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CTS 89

Observation

Spectrum ID90985522_sp1
Alt nameg1014116-124043
z0.0680
RA, Dec153.5483, -12.6787
MJD59672.52
SNR/Å B/R4.4/7.2
Obs Airmass1.08
SMSS ID90985522
Closest SMSS10.39'', 90985524
SMSS Mean r6"ap16.4 ± 0.0
2MASS Kext12.3 ± 0.1

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.060
Power law αν-0.29 ± 0.46
log L5100,AGN43.26 ± 0.05
log HβBr/[O III]-0.35 ± 0.04
log ML5100/M7.56 ± 0.07
log M/M7.81 ± 0.07
log M/M7.71 ± 0.07
log M[O III]/M8.04 ± 0.06

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 Narrow40.50 ± 0.14444 ± 65236 ± 277.02 ± 1.02
Hγ Broad41.12 ± 0.201353 ± 600484 ± 19726.44 ± 1.47
[O III] 436440.65 ± 0.18402 ± 66170 ± 279.58 ± 0.80
He II Narrow40.40 ± 0.14402 ± 66170 ± 276.33 ± 0.79
He II Broad40.64 ± 0.161191 ± 69505 ± 2810.26 ± 1.33
Hβ Narrow41.03 ± 0.04444 ± 65236 ± 2729.38 ± 1.13
Hβ Broad41.77 ± 0.043091 ± 2181119 ± 150143.67 ± 2.32
[O III] 500742.12 ± 0.01444 ± 65236 ± 27372.46 ± 1.36
He I Narrow39.86 ± 0.26402 ± 66170 ± 272.70 ± 0.79
He I Broad40.20 ± 0.231182 ± 68502 ± 285.65 ± 1.47
[O I] 630040.09 ± 0.11402 ± 66170 ± 275.20 ± 0.71
Hα Narrow41.49 ± 0.05402 ± 66170 ± 27134.05 ± 1.20
Hα Broad42.46 ± 0.013245 ± 2361212 ± 421238.74 ± 2.95
[N II] 658539.61 ± 0.41402 ± 66170 ± 271.83 ± 1.01
[S II] 671840.64 ± 0.04402 ± 66170 ± 2720.34 ± 0.98
[S II] 673240.52 ± 0.05402 ± 66170 ± 2715.57 ± 1.04

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 SNR29.41
Hβ Broad SNR8.41
Hγ Broad SNR4.42
AGN frac0.79
Host frac0.21
log L5100,Host42.68
Fe II/Hβ0.31
Fe II/[O III]0.13

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer0
balmer_snr0
hb_width0
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.