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2MASS J21304994-0208145

Observation

Spectrum ID4948374_sp1
Alt nameg2130499-020814
z0.0526
RA, Dec322.7081, -2.1374
MJD60088.79
SNR/Å B/R12.4/19.1
Obs Airmass1.15
SMSS ID4948374
Closest SMSSNone (< 15")
SMSS Mean r6"ap16.5 ± 0.0
2MASS Kext13.2 ± 0.1

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.053
Power law αν-1.22 ± 0.12
log L5100,AGN43.29 ± 0.02
log HβBr/[O III]-0.18 ± 0.02
log ML5100/M7.06 ± 0.08
log M/M6.48 ± 0.05
log M/M6.85 ± 0.08
log M[O III]/M7.07 ± 0.08

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 Narrow40.10 ± 0.07247 ± 62105 ± 252.94 ± 0.29
Hγ Broad40.37 ± 0.121991 ± 598856 ± 775.26 ± 0.78
[O III] 436439.79 ± 0.12246 ± 62104 ± 251.43 ± 0.23
He II Narrow39.39 ± 0.26246 ± 62104 ± 250.60 ± 0.21
He II Broad39.48 ± 0.391179 ± 62500 ± 250.75 ± 0.45
Hβ Narrow40.33 ± 0.04247 ± 62105 ± 255.40 ± 0.27
Hβ Broad41.02 ± 0.021711 ± 142867 ± 4026.18 ± 0.77
[O III] 500741.19 ± 0.01247 ± 62105 ± 2540.50 ± 0.31
He I Narrow38.95 ± 0.40246 ± 62104 ± 250.26 ± 0.16
He I Broad39.82 ± 0.161179 ± 62500 ± 251.92 ± 0.36
[O I] 630039.78 ± 0.06246 ± 62104 ± 251.89 ± 0.18
Hα Narrow41.11 ± 0.01246 ± 62104 ± 2540.96 ± 0.28
Hα Broad41.55 ± 0.011336 ± 64598 ± 25113.10 ± 0.76
[N II] 658540.44 ± 0.02246 ± 62104 ± 258.89 ± 0.23
[S II] 671840.20 ± 0.03246 ± 62104 ± 255.19 ± 0.19
[S II] 673240.10 ± 0.03246 ± 62104 ± 254.11 ± 0.19

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 SNR21.64
Hβ Broad SNR6.38
Hγ Broad SNR1.59
AGN frac0.75
Host frac0.25
log L5100,Host42.80
Fe II/Hβ0.91
Fe II/[O III]0.60

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.