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2MASS J15080462-4244448

Observation

Spectrum ID310181797_sp3
Alt nameg1508046-424445
z0.0562
RA, Dec227.0190, -42.7458
MJD59726.6
SNR/Å B/R13.9/27.7
Obs Airmass1.07
SMSS ID310181797
Closest SMSS5.01'', 2460485054
SMSS Mean r6"ap16.4 ± 0.1
2MASS Kext12.5 ± 0.1

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.106
Power law αν-0.66 ± 0.17
log L5100,AGN43.32 ± 0.03
log HβBr/[O III]0.27 ± 0.01
log ML5100/M7.91 ± 0.05
log M/M7.55 ± 0.02
log M/M7.96 ± 0.05
log M[O III]/M7.99 ± 0.05

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 Narrow40.24 ± 0.11357 ± 63357 ± 273.41 ± 0.67
Hγ Broad41.14 ± 0.043822 ± 3851520 ± 5926.74 ± 1.25
[O III] 436439.83 ± 0.18334 ± 63141 ± 251.33 ± 0.33
He II Narrow39.76 ± 0.17334 ± 63141 ± 251.25 ± 0.32
He II Broad40.99 ± 0.0712538 ± 1335324 ± 5621.19 ± 1.97
Hβ Narrow40.51 ± 0.05357 ± 63357 ± 277.38 ± 0.67
Hβ Broad41.63 ± 0.014464 ± 2301958 ± 4097.46 ± 1.43
[O III] 500741.36 ± 0.01357 ± 63357 ± 2754.70 ± 0.70
He I Narrow38.99 ± 0.39334 ± 63141 ± 250.29 ± 0.20
He I Broad40.93 ± 0.024148 ± 851761 ± 3525.17 ± 0.78
[O I] 630039.76 ± 0.08334 ± 63141 ± 251.86 ± 0.22
Hα Narrow40.95 ± 0.01334 ± 63141 ± 2530.32 ± 0.34
Hα Broad42.02 ± 0.013304 ± 671525 ± 26355.67 ± 1.36
[N II] 658540.67 ± 0.02334 ± 63141 ± 2515.98 ± 0.31
[S II] 671840.27 ± 0.03334 ± 63141 ± 256.61 ± 0.26
[S II] 673240.18 ± 0.03334 ± 63141 ± 255.40 ± 0.26

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 SNR19.66
Hβ Broad SNR8.35
Hγ Broad SNR3.87
AGN frac0.54
Host frac0.46
log L5100,Host43.24
Fe II/Hβ0.39
Fe II/[O III]0.71

Quality flags

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