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IRAS 19237-1831

Observation

Spectrum ID264081448_sp1
Alt nameUVQSJ192636.95-182553.0
z0.0786
RA, Dec291.6540, -18.4314
MJD60905.44
SNR/Å B/R12.0/13.6
Obs Airmass1.06
SMSS ID264081448
Closest SMSS12.47'', 264081449
SMSS Mean r6"ap14.4 ± 0.1
2MASS Kextnan ± nan

AGN Properties

Spectrum TypeSy 1.2
Quality Flaggood
AGN referenceUVQS
MW E(B−V)0.087
Power law αν0.47 ± 0.03
log L5100,AGN44.62 ± 0.01
log HβBr/[O III]0.60 ± 0.04
log ML5100/M8.30 ± 0.07
log M/M8.10 ± 0.07
log M/M8.40 ± 0.07
log M[O III]/M8.32 ± 0.07

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 Narrow41.24 ± 0.27494 ± 88397 ± 791.72 ± 0.45
Hγ Broad42.42 ± 0.042388 ± 413912 ± 6921.15 ± 0.71
[O III] 436441.23 ± 0.18409 ± 96173 ± 401.57 ± 0.26
He II Narrow40.93 ± 0.24409 ± 96173 ± 400.94 ± 0.27
He II Broad41.69 ± 0.123098 ± 4111315 ± 1744.95 ± 0.72
Hβ Narrow42.01 ± 0.10494 ± 88398 ± 7911.52 ± 0.59
Hβ Broad42.98 ± 0.023652 ± 2751483 ± 227106.56 ± 1.08
[O III] 500742.39 ± 0.04494 ± 88398 ± 7928.79 ± 0.59
He I Narrow40.57 ± 0.33409 ± 96173 ± 400.74 ± 0.28
He I Broad41.85 ± 0.062566 ± 3651090 ± 15512.21 ± 0.74
[O I] 630040.64 ± 0.24409 ± 96173 ± 401.01 ± 0.31
Hα Narrow42.21 ± 0.08409 ± 96173 ± 4037.58 ± 0.81
Hα Broad43.48 ± 0.012214 ± 931213 ± 39687.31 ± 1.75
[N II] 658540.60 ± 0.41409 ± 96173 ± 401.05 ± 0.62
[S II] 671841.21 ± 0.11409 ± 96173 ± 404.22 ± 0.45
[S II] 673241.13 ± 0.11409 ± 96173 ± 403.44 ± 0.45

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 SNR45.28
Hβ Broad SNR13.93
Hγ Broad SNR6.69
AGN frac0.91
Host frac0.09
log L5100,Host43.62
Fe II/Hβ0.82
Fe II/[O III]3.28

Quality flags

spurious_hab/hbb0.0/0
l51002
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.