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5778852799983279744

Observation

Spectrum ID408140206_sp1
Alt name5778852799983279744
z0.0718
RA, Dec244.7576, -78.5437
MJD59649.75
SNR/Å B/R18.5/26.5
Obs Airmass1.49
SMSS ID408140206
Closest SMSS5.94'', 408140208
SMSS Mean r6"ap14.7 ± 0.1
2MASS Kextnan ± nan

AGN Properties

Spectrum TypeSy 1.0
Quality Flaggood
AGN referenceAllBRICQS
MW E(B−V)0.146
Power law αν-0.63 ± 0.05
log L5100,AGN44.19 ± 0.01
log HβBr/[O III]0.88 ± 0.03
log ML5100/M8.13 ± 0.03
log M/M7.90 ± 0.04
log M/M8.13 ± 0.03
log M[O III]/M7.88 ± 0.04

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 Narrow40.38 ± 0.29287 ± 64405 ± 280.63 ± 0.30
Hγ Broad41.70 ± 0.043747 ± 3391475 ± 5112.98 ± 0.60
[O III] 436439.83 ± 0.40245 ± 63103 ± 250.18 ± 0.13
He II Narrow39.85 ± 0.35245 ± 63103 ± 250.21 ± 0.13
He II Broad41.48 ± 0.0810942 ± 1094646 ± 458.89 ± 0.91
Hβ Narrow40.46 ± 0.24287 ± 64405 ± 280.88 ± 0.29
Hβ Broad42.33 ± 0.013729 ± 1371838 ± 3966.60 ± 0.74
[O III] 500741.45 ± 0.02287 ± 64405 ± 289.11 ± 0.33
He I Narrow39.80 ± 0.30245 ± 63103 ± 250.25 ± 0.10
He I Broad40.80 ± 0.081797 ± 85763 ± 352.53 ± 0.26
[O I] 630039.70 ± 0.28245 ± 63103 ± 250.22 ± 0.10
Hα Narrow40.92 ± 0.03245 ± 63103 ± 253.87 ± 0.15
Hα Broad42.80 ± 0.012825 ± 641334 ± 25295.63 ± 0.66
[N II] 658540.14 ± 0.16245 ± 63103 ± 250.66 ± 0.13
[S II] 671840.15 ± 0.14245 ± 63103 ± 250.68 ± 0.15
[S II] 673240.15 ± 0.12245 ± 63103 ± 250.68 ± 0.12

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 SNR37.53
Hβ Broad SNR12.84
Hγ Broad SNR3.85
AGN frac0.90
Host frac0.10
log L5100,Host43.25
Fe II/Hβ0.95
Fe II/[O III]7.26

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.