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6037522256277200256

Observation

Spectrum ID141214827_sp1
Alt name6037522256277200256
z0.0878
RA, Dec244.5586, -30.9907
MJD59792.54
SNR/Å B/R7.9/8.9
Obs Airmass1.32
SMSS ID141214827
Closest SMSS9.77'', 141214828
SMSS Mean r6"ap16.6 ± 0.1
2MASS Kextnan ± nan

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN referenceAllBRICQS
MW E(B−V)0.281
Power law αν-0.73 ± 0.16
log L5100,AGN44.22 ± 0.02
log HβBr/[O III]0.24 ± 0.02
log ML5100/M7.71 ± 0.09
log M/M7.49 ± 0.05
log M/M7.72 ± 0.09
log M[O III]/M7.78 ± 0.09

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 Narrow40.97 ± 0.14316 ± 63235 ± 352.32 ± 0.70
Hγ Broad41.92 ± 0.052553 ± 268955 ± 3720.90 ± 1.10
[O III] 436440.80 ± 0.17307 ± 63129 ± 251.57 ± 0.36
He II Narrow40.12 ± 0.47307 ± 63129 ± 250.36 ± 0.33
He II Broad41.50 ± 0.071248 ± 72530 ± 298.52 ± 0.72
Hβ Narrow41.24 ± 0.08316 ± 63235 ± 354.98 ± 0.72
Hβ Broad42.39 ± 0.022262 ± 2251211 ± 3671.01 ± 1.37
[O III] 500742.15 ± 0.01316 ± 63235 ± 3542.44 ± 0.82
He I Narrow40.29 ± 0.33307 ± 63129 ± 250.72 ± 0.32
He I Broad41.02 ± 0.141181 ± 63501 ± 253.87 ± 0.65
[O I] 630040.73 ± 0.11307 ± 63129 ± 252.17 ± 0.39
Hα Narrow41.83 ± 0.02307 ± 63129 ± 2528.80 ± 0.47
Hα Broad42.91 ± 0.011645 ± 66944 ± 25343.15 ± 1.57
[N II] 658540.78 ± 0.13307 ± 63129 ± 252.55 ± 0.42
[S II] 671841.01 ± 0.07307 ± 63129 ± 254.46 ± 0.49
[S II] 673240.79 ± 0.10307 ± 63129 ± 252.72 ± 0.49

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 SNR27.51
Hβ Broad SNR8.61
Hγ Broad SNR3.56
AGN frac0.90
Host frac0.10
log L5100,Host43.26
Fe II/Hβ0.71
Fe II/[O III]1.23

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.