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2MASS J07282338-4408241

Observation

Spectrum ID470026228_sp1
Alt nameg0728234-440824
z0.0816
RA, Dec112.0974, -44.1401
MJD60288.66
SNR/Å B/R9.1/13.6
Obs Airmass1.03
SMSS ID470026228
Closest SMSS13.42'', 470026227
SMSS Mean r6"ap17.3 ± 0.2
2MASS Kext12.8 ± 0.1

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.302
Power law αν-0.62 ± 0.23
log L5100,AGN43.68 ± 0.03
log HβBr/[O III]0.45 ± 0.02
log ML5100/M7.82 ± 0.04
log M/M8.00 ± 0.04
log M/M7.95 ± 0.03
log M[O III]/M7.90 ± 0.03

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 Narrow40.12 ± 0.31380 ± 63184 ± 261.10 ± 0.48
Hγ Broad41.58 ± 0.042517 ± 6361428 ± 8432.68 ± 1.62
[O III] 436440.72 ± 0.08366 ± 63155 ± 254.52 ± 0.46
He II Narrow40.28 ± 0.16366 ± 63155 ± 251.78 ± 0.41
He II Broad40.76 ± 0.234275 ± 6271815 ± 2664.93 ± 1.37
Hβ Narrow40.75 ± 0.07380 ± 63184 ± 265.53 ± 0.53
Hβ Broad42.14 ± 0.013355 ± 1261753 ± 74137.91 ± 2.07
[O III] 500741.69 ± 0.01380 ± 63184 ± 2650.26 ± 0.53
He I Narrow39.89 ± 0.26366 ± 63155 ± 250.99 ± 0.52
He I Broad41.42 ± 0.045099 ± 2162165 ± 9134.23 ± 1.71
[O I] 630040.51 ± 0.06366 ± 63155 ± 254.57 ± 0.45
Hα Narrow41.35 ± 0.02366 ± 63155 ± 2533.69 ± 0.70
Hα Broad42.79 ± 0.013197 ± 641406 ± 29927.04 ± 2.85
[N II] 658541.04 ± 0.03366 ± 63155 ± 2516.65 ± 0.66
[S II] 671840.67 ± 0.05366 ± 63155 ± 257.20 ± 0.69
[S II] 673240.67 ± 0.06366 ± 63155 ± 257.19 ± 0.72

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 SNR37.59
Hβ Broad SNR9.92
Hγ Broad SNR4.03
AGN frac0.68
Host frac0.32
log L5100,Host43.36
Fe II/Hβ0.33
Fe II/[O III]0.95

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer0
balmer_snr0
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.