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2MASS J07103298-5357523

Observation

Spectrum ID471462345_sp1
Alt nameg0710330-535752
z0.0486
RA, Dec107.6374, -53.9646
MJD60287.66
SNR/Å B/R7.2/17.5
Obs Airmass1.08
SMSS ID471462345
Closest SMSS7.52'', 471462347
SMSS Mean r6"ap16.1 ± 0.1
2MASS Kext12.0 ± 0.1

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.112
Power law αν-1.19 ± 0.37
log L5100,AGN42.95 ± 0.04
log HβBr/[O III]0.29 ± 0.03
log ML5100/M7.34 ± 0.04
log M/M7.27 ± 0.02
log M/M7.41 ± 0.04
log M[O III]/M7.41 ± 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 Narrow39.72 ± 0.31567 ± 66297 ± 272.65 ± 1.03
Hγ Broad40.59 ± 0.092483 ± 202803 ± 3919.30 ± 1.92
[O III] 436439.40 ± 0.38432 ± 64183 ± 261.26 ± 0.75
He II Narrow39.50 ± 0.29432 ± 64183 ± 261.67 ± 0.67
He II Broad40.42 ± 0.124141 ± 1071758 ± 4514.13 ± 2.12
Hβ Narrow40.10 ± 0.12567 ± 66297 ± 276.88 ± 0.88
Hβ Broad41.32 ± 0.032765 ± 912192 ± 128115.20 ± 3.93
[O III] 500741.03 ± 0.01567 ± 66297 ± 2759.83 ± 0.91
He I Narrow39.06 ± 0.39432 ± 64183 ± 260.73 ± 0.54
He I Broad40.87 ± 0.035245 ± 1392227 ± 5847.61 ± 2.09
[O I] 630040.00 ± 0.06432 ± 64183 ± 266.70 ± 0.57
Hα Narrow40.79 ± 0.03432 ± 64183 ± 2643.24 ± 0.97
Hα Broad42.01 ± 0.012391 ± 651114 ± 25725.02 ± 2.49
[N II] 658540.57 ± 0.03432 ± 64183 ± 2626.07 ± 0.84
[S II] 671840.36 ± 0.03432 ± 64183 ± 2616.35 ± 0.65
[S II] 673240.28 ± 0.03432 ± 64183 ± 2613.76 ± 0.66

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 SNR31.19
Hβ Broad SNR5.93
Hγ Broad SNR2.07
AGN frac0.54
Host frac0.46
log L5100,Host42.88
Fe II/Hβ0.41
Fe II/[O III]0.80

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer0
balmer_snr1
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.