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
Hα 6564.614 3.282 1.00 ✓
Hβ 4862.721 2.431 0.35 ✗
Hγ 4341.684 2.171 0.17 ✗
Hδ 4102.892 2.051 0.10 ✗
Hε 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