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6296194358245802752

Observation

Spectrum ID108485631_sp1
Alt name6296194358245802752
z0.0828
RA, Dec214.3295, -18.5001
MJD60798.44
SNR/Å B/R6.2/9.1
Obs Airmass1.39
SMSS ID108485631
Closest SMSSNone (< 15")
SMSS Mean r6"ap16.6 ± 0.0
2MASS Kextnan ± nan

AGN Properties

Spectrum TypeSy 1.0
Quality Flaggood
AGN referenceAllBRICQS2
MW E(B−V)0.080
Power law αν0.13 ± 0.19
log L5100,AGN43.73 ± 0.02
log HβBr/[O III]0.85 ± 0.19
log ML5100/M7.20 ± 0.11
log M/M7.05 ± 0.05
log M/M7.18 ± 0.12
log M[O III]/M6.92 ± 0.15

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 Narrow40.62 ± 0.45385 ± 180216 ± 1234.16 ± 0.74
Hγ Broad41.43 ± 0.101558 ± 508619 ± 19314.54 ± 1.19
[O III] 436440.12 ± 0.31257 ± 78108 ± 321.02 ± 0.43
He II Narrow40.04 ± 0.31257 ± 78108 ± 320.96 ± 0.44
He II Broad40.54 ± 0.281356 ± 83576 ± 342.77 ± 1.00
Hβ Narrow41.01 ± 0.38385 ± 180216 ± 12312.57 ± 0.76
Hβ Broad41.84 ± 0.051613 ± 214585 ± 11448.64 ± 1.25
[O III] 500740.99 ± 0.18385 ± 180216 ± 12310.22 ± 0.83
He I Narrow39.95 ± 0.32257 ± 78108 ± 321.29 ± 0.52
He I Broad40.73 ± 0.191369 ± 187581 ± 796.88 ± 0.99
[O I] 630040.17 ± 0.16257 ± 78108 ± 322.42 ± 0.51
Hα Narrow41.41 ± 0.06257 ± 78108 ± 3243.52 ± 0.91
Hα Broad42.42 ± 0.011388 ± 79550 ± 63407.97 ± 1.76
[N II] 658540.92 ± 0.09257 ± 78108 ± 3214.36 ± 0.63
[S II] 671840.57 ± 0.12257 ± 78108 ± 327.03 ± 0.77
[S II] 673240.35 ± 0.11257 ± 78108 ± 324.26 ± 0.65

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 SNR28.61
Hβ Broad SNR9.31
Hγ Broad SNR4.15
AGN frac0.83
Host frac0.17
log L5100,Host43.05
Fe II/Hβ2.04
Fe II/[O III]10.32

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.