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2MASS J09172721-6456270

Observation

Spectrum ID457468024_sp1
Alt nameg0917272-645628
z0.0860
RA, Dec139.3634, -64.9408
MJD58111.61
SNR/Å B/R2.3/4.1
Obs Airmass1.32
SMSS ID457468024
Closest SMSS6.17'', 457468026
SMSS Mean r6"ap16.8 ± 0.2
2MASS Kext13.4 ± 0.2

AGN Properties

Spectrum TypeSy 1.8
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.180
Power law αν-0.50 ± 0.65
log L5100,AGN44.09 ± 0.08
log HβBr/[O III]-0.66 ± 0.07
log ML5100/M7.84 ± 0.22
log M/M8.37 ± 0.20
log M/M7.89 ± 0.22
log M[O III]/M8.40 ± 0.22

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 Narrow41.58 ± 0.24649 ± 94272 ± 3513.61 ± 2.26
Hγ Broad41.85 ± 0.191254 ± 114455 ± 4618.94 ± 3.10
[O III] 436441.46 ± 0.21380 ± 113160 ± 478.67 ± 1.67
He II Narrow41.21 ± 0.31380 ± 113160 ± 475.27 ± 1.62
He II Broad41.55 ± 0.231282 ± 93544 ± 3812.57 ± 2.98
Hβ Narrow41.92 ± 0.08649 ± 94272 ± 3535.16 ± 2.33
Hβ Broad42.35 ± 0.062819 ± 7211266 ± 8581.88 ± 5.48
[O III] 500743.02 ± 0.01649 ± 94272 ± 35444.11 ± 3.08
He I Narrow40.87 ± 0.33380 ± 113160 ± 473.48 ± 1.06
He I Broad41.04 ± 0.371194 ± 71507 ± 295.49 ± 1.97
[O I] 630041.45 ± 0.09380 ± 113160 ± 4714.50 ± 1.31
Hα Narrow42.28 ± 0.12380 ± 113160 ± 47113.77 ± 1.77
Hα Broad43.11 ± 0.033906 ± 9632026 ± 59777.91 ± 6.46
[N II] 658541.55 ± 0.15380 ± 113160 ± 4720.33 ± 1.64
[S II] 671841.84 ± 0.06380 ± 113160 ± 4739.61 ± 1.86
[S II] 673241.72 ± 0.07380 ± 113160 ± 4730.31 ± 1.82

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 SNR7.29
Hβ Broad SNR2.53
Hγ Broad SNR2.06
AGN frac0.79
Host frac0.20
log L5100,Host43.49
Fe II/Hβ0.46
Fe II/[O III]0.09

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer1
balmer_snr1
hb_width0
balmer_width2

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