JWST Galaxy Spectral Lines

Galaxy Spectral Lines Interactive Reference

JWST Galaxy Spectral Lines

JWST NIRCam WFSS reference for galaxy observations at any redshift
F356W grism (3.0–4.0 μm) + F444W grism (3.8–5.0 μm) used simultaneously

📊 All wavelengths are vacuum (Å) — sources: SDSS DR7, NIST ASD, Morton (2003, ApJS, 149, 205), Osterbrock & Ferland (2006)
z = 4.0 | Lookback Time: ~12.5 Gyr | Universe Age: ~1.2 Gyr

📡 Observed Wavelength Positions & JWST Coverage

1.0 μm 2.0 μm 3.0 μm 4.0 μm 5.0 μm 6.0 μm

Observable Lines

🔴 Emission Lines

Hydrogen Series

Lyman Series (n→1) — UV resonance
LineRest λ (Å)Obs λ (μm)TransitionJWST
Lyα 1215.670 0.608 n=2→1
Lyβ 1025.722 0.513 n=3→1
Lyγ 972.537 0.486 n=4→1
Lyδ 949.743 0.475 n=5→1
Balmer Series (n→2)
LineRest λ (Å)Obs λ (μm)Rel. FluxJWST
6564.614 3.282 1.00
4862.721 2.431 0.35
4341.684 2.171 0.17
4102.892 2.051 0.10
3970.072 1.985 0.06
H6 (Hζ) 3889.064 1.945 0.04
H7 (Hη) 3835.391 1.918 0.03
H8 3797.904 1.899 0.02
H9 3771.701 1.886 0.02
H10 3750.153 1.875 0.01
Paschen Series (n→3) - Infrared
LineRest λ (Å)Obs λ (μm)TransitionJWST
Pa α 18756.0 9.38 n=4→3
Pa β 12821.6 6.41 n=5→3
Pa γ 10941.1 5.47 n=6→3
Pa δ 10052.1 5.026 n=7→3
Pa ε 9547.6 4.774 n=8→3
Pa ζ 9231.6 4.616 n=9→3
Pa 8 9017.4 4.509 n=10→3
Brackett Series (n→4) - Far-Infrared
LineRest λ (Å)Obs λ (μm)TransitionJWST
Br α 40522.8 20.26 n=5→4
Br β 26258.7 13.13 n=6→4
Br γ 21661.2 10.831 n=7→4
Br δ 19450.7 9.725 n=8→4
Br ε 18178.6 9.089 n=9→4

Neon Lines (AGN / Ionization)

LineRest λ (Å)Obs λ (μm)NotesJWST
[NeV]λ3347 3346.790 1.673 AGN tracer
[NeV]λ3427 3426.843 1.713 AGN tracer
[NeIII]λ3870 3869.856 1.935 Ionization diag
[NeIII]λ3969 3968.590 1.984 Blends with Hε

Oxygen Forbidden Lines

LineRest λ (Å)Obs λ (μm)NotesJWST
[OII]λ3727 3727.092 1.864 Doublet (density)
[OII]λ3730 3729.875 1.865 Doublet (density)
[OIII]λ4363 4364.436 2.182 Auroral — Te diag
[OIII]λ4959 4960.295 2.480 Doublet 1:3
[OIII]λ5007 5008.239 2.504 Doublet 3:1
[OI]λ6300 6302.046 3.151 Shock / AGN
[OI]λ6364 6365.536 3.183 1/3 of [OI]6300
[OII]λ7322 7321.977 3.661 Te diagnostic
[OII]λ7333 7332.590 3.666 Te diagnostic

Helium Lines

LineRest λ (Å)Obs λ (μm)NotesJWST
He II λ4687 4687.015 2.344 AGN / WR stars
He I λ5877 5877.249 2.939 Recombination
He I λ6678 6679.995 3.340 Recombination
He I λ7065 7067.138 3.534 Triplet
He I λ10830 (weak) 10829.091 5.415 2³P₀→2³S₁ (weak)
He I λ10830 (med) 10830.250 5.415 2³P₁→2³S₁ (medium)
He I λ10830 (strong) 10830.340 5.415 2³P₂→2³S₁ (strongest) — winds/AGN

