 0.25
log L5100,AGN43.35 ± 0.05
log HβBr/[O III]-0.14 ± 0.02
log ML5100/M8.66 ± 0.16
log M/M8.02 ± 0.04
log M/M8.80 ± 0.16
log M[O III]/M9.03 ± 0.16

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 Narrow40.58 ± 0.12575 ± 63376 ± 266.27 ± 0.93
Hγ Broad40.74 ± 0.201661 ± 6791678 ± 2188.44 ± 1.99
[O III] 436440.55 ± 0.08552 ± 63234 ± 255.93 ± 0.65
He II Narrow40.28 ± 0.20552 ± 63234 ± 253.67 ± 0.61
He II Broad40.30 ± 0.291179 ± 62500 ± 253.84 ± 0.88
Hβ Narrow41.03 ± 0.03575 ± 63376 ± 2622.24 ± 1.04
Hβ Broad41.85 ± 0.0210381 ± 18565220 ± 44150.86 ± 5.13
[O III] 500741.99 ± 0.01575 ± 63376 ± 26217.26 ± 1.35
He I Narrow40.06 ± 0.13552 ± 63234 ± 253.55 ± 0.69
He I Broad40.98 ± 0.1113217 ± 675613 ± 2729.23 ± 4.59
[O I] 630040.72 ± 0.03552 ± 63234 ± 2518.47 ± 0.70
Hα Narrow41.53 ± 0.01552 ± 63234 ± 25129.41 ± 1.07
Hα Broad42.32 ± 0.014545 ± 2212392 ± 25809.96 ± 3.51
[N II] 658541.45 ± 0.01552 ± 63234 ± 25110.45 ± 1.05
[S II] 671840.97 ± 0.02552 ± 63234 ± 2537.92 ± 1.01
[S II] 673240.95 ± 0.02552 ± 63234 ± 2535.99 ± 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 SNR14.74
Hβ Broad SNR3.35
Hγ Broad SNR1.06
AGN frac0.35
Host frac0.65
log L5100,Host43.62
Fe II/Hβ0.44
Fe II/[O III]0.32

Quality flags

spurious_hab/hbb0.0/0
l51001
balmer0
balmer_snr1
hb_width1
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.