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NVSS J161143-343530

Observation

Spectrum ID117747295_sp1
Alt nameg1611435-343529
z0.0612
RA, Dec242.9314, -34.5913
MJD60163.38
SNR/Å B/R8.0/12.1
Obs Airmass1.00
SMSS ID117747295
Closest SMSS1.77'', 2190727975
SMSS Mean r6"ap15.8 ± 0.1
2MASS Kext11.9 ± 0.1

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.271
Power law αν0.17 ± 0.18
log L5100,AGN43.79 ± 0.03
log HβBr/[O III]-0.10 ± 0.15
log ML5100/M8.17 ± 0.42
log M/M8.37 ± 0.07
log M/M8.24 ± 0.43
log M[O III]/M8.46 ± 0.42

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 Narrow40.87 ± 0.08342 ± 63166 ± 283.99 ± 0.39
Hγ Broad41.18 ± 0.152388 ± 737765 ± 1778.54 ± 0.83
[O III] 436440.48 ± 0.14328 ± 63138 ± 251.79 ± 0.33
He II Narrow40.36 ± 0.17328 ± 63138 ± 251.57 ± 0.35
He II Broad41.08 ± 0.133284 ± 4821395 ± 2058.55 ± 1.12
Hβ Narrow41.25 ± 0.06342 ± 63166 ± 2813.06 ± 0.46
Hβ Broad42.12 ± 0.154737 ± 18161773 ± 68897.08 ± 1.60
[O III] 500742.22 ± 0.01342 ± 63166 ± 28127.39 ± 0.61
He I Narrow40.30 ± 0.16328 ± 63138 ± 252.23 ± 0.36
He I Broad40.51 ± 0.272908 ± 15331235 ± 6513.69 ± 1.13
[O I] 630040.79 ± 0.04328 ± 63138 ± 258.01 ± 0.40
Hα Narrow41.85 ± 0.02328 ± 63138 ± 2598.99 ± 0.75
Hα Broad42.73 ± 0.015080 ± 3562326 ± 33768.51 ± 2.56
[N II] 658541.51 ± 0.03328 ± 63138 ± 2546.14 ± 0.71
[S II] 671841.20 ± 0.02328 ± 63138 ± 2523.71 ± 0.53
[S II] 673241.12 ± 0.03328 ± 63138 ± 2520.08 ± 0.53

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 SNR18.52
Hβ Broad SNR6.89
Hγ Broad SNR1.90
AGN frac0.81
Host frac0.19
log L5100,Host43.16
Fe II/Hβ0.43
Fe II/[O III]0.35

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer0
balmer_snr1
hb_width0
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.