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2MASS J11494680-4627515

Observation

Spectrum ID409469820_sp1
Alt name5377665986541771776
z0.0949
RA, Dec177.4450, -46.4643
MJD60800.39
SNR/Å B/R13.5/17.5
Obs Airmass1.09
SMSS ID409469820
Closest SMSS5.82'', 409469821
SMSS Mean r6"ap16.7 ± 0.1
2MASS Kext13.0 ± 0.1

AGN Properties

Spectrum TypeSy 1.0
Quality Flaggood
AGN referenceAllBRICQS2
MW E(B−V)0.082
Power law αν0.38 ± 0.09
log L5100,AGN43.90 ± 0.01
log HβBr/[O III]0.77 ± 0.03
log ML5100/M7.73 ± 0.03
log M/M7.54 ± 0.03
log M/M7.77 ± 0.03
log M[O III]/M7.57 ± 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 Narrow40.80 ± 0.12366 ± 63397 ± 372.83 ± 0.47
Hγ Broad41.75 ± 0.033305 ± 7511563 ± 5724.74 ± 0.88
[O III] 436440.37 ± 0.17337 ± 63142 ± 251.06 ± 0.24
He II Narrow40.23 ± 0.17337 ± 63142 ± 250.91 ± 0.25
He II Broad41.97 ± 0.0317660 ± 627499 ± 2549.69 ± 1.95
Hβ Narrow41.10 ± 0.06366 ± 63397 ± 377.26 ± 0.56
Hβ Broad42.15 ± 0.012717 ± 831514 ± 4182.53 ± 1.25
[O III] 500741.38 ± 0.03366 ± 63397 ± 3714.87 ± 0.62
He I Narrow40.05 ± 0.17337 ± 63142 ± 251.02 ± 0.22
He I Broad41.48 ± 0.023360 ± 821427 ± 3427.12 ± 0.82
[O I] 630039.58 ± 0.36337 ± 63142 ± 250.41 ± 0.27
Hα Narrow41.57 ± 0.01337 ± 63142 ± 2543.99 ± 0.48
Hα Broad42.54 ± 0.012240 ± 651091 ± 25410.35 ± 1.48
[N II] 658541.03 ± 0.03337 ± 63142 ± 2512.67 ± 0.41
[S II] 671840.76 ± 0.03337 ± 63142 ± 257.25 ± 0.40
[S II] 673240.55 ± 0.07337 ± 63142 ± 254.41 ± 0.39

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 SNR30.00
Hβ Broad SNR12.73
Hγ Broad SNR5.35
AGN frac0.81
Host frac0.19
log L5100,Host43.26
Fe II/Hβ0.50
Fe II/[O III]2.96

Quality flags

spurious_hab/hbb0.0/0
l51002
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.