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2MASS J16161077-1014059

Observation

Spectrum ID192188594_sp3
Alt nameg1616108-101406
z0.0767
RA, Dec244.0449, -10.2350
MJD60414.57
SNR/Å B/R10.8/13.6
Obs Airmass1.49
SMSS ID192188594
Closest SMSS13.95'', 192188595
SMSS Mean r6"ap17.4 ± 0.1
2MASS Kext12.6 ± 0.1

AGN Properties

Spectrum TypeSy 1.5
Quality Flaggood
AGN reference6dFGS
MW E(B−V)0.234
Power law αν-0.07 ± 0.31
log L5100,AGN43.33 ± 0.05
log HβBr/[O III]0.29 ± 0.02
log ML5100/M7.48 ± 0.04
log M/M7.20 ± 0.03
log M/M7.61 ± 0.04
log M[O III]/M7.63 ± 0.03

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 ± 0.13320 ± 63281 ± 343.05 ± 0.97
Hγ Broad41.35 ± 0.033481 ± 2991273 ± 4939.25 ± 1.56
[O III] 436439.87 ± 0.23299 ± 63126 ± 251.33 ± 0.46
He II Narrow40.30 ± 0.08299 ± 63126 ± 254.06 ± 0.49
He II Broad41.39 ± 0.047592 ± 3363224 ± 14350.30 ± 2.70
Hβ Narrow40.55 ± 0.07320 ± 63281 ± 347.77 ± 0.98
Hβ Broad41.79 ± 0.012715 ± 1001444 ± 67136.28 ± 2.67
[O III] 500741.51 ± 0.01320 ± 63281 ± 3474.23 ± 1.09
He I Narrow39.27 ± 0.41299 ± 63126 ± 250.59 ± 0.57
He I Broad40.68 ± 0.082200 ± 203934 ± 8614.83 ± 1.63
[O I] 630039.65 ± 0.22299 ± 63126 ± 251.62 ± 0.55
Hα Narrow40.93 ± 0.02299 ± 63126 ± 2533.33 ± 0.80
Hα Broad42.19 ± 0.011949 ± 691010 ± 25602.33 ± 2.99
[N II] 658540.70 ± 0.03299 ± 63126 ± 2519.81 ± 0.80
[S II] 671840.35 ± 0.06299 ± 63126 ± 259.18 ± 1.06
[S II] 673240.40 ± 0.06299 ± 63126 ± 2510.39 ± 1.16

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 SNR24.95
Hβ Broad SNR9.64
Hγ Broad SNR3.87
AGN frac0.43
Host frac0.57
log L5100,Host43.45
Fe II/Hβ0.15
Fe II/[O III]0.29

Quality flags

spurious_hab/hbb0.0/0
l51001
balmer0
balmer_snr0
hb_width1
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.