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2MASS J15155929-3602337

Observation

Spectrum ID112952110_sp1
Alt name6199896346751788160
z0.0731
RA, Dec228.9971, -36.0427
MJD60843.53
SNR/Å B/R10.1/12.5
Obs Airmass1.03
SMSS ID112952110
Closest SMSSNone (< 15")
SMSS Mean r6"ap16.4 ± 0.1
2MASS Kextnan ± nan

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN referenceAllBRICQS2
MW E(B−V)0.129
Power law αν0.33 ± 0.09
log L5100,AGN43.68 ± 0.01
log HβBr/[O III]0.16 ± 0.02
log ML5100/M7.29 ± 0.05
log M/M6.92 ± 0.04
log M/M7.32 ± 0.05
log M[O III]/M7.41 ± 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 Narrow40.52 ± 0.11305 ± 63235 ± 302.42 ± 0.55
Hγ Broad41.25 ± 0.061399 ± 132821 ± 10213.00 ± 0.93
[O III] 436440.10 ± 0.19296 ± 63124 ± 250.94 ± 0.25
He II Narrow40.27 ± 0.09296 ± 63124 ± 251.61 ± 0.22
He II Broad41.10 ± 0.074695 ± 3661994 ± 15511.00 ± 1.09
Hβ Narrow40.84 ± 0.05305 ± 63235 ± 306.62 ± 0.57
Hβ Broad41.94 ± 0.011823 ± 921890 ± 5781.80 ± 1.57
[O III] 500741.77 ± 0.01305 ± 63235 ± 3059.94 ± 0.68
He I Narrow39.54 ± 0.32296 ± 63124 ± 250.51 ± 0.30
He I Broad41.09 ± 0.066903 ± 2502931 ± 10618.13 ± 1.21
[O I] 630039.81 ± 0.16296 ± 63124 ± 251.11 ± 0.27
Hα Narrow41.26 ± 0.01296 ± 63124 ± 2534.82 ± 0.46
Hα Broad42.15 ± 0.011447 ± 64688 ± 25270.18 ± 2.14
[N II] 658540.68 ± 0.03296 ± 63124 ± 259.10 ± 0.39
[S II] 671840.53 ± 0.04296 ± 63124 ± 256.79 ± 0.38
[S II] 673240.42 ± 0.04296 ± 63124 ± 255.32 ± 0.36

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 SNR26.01
Hβ Broad SNR11.80
Hγ Broad SNR4.62
AGN frac0.89
Host frac0.11
log L5100,Host42.78
Fe II/Hβ0.75
Fe II/[O III]1.10

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.