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NGC 6814

Observation

Spectrum ID286051911_sp1
Alt nameg1942406-101925
z0.0055
RA, Dec295.6691, -10.3236
MJD60163.53
SNR/Å B/R18.2/28.8
Obs Airmass1.07
SMSS ID286051911
Closest SMSS5.52'', 2399565663
SMSS Mean r6"ap14.0 ± 0.1
2MASS Kext7.7 ± 0.0

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.159
Power law αν-0.51 ± 0.16
log L5100,AGN42.05 ± 0.02
log HβBr/[O III]0.23 ± 0.02
log ML5100/M7.19 ± 0.05
log M/M6.82 ± 0.05
log M/M7.23 ± 0.07
log M[O III]/M7.22 ± 0.07

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 Narrow38.39 ± 0.25289 ± 63142 ± 250.84 ± 0.26
Hγ Broad39.93 ± 0.102597 ± 694998 ± 24031.88 ± 0.79
[O III] 436438.54 ± 0.19249 ± 63105 ± 251.26 ± 0.23
He II Narrow38.15 ± 0.27249 ± 63105 ± 250.58 ± 0.19
He II Broad39.18 ± 0.242368 ± 10121005 ± 4306.27 ± 0.63
Hβ Narrow38.92 ± 0.07289 ± 63142 ± 253.40 ± 0.28
Hβ Broad40.38 ± 0.023667 ± 1411444 ± 102106.70 ± 0.94
[O III] 500740.15 ± 0.01289 ± 63142 ± 2563.32 ± 0.25
He I Narrow38.32 ± 0.21249 ± 63105 ± 251.18 ± 0.30
He I Broad39.67 ± 0.104433 ± 14151882 ± 60126.76 ± 1.39
[O I] 630038.70 ± 0.05249 ± 63105 ± 253.20 ± 0.22
Hα Narrow39.42 ± 0.03249 ± 63105 ± 2517.93 ± 0.38
Hα Broad40.86 ± 0.013199 ± 801195 ± 34481.67 ± 1.14
[N II] 658539.75 ± 0.02249 ± 63105 ± 2538.08 ± 0.38
[S II] 671839.18 ± 0.02249 ± 63105 ± 2510.46 ± 0.27
[S II] 673239.18 ± 0.02249 ± 63105 ± 2510.51 ± 0.27

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 SNR35.03
Hβ Broad SNR13.39
Hγ Broad SNR7.36
AGN frac0.50
Host frac0.50
log L5100,Host42.04
Fe II/Hβ0.57
Fe II/[O III]1.00

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer0
balmer_snr0
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.