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2MASS J09114771-1151397

Observation

Spectrum ID88193721_sp1
Alt nameg0911477-115140
z0.0707
RA, Dec137.9488, -11.8610
MJD59668.52
SNR/Å B/R15.4/29.1
Obs Airmass1.16
SMSS ID88193721
Closest SMSSNone (< 15")
SMSS Mean r6"ap16.4 ± 0.1
2MASS Kext12.7 ± 0.1

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.040
Power law αν-1.07 ± 0.18
log L5100,AGN43.33 ± 0.03
log HβBr/[O III]0.17 ± 0.02
log ML5100/M7.20 ± 0.04
log M/M7.14 ± 0.03
log M/M7.23 ± 0.04
log M[O III]/M7.30 ± 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 Narrow39.99 ± 0.16322 ± 63291 ± 291.99 ± 0.69
Hγ Broad41.12 ± 0.032881 ± 149924 ± 3426.91 ± 0.98
[O III] 436439.72 ± 0.23316 ± 63132 ± 251.07 ± 0.34
He II Narrow40.01 ± 0.10316 ± 63132 ± 252.27 ± 0.35
He II Broad41.32 ± 0.0310228 ± 2174344 ± 9246.13 ± 2.06
Hβ Narrow40.40 ± 0.07322 ± 63291 ± 295.78 ± 0.94
Hβ Broad41.60 ± 0.011949 ± 711387 ± 4590.52 ± 1.70
[O III] 500741.42 ± 0.01322 ± 63291 ± 2962.09 ± 0.76
He I Narrow39.00 ± 0.40316 ± 63132 ± 250.27 ± 0.24
He I Broad40.58 ± 0.041676 ± 125711 ± 5210.19 ± 0.53
[O I] 630039.72 ± 0.09316 ± 63132 ± 251.51 ± 0.22
Hα Narrow40.98 ± 0.01316 ± 63132 ± 2528.69 ± 0.31
Hα Broad42.06 ± 0.011994 ± 64864 ± 25343.77 ± 1.07
[N II] 658540.62 ± 0.02316 ± 63132 ± 2512.66 ± 0.29
[S II] 671840.37 ± 0.03316 ± 63132 ± 257.22 ± 0.32
[S II] 673240.21 ± 0.04316 ± 63132 ± 254.96 ± 0.29

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 SNR34.45
Hβ Broad SNR12.80
Hγ Broad SNR4.86
AGN frac0.47
Host frac0.53
log L5100,Host43.39
Fe II/Hβ0.38
Fe II/[O III]0.56

Quality flags

spurious_hab/hbb0.0/0
l51001
balmer0
balmer_snr0
hb_width2
balmer_width1

Hα mass estimates from Cho+2023. Remaining mass estimates from R–L relations in Wang & Woo 2024 and zero-points from Amrutha+2026.