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IRAS F23590-7713

Observation

Spectrum ID491327996_sp1
Alt nameg0001461-765714
z0.0585
RA, Dec0.4420, -76.9540
MJD60254.46
SNR/Å B/R13.5/21.8
Obs Airmass1.43
SMSS ID491327996
Closest SMSSNone (< 15")
SMSS Mean r6"ap15.9 ± 0.2
2MASS Kext12.2 ± 0.1

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.050
Power law αν0.34 ± 0.14
log L5100,AGN43.26 ± 0.04
log HβBr/[O III]-0.32 ± 0.02
log ML5100/M8.01 ± 0.04
log M/M7.69 ± 0.02
log M/M7.97 ± 0.04
log M[O III]/M8.28 ± 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 Narrow40.31 ± 0.08385 ± 63210 ± 253.97 ± 0.44
Hγ Broad40.80 ± 0.083153 ± 6061120 ± 10913.14 ± 0.94
[O III] 436439.93 ± 0.16336 ± 63142 ± 251.67 ± 0.33
He II Narrow39.91 ± 0.14336 ± 63142 ± 251.91 ± 0.34
He II Broad39.99 ± 0.271405 ± 273597 ± 1151.98 ± 0.68
Hβ Narrow40.67 ± 0.03385 ± 63210 ± 2511.75 ± 0.49
Hβ Broad41.37 ± 0.025149 ± 1781870 ± 8858.82 ± 1.40
[O III] 500741.70 ± 0.01385 ± 63210 ± 25135.71 ± 0.61
He I Narrow39.48 ± 0.25336 ± 63142 ± 251.19 ± 0.39
He I Broad40.34 ± 0.122118 ± 434899 ± 1847.96 ± 1.02
[O I] 630040.57 ± 0.02336 ± 63142 ± 2517.30 ± 0.45
Hα Narrow41.13 ± 0.01336 ± 63142 ± 2569.02 ± 0.76
Hα Broad42.19 ± 0.013446 ± 712200 ± 44791.32 ± 3.59
[N II] 658541.15 ± 0.01336 ± 63142 ± 2572.29 ± 0.71
[S II] 671840.77 ± 0.01336 ± 63142 ± 2531.46 ± 0.55
[S II] 673240.73 ± 0.01336 ± 63142 ± 2529.33 ± 0.56

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 SNR21.49
Hβ Broad SNR4.01
Hγ Broad SNR2.16
AGN frac0.45
Host frac0.55
log L5100,Host43.34
Fe II/Hβ0.10
Fe II/[O III]0.05

Quality flags

spurious_hab/hbb0.0/0
l51001
balmer0
balmer_snr1
hb_width0
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.