← atlas

6dFGS gJ100610.7-394101

Observation

Spectrum ID79545617_sp1
Alt nameg1006107-394101
z0.0291
RA, Dec151.5445, -39.6837
MJD59352.37
SNR/Å B/R15.7/35.3
Obs Airmass1.02
SMSS ID79545617
Closest SMSS7.77'', 2132683970
SMSS Mean r6"ap15.8 ± 0.0
2MASS Kext11.7 ± 0.1

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.126
Power law αν-0.82 ± 0.16
log L5100,AGN42.98 ± 0.02
log HβBr/[O III]0.45 ± 0.02
log ML5100/M7.29 ± 0.03
log M/M6.91 ± 0.03
log M/M7.34 ± 0.04
log M[O III]/M7.26 ± 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 Narrow39.49 ± 0.26401 ± 64244 ± 261.38 ± 0.46
Hγ Broad40.68 ± 0.042624 ± 163979 ± 3520.85 ± 0.98
[O III] 436439.58 ± 0.12270 ± 63114 ± 251.68 ± 0.29
He II Narrow39.56 ± 0.10270 ± 63114 ± 251.75 ± 0.25
He II Broad40.62 ± 0.0611014 ± 774677 ± 3120.30 ± 1.65
Hβ Narrow40.00 ± 0.07401 ± 64245 ± 265.14 ± 0.39
Hβ Broad41.28 ± 0.012591 ± 552320 ± 5998.57 ± 1.76
[O III] 500740.83 ± 0.01401 ± 64245 ± 2635.54 ± 0.42
He I Narrow38.73 ± 0.30270 ± 63114 ± 250.34 ± 0.15
He I Broad40.39 ± 0.033017 ± 751281 ± 3115.46 ± 0.55
[O I] 630038.58 ± 0.36270 ± 63114 ± 250.26 ± 0.17
Hα Narrow40.21 ± 0.02270 ± 63114 ± 2511.68 ± 0.23
Hα Broad41.71 ± 0.011956 ± 63968 ± 25372.85 ± 0.84
[N II] 658540.02 ± 0.02270 ± 63114 ± 257.68 ± 0.21
[S II] 671839.76 ± 0.03270 ± 63114 ± 254.25 ± 0.21
[S II] 673239.70 ± 0.04270 ± 63114 ± 253.76 ± 0.20

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 SNR38.76
Hβ Broad SNR11.71
Hγ Broad SNR4.82
AGN frac0.54
Host frac0.46
log L5100,Host42.91
Fe II/Hβ0.23
Fe II/[O III]0.67

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer0
balmer_snr0
hb_width2
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.