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5590460656614152576

Observation

Spectrum ID30817595_sp1
Alt name5590460656614152576
z0.0305
RA, Dec107.3835, -35.6296
MJD60672.65
SNR/Å B/R13.3/20.1
Obs Airmass1.02
SMSS ID30817595
Closest SMSS7.97'', 2057597554
SMSS Mean r6"ap16.2 ± 0.1
2MASS Kext11.9 ± 0.1

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN referenceAllBRICQS2
MW E(B−V)0.345
Power law αν0.46 ± 0.03
log L5100,AGN43.29 ± 0.01
log HβBr/[O III]0.24 ± 0.05
log ML5100/M7.72 ± 0.05
log M/M7.18 ± 0.03
log M/M7.72 ± 0.06
log M[O III]/M7.75 ± 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 Narrow39.64 ± 0.22203 ± 63113 ± 400.73 ± 0.27
Hγ Broad40.72 ± 0.131813 ± 527671 ± 2318.34 ± 0.72
[O III] 436439.79 ± 0.13192 ± 6380 ± 251.11 ± 0.18
He II Narrow39.49 ± 0.22192 ± 6380 ± 250.66 ± 0.18
He II Broad40.81 ± 0.182631 ± 10211117 ± 43413.44 ± 0.70
Hβ Narrow40.18 ± 0.05203 ± 63113 ± 403.34 ± 0.28
Hβ Broad41.48 ± 0.043642 ± 2061513 ± 22570.70 ± 1.00
[O III] 500741.23 ± 0.02203 ± 63113 ± 4042.93 ± 0.38
He I Narrow39.04 ± 0.25192 ± 6380 ± 250.41 ± 0.15
He I Broad40.09 ± 0.151560 ± 288663 ± 1224.77 ± 0.45
[O I] 630039.47 ± 0.11192 ± 6380 ± 251.29 ± 0.19
Hα Narrow40.51 ± 0.02192 ± 6380 ± 2515.60 ± 0.31
Hα Broad41.79 ± 0.012536 ± 951100 ± 75304.57 ± 1.10
[N II] 658540.43 ± 0.02192 ± 6380 ± 2513.12 ± 0.29
[S II] 671840.01 ± 0.04192 ± 6380 ± 255.21 ± 0.24
[S II] 673239.97 ± 0.04192 ± 6380 ± 254.86 ± 0.24

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 SNR19.25
Hβ Broad SNR9.01
Hγ Broad SNR3.67
AGN frac0.71
Host frac0.29
log L5100,Host42.90
Fe II/Hβ0.50
Fe II/[O III]0.89

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.