Nitrogen & Sulfur Lines

LineRest λ (Å)Obs λ (μm)NotesJWST
[NII]λ5755 5756.185 2.878 Auroral — Te diag
[NII]λ6549 6549.860 3.275 Doublet weak
[NII]λ6584 6585.270 3.293 Doublet strong — BPT
[SII]λ6718 6718.290 3.359 Density diag
[SII]λ6732 6732.680 3.366 Density diag
[SIII]λ9069 9071.100 4.536 Strong NIR
[SIII]λ9532 9533.200 4.767 Strong NIR

Argon Lines

LineRest λ (Å)Obs λ (μm)NotesJWST
[ArIII]λ7136 7137.770 3.569 Ionization diag
[ArIII]λ7751 7753.239 3.877 Ionization diag

Iron Lines (NIR)

LineRest λ (Å)Obs λ (μm)NotesJWST
[Fe II] 1.257 μm 12570.0 6.285 Shock / AGN
[Fe II] 1.644 μm 16436.0 8.218 Shock / SFR

UV Lines (AGN / High-z tracers)

LineRest λ (Å)Obs λ (μm)NotesJWST
N V λ1239 1238.821 0.619 AGN / HII
N V λ1243 1242.804 0.621 AGN / HII
Si IV λ1394 1393.755 0.697 ISM / wind
Si IV λ1403 1402.770 0.701 ISM / wind
C IV λ1548 1548.205 0.774 Doublet — AGN
C IV λ1551 1550.779 0.775 Doublet — AGN
He II λ1640 1640.420 0.820 AGN / WR indicator
O III] λ1661 1660.809 0.830 Semi-forbidden doublet
O III] λ1666 1666.150 0.833 Semi-forbidden doublet
Al III λ1855 1854.718 0.927 AGN BLR
Al III λ1863 1862.790 0.931 AGN BLR
C III] λ1907 1906.683 0.953 Semi-forbidden doublet
C III] λ1909 1908.734 0.954 Semi-forbidden doublet
Mg II λ2796 2796.352 1.398 Doublet — AGN
Mg II λ2804 2803.531 1.402 Doublet — AGN

🔵 Stellar & ISM Absorption Lines

UV ISM / CGM Absorption

Vacuum wavelengths from Morton (2003, ApJS, 149, 205)

LineRest λ (Å)Obs λ (μm)NotesJWST
Si II λ1260 1260.422 0.630 Strong ISM
O I λ1302 1302.169 0.651 ISM + geocoronal
Si II λ1304 1304.370 0.652 ISM
C II λ1334 1334.532 0.667 Strong ISM
Fe II λ1608 1608.451 0.804 ISM iron
Al II λ1671 1670.787 0.835 Strong ISM
Si II λ1527 1526.707 0.763 ISM
Fe II λ2344 2344.214 1.172 ISM iron complex
Fe II λ2374 2374.461 1.187 ISM iron complex
Fe II λ2383 2382.765 1.191 ISM iron complex
Fe II λ2587 2586.650 1.293 ISM iron complex
Fe II λ2600 2600.173 1.300 Strongest ISM FeII
Mg I λ2853 2852.963 1.426 ISM / stellar

Strong Stellar Features

LineRest λ (Å)Obs λ (μm)DiagnosticJWST
Ca II K 3934.777 1.967 Age indicator
Ca II H 3969.588 1.985 Age indicator
G-band 4305.610 2.153 CH molecular band
Hβ abs 4862.721 2.431 Stellar Balmer abs
Mg I b 5176.700 2.588 Metallicity
Na I D 5895.600 2.948 ISM / stellar
Hα abs 6564.614 3.282 Stellar Balmer abs
Ca II λ8498 8500.360 4.250 NIR triplet
Ca II λ8542 8544.440 4.272 NIR triplet
Ca II λ8664 8664.52 4.33 NIR triplet
Observable with current selection
Outside current coverage

🛰️ JWST NIRCam Grism Specifications

F356W Grism: λ = 3.0–4.0 μm, R ~ 1600, optimal for z = 4–6 Hα, [OIII], [SII] observations

F444W Grism: λ = 3.8–5.0 μm, R ~ 1600, optimal for z = 5–7 Hα, higher-z [OIII] observations

Observing Strategy: Use both grisms for optimal line coverage across different redshift ranges

📋 Selected Line Details

Click on any line in the tables above to see detailed information and observability.

Created by: Ronaldo Laishram

© 2025 Ronaldo Laishram | www.ronaldolaishram.com

Galaxy Spectral Lines Interactive Reference for JWST NIRCam Observations