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NVSS J082749-142715

Observation

Spectrum ID72381622_sp1
Alt nameg0827501-142713
z0.0682
RA, Dec126.9589, -14.4535
MJD60018.45
SNR/Å B/R11.8/22.3
Obs Airmass1.05
SMSS ID72381622
Closest SMSS4.96'', 72381621
SMSS Mean r6"ap16.5 ± 0.1
2MASS Kext12.8 ± 0.2

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.043
Power law αν-0.33 ± 0.12
log L5100,AGN43.55 ± 0.02
log HβBr/[O III]0.26 ± 0.02
log ML5100/M7.25 ± 0.03
log M/M6.86 ± 0.04
log M/M7.24 ± 0.04
log M[O III]/M7.27 ± 0.03

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 Narrow40.43 ± 0.14401 ± 63257 ± 262.90 ± 0.40
Hγ Broad41.20 ± 0.041675 ± 200709 ± 6216.97 ± 0.75
[O III] 436439.58 ± 0.35296 ± 63126 ± 250.42 ± 0.24
He II Narrow40.09 ± 0.10296 ± 63126 ± 251.52 ± 0.24
He II Broad41.63 ± 0.0317659 ± 637499 ± 2553.11 ± 2.06
Hβ Narrow40.96 ± 0.03401 ± 63257 ± 2612.02 ± 0.41
Hβ Broad41.71 ± 0.021859 ± 681629 ± 6567.67 ± 1.47
[O III] 500741.45 ± 0.01401 ± 63257 ± 2638.52 ± 0.44
He I Narrow39.62 ± 0.15296 ± 63126 ± 250.74 ± 0.16
He I Broad40.98 ± 0.033380 ± 1181435 ± 4917.08 ± 0.59
[O I] 630040.06 ± 0.05296 ± 63126 ± 252.33 ± 0.18
Hα Narrow41.22 ± 0.01296 ± 63126 ± 2536.01 ± 0.27
Hα Broad42.09 ± 0.011404 ± 63656 ± 25268.19 ± 0.71
[N II] 658541.09 ± 0.01296 ± 63126 ± 2526.80 ± 0.25
[S II] 671840.74 ± 0.01296 ± 63126 ± 2512.35 ± 0.26
[S II] 673240.66 ± 0.02296 ± 63126 ± 2510.35 ± 0.28

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 SNR38.40
Hβ Broad SNR12.62
Hγ Broad SNR6.58
AGN frac0.81
Host frac0.19
log L5100,Host42.92
Fe II/Hβ0.44
Fe II/[O III]0.82

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer0
balmer_snr0
hb_width2
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.