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2MASS J08200308-1741507

Observation

Spectrum ID70014132_sp1
Alt nameg0820031-174151
z0.0736
RA, Dec125.0129, -17.6975
MJD59668.48
SNR/Å B/R14.1/25.0
Obs Airmass1.10
SMSS ID70014132
Closest SMSS7.49'', 70014131
SMSS Mean r6"ap16.7 ± 0.0
2MASS Kext12.7 ± 0.2

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.111
Power law αν-0.71 ± 0.19
log L5100,AGN43.44 ± 0.03
log HβBr/[O III]0.25 ± 0.04
log ML5100/M7.16 ± 0.06
log M/M6.95 ± 0.03
log M/M7.00 ± 0.07
log M[O III]/M7.02 ± 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 Narrow40.27 ± 0.12364 ± 63289 ± 492.77 ± 0.62
Hγ Broad40.71 ± 0.112432 ± 426930 ± 897.25 ± 0.92
[O III] 436439.62 ± 0.32356 ± 63150 ± 250.63 ± 0.31
He II Narrow39.66 ± 0.28356 ± 63150 ± 250.75 ± 0.31
He II Broad41.08 ± 0.0813130 ± 1435576 ± 6019.79 ± 2.01
Hβ Narrow40.79 ± 0.04364 ± 63289 ± 4910.57 ± 0.64
Hβ Broad41.29 ± 0.031762 ± 1261276 ± 8833.82 ± 1.40
[O III] 500741.04 ± 0.02364 ± 63289 ± 4919.80 ± 0.70
He I Narrow39.72 ± 0.20356 ± 63150 ± 251.17 ± 0.29
He I Broad40.43 ± 0.081637 ± 107695 ± 455.81 ± 0.56
[O I] 630039.98 ± 0.07356 ± 63150 ± 252.33 ± 0.26
Hα Narrow41.40 ± 0.01356 ± 63150 ± 2564.43 ± 0.37
Hα Broad41.86 ± 0.011842 ± 651222 ± 52187.58 ± 2.18
[N II] 658541.10 ± 0.01356 ± 63150 ± 2532.17 ± 0.35
[S II] 671840.62 ± 0.02356 ± 63150 ± 2510.92 ± 0.35
[S II] 673240.49 ± 0.03356 ± 63150 ± 258.20 ± 0.39

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 SNR16.57
Hβ Broad SNR5.60
Hγ Broad SNR1.69
AGN frac0.53
Host frac0.47
log L5100,Host43.39
Fe II/Hβ0.60
Fe II/[O III]1.06

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer0
balmer_snr1
hb_width2
balmer_width1

Hα mass estimates from Cho+2023. Remaining mass estimates from R–L relations in Wang & Woo 2024 and zero-points from Amrutha+2026.