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NVSS J192006-273441

Observation

Spectrum ID231377863_sp1
Alt nameg1920063-273434
z0.0634
RA, Dec290.0264, -27.5762
MJD60914.47
SNR/Å B/R11.2/17.0
Obs Airmass1.00
SMSS ID231377863
Closest SMSS9.62'', 231377870
SMSS Mean r6"ap16.1 ± 0.1
2MASS Kext12.0 ± 0.1

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.115
Power law αν0.18 ± 0.09
log L5100,AGN43.57 ± 0.01
log HβBr/[O III]0.34 ± 0.01
log ML5100/M7.45 ± 0.02
log M/M7.35 ± 0.03
log M/M7.55 ± 0.02
log M[O III]/M7.55 ± 0.02

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 Narrow40.34 ± 0.13297 ± 63257 ± 272.11 ± 0.42
Hγ Broad41.40 ± 0.032689 ± 2511074 ± 5424.28 ± 0.86
[O III] 436439.58 ± 0.35262 ± 63109 ± 250.37 ± 0.23
He II Narrow40.14 ± 0.10262 ± 63109 ± 251.56 ± 0.24
He II Broad41.20 ± 0.045269 ± 1292238 ± 5418.18 ± 1.12
Hβ Narrow40.61 ± 0.07297 ± 63257 ± 275.01 ± 0.46
Hβ Broad41.98 ± 0.012308 ± 571479 ± 51116.88 ± 1.46
[O III] 500741.64 ± 0.01297 ± 63257 ± 2757.06 ± 0.50
He I Narrow39.21 ± 0.38262 ± 63109 ± 250.30 ± 0.21
He I Broad40.89 ± 0.041983 ± 112842 ± 4714.18 ± 0.70
[O I] 630039.99 ± 0.08262 ± 63109 ± 252.10 ± 0.25
Hα Narrow41.05 ± 0.02262 ± 63109 ± 2526.68 ± 0.48
Hα Broad42.39 ± 0.012017 ± 64917 ± 25579.39 ± 1.46
[N II] 658540.78 ± 0.02262 ± 63109 ± 2514.49 ± 0.40
[S II] 671840.41 ± 0.03262 ± 63109 ± 256.47 ± 0.31
[S II] 673240.28 ± 0.04262 ± 63109 ± 254.77 ± 0.30

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 SNR44.69
Hβ Broad SNR17.33
Hγ Broad SNR5.85
AGN frac0.81
Host frac0.19
log L5100,Host42.94
Fe II/Hβ0.57
Fe II/[O III]1.24

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.