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2MASS J00395667-1749404

Observation

Spectrum ID12051737_sp1
Alt nameg0039566-174940
z0.0874
RA, Dec9.9861, -17.8279
MJD60225.57
SNR/Å B/R12.6/20.6
Obs Airmass1.03
SMSS ID12051737
Closest SMSSNone (< 15")
SMSS Mean r6"ap17.2 ± 0.1
2MASS Kext13.5 ± 0.1

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.018
Power law αν-1.78 ± 0.10
log L5100,AGN43.48 ± 0.01
log HβBr/[O III]-0.29 ± 0.03
log ML5100/M7.02 ± 0.05
log M/M6.56 ± 0.04
log M/M6.82 ± 0.06
log M[O III]/M7.11 ± 0.05

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 Narrow40.49 ± 0.07402 ± 63253 ± 265.04 ± 0.42
Hγ Broad40.34 ± 0.161229 ± 70391 ± 253.09 ± 0.55
[O III] 436439.71 ± 0.22360 ± 63152 ± 250.84 ± 0.28
He II Narrow39.95 ± 0.13360 ± 63152 ± 251.47 ± 0.26
He II Broad41.18 ± 0.0617659 ± 637499 ± 2525.21 ± 2.05
Hβ Narrow40.76 ± 0.05402 ± 63253 ± 269.59 ± 0.42
Hβ Broad41.23 ± 0.031477 ± 75932 ± 5028.40 ± 0.94
[O III] 500741.52 ± 0.01402 ± 63253 ± 2655.96 ± 0.47
He I Narrow39.92 ± 0.16360 ± 63152 ± 251.45 ± 0.23
He I Broad40.17 ± 0.131180 ± 62501 ± 252.57 ± 0.37
[O I] 630040.25 ± 0.04360 ± 63152 ± 253.12 ± 0.20
Hα Narrow41.30 ± 0.01360 ± 63152 ± 2535.28 ± 0.24
Hα Broad41.73 ± 0.011292 ± 63552 ± 2595.92 ± 0.60
[N II] 658541.19 ± 0.01360 ± 63152 ± 2527.62 ± 0.26
[S II] 671840.68 ± 0.02360 ± 63152 ± 258.68 ± 0.25
[S II] 673240.60 ± 0.02360 ± 63152 ± 257.18 ± 0.25

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 SNR23.73
Hβ Broad SNR7.40
Hγ Broad SNR1.70
AGN frac0.81
Host frac0.19
log L5100,Host42.85
Fe II/Hβ1.75
Fe II/[O III]0.90

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer0
balmer_snr1
hb_width1
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.