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6714297501686651776

Observation

Spectrum ID211074404_sp1
Alt name6714297501686651776
z0.0588
RA, Dec288.3627, -40.5057
MJD60772.78
SNR/Å B/R13.5/23.3
Obs Airmass1.07
SMSS ID211074404
Closest SMSS13.52'', 1248731782
SMSS Mean r6"ap16.6 ± 0.1
2MASS Kext13.0 ± 0.1

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN referenceAllBRICQS2
MW E(B−V)0.090
Power law αν-0.80 ± 0.17
log L5100,AGN43.28 ± 0.03
log HβBr/[O III]-0.06 ± 0.02
log ML5100/M7.73 ± 0.08
log M/M7.38 ± 0.02
log M/M7.67 ± 0.09
log M[O III]/M7.84 ± 0.08

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 Narrow40.24 ± 0.11422 ± 63255 ± 273.83 ± 0.46
Hγ Broad40.76 ± 0.071837 ± 474932 ± 10512.69 ± 0.95
[O III] 436439.72 ± 0.22409 ± 63173 ± 251.16 ± 0.33
He II Narrow39.75 ± 0.16409 ± 63173 ± 251.38 ± 0.32
He II Broad41.13 ± 0.0617659 ± 637499 ± 2532.51 ± 2.44
Hβ Narrow40.75 ± 0.03422 ± 63255 ± 2714.08 ± 0.48
Hβ Broad41.34 ± 0.023693 ± 3391604 ± 5255.73 ± 1.51
[O III] 500741.40 ± 0.01422 ± 63255 ± 2765.72 ± 0.51
He I Narrow39.69 ± 0.13409 ± 63173 ± 251.56 ± 0.26
He I Broad40.60 ± 0.053308 ± 1811405 ± 7612.51 ± 0.86
[O I] 630040.21 ± 0.03409 ± 63173 ± 255.61 ± 0.28
Hα Narrow41.33 ± 0.01409 ± 63173 ± 2577.25 ± 0.44
Hα Broad41.81 ± 0.013113 ± 691444 ± 64235.72 ± 1.93
[N II] 658541.10 ± 0.01409 ± 63173 ± 2546.30 ± 0.41
[S II] 671840.66 ± 0.01409 ± 63173 ± 2516.93 ± 0.33
[S II] 673240.55 ± 0.02409 ± 63173 ± 2513.20 ± 0.34

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 SNR14.56
Hβ Broad SNR6.10
Hγ Broad SNR3.14
AGN frac0.59
Host frac0.41
log L5100,Host43.12
Fe II/Hβ0.53
Fe II/[O III]0.46

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.