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2MASS J05053990-7912013

Observation

Spectrum ID490877201_sp1
Alt name4624111912867529344
z0.0827
RA, Dec76.4164, -79.2003
MJD59969.55
SNR/Å B/R14.0/20.8
Obs Airmass1.57
SMSS ID490877201
Closest SMSSNone (< 15")
SMSS Mean r6"ap16.4 ± 0.0
2MASS Kextnan ± nan

AGN Properties

Spectrum TypeSy 1.0
Quality Flaggood
AGN referenceAllBRICQS2
MW E(B−V)0.124
Power law αν-0.09 ± 0.11
log L5100,AGN43.75 ± 0.01
log HβBr/[O III]0.73 ± 0.01
log ML5100/M7.76 ± 0.02
log M/M7.39 ± 0.04
log M/M7.91 ± 0.02
log M[O III]/M7.73 ± 0.02

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 Narrow40.66 ± 0.09408 ± 63223 ± 262.99 ± 0.29
Hγ Broad41.61 ± 0.022850 ± 2391070 ± 4627.16 ± 0.74
[O III] 436440.37 ± 0.12364 ± 63154 ± 251.56 ± 0.25
He II Narrow40.35 ± 0.10364 ± 63154 ± 251.73 ± 0.24
He II Broad41.46 ± 0.045683 ± 3802413 ± 16121.94 ± 1.00
Hβ Narrow41.12 ± 0.03408 ± 63223 ± 2610.71 ± 0.32
Hβ Broad42.27 ± 0.013010 ± 702648 ± 88152.01 ± 1.80
[O III] 500741.53 ± 0.01408 ± 63223 ± 2629.66 ± 0.37
He I Narrow40.20 ± 0.09364 ± 63154 ± 251.86 ± 0.23
He I Broad41.27 ± 0.023529 ± 1731498 ± 7322.31 ± 0.68
[O I] 630039.51 ± 0.27364 ± 63154 ± 250.43 ± 0.24
Hα Narrow41.39 ± 0.02364 ± 63154 ± 2536.06 ± 0.37
Hα Broad42.60 ± 0.011808 ± 65969 ± 25580.18 ± 1.01
[N II] 658540.62 ± 0.04364 ± 63154 ± 256.18 ± 0.32
[S II] 671840.27 ± 0.08364 ± 63154 ± 252.84 ± 0.40
[S II] 673240.28 ± 0.07364 ± 63154 ± 252.92 ± 0.41

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 SNR60.08
Hβ Broad SNR18.53
Hγ Broad SNR7.61
AGN frac0.82
Host frac0.18
log L5100,Host43.09
Fe II/Hβ0.43
Fe II/[O III]2.32

Quality flags

spurious_hab/hbb0.0/0
l51000
balmer0
balmer_snr0
hb_width2
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.