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NVSS J060105-261058

Observation

Spectrum ID48021736_sp1
Alt nameg0601057-261110
z0.0391
RA, Dec90.2737, -26.1860
MJD59673.45
SNR/Å B/R14.6/30.6
Obs Airmass1.47
SMSS ID48021736
Closest SMSS11.63'', 48021737
SMSS Mean r6"ap15.6 ± 0.1
2MASS Kext11.5 ± 0.1

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.028
Power law αν-0.15 ± 0.25
log L5100,AGN42.92 ± 0.04
log HβBr/[O III]0.18 ± 0.02
log ML5100/M8.11 ± 0.05
log M/M7.67 ± 0.02
log M/M8.18 ± 0.05
log M[O III]/M8.23 ± 0.05

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 Narrow39.54 ± 0.27324 ± 63191 ± 251.58 ± 0.63
Hγ Broad40.59 ± 0.083361 ± 3921349 ± 5217.40 ± 2.00
[O III] 436439.25 ± 0.32253 ± 63106 ± 250.82 ± 0.43
He II Narrow39.24 ± 0.31253 ± 63106 ± 250.91 ± 0.40
He II Broad39.62 ± 0.301180 ± 62500 ± 252.16 ± 0.88
Hβ Narrow40.12 ± 0.06324 ± 63191 ± 257.30 ± 0.64
Hβ Broad41.28 ± 0.026839 ± 3102649 ± 37105.35 ± 2.36
[O III] 500741.10 ± 0.01324 ± 63191 ± 2573.96 ± 0.68
He I Narrow38.95 ± 0.30253 ± 63106 ± 250.70 ± 0.31
He I Broad40.69 ± 0.046541 ± 1052778 ± 4438.17 ± 1.75
[O I] 630039.57 ± 0.08253 ± 63106 ± 253.37 ± 0.38
Hα Narrow40.47 ± 0.01253 ± 63106 ± 2528.57 ± 0.49
Hα Broad41.78 ± 0.014456 ± 701880 ± 36581.42 ± 2.63
[N II] 658540.53 ± 0.01253 ± 63106 ± 2533.02 ± 0.50
[S II] 671840.03 ± 0.03253 ± 63106 ± 2510.83 ± 0.44
[S II] 673239.87 ± 0.04253 ± 63106 ± 257.50 ± 0.44

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 SNR13.35
Hβ Broad SNR4.05
Hγ Broad SNR1.92
AGN frac0.32
Host frac0.68
log L5100,Host43.24
Fe II/Hβ0.60
Fe II/[O III]0.91

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.