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2MASS J18065901-5002462

Observation

Spectrum ID2676348235_sp1
Alt name6706071161850699264
z0.0500
RA, Dec271.7447, -50.0474
MJD60830.6
SNR/Å B/R26.2/37.9
Obs Airmass1.08
SMSS ID2676348235
Closest SMSS5.09'', 2676348236
SMSS Mean r6"apnan ± nan
2MASS Kextnan ± nan

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN referenceAllBRICQS2
MW E(B−V)0.127
Power law αν-1.26 ± 0.02
log L5100,AGN43.88 ± 0.01
log HβBr/[O III]0.65 ± 0.01
log ML5100/M7.46 ± 0.03
log M/M7.18 ± 0.03
log M/M7.35 ± 0.03
log M[O III]/M7.19 ± 0.04

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 Narrow40.20 ± 0.11256 ± 63126 ± 280.93 ± 0.17
Hγ Broad41.37 ± 0.032212 ± 1751137 ± 8313.81 ± 0.54
[O III] 436439.78 ± 0.22250 ± 63105 ± 250.35 ± 0.12
He II Narrow39.72 ± 0.20250 ± 63105 ± 250.33 ± 0.10
He II Broad40.97 ± 0.053742 ± 1841589 ± 785.92 ± 0.41
Hβ Narrow40.26 ± 0.08256 ± 63126 ± 281.15 ± 0.15
Hβ Broad41.80 ± 0.012014 ± 641013 ± 3540.35 ± 0.42
[O III] 500741.14 ± 0.01256 ± 63126 ± 289.11 ± 0.15
He I Narrow39.53 ± 0.22250 ± 63105 ± 250.25 ± 0.08
He I Broad41.12 ± 0.023080 ± 1261308 ± 539.75 ± 0.29
[O I] 630039.43 ± 0.23250 ± 63105 ± 250.21 ± 0.08
Hα Narrow40.97 ± 0.02250 ± 63105 ± 257.42 ± 0.13
Hα Broad42.20 ± 0.011899 ± 66910 ± 25126.23 ± 0.40
[N II] 658540.63 ± 0.03250 ± 63105 ± 253.41 ± 0.11
[S II] 671840.23 ± 0.04250 ± 63105 ± 251.38 ± 0.09
[S II] 673240.19 ± 0.04250 ± 63105 ± 251.25 ± 0.09

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 SNR34.82
Hβ Broad SNR17.38
Hγ Broad SNR6.48
AGN frac0.78
Host frac0.22
log L5100,Host43.33
Fe II/Hβ1.15
Fe II/[O III]5.22

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.