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
🔴 Emission Lines
Hydrogen Series
Lyman Series (n→1) — UV resonance
| Line | Rest λ (Å) | Obs λ (μm) | Transition | JWST |
| 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)
| Line | Rest λ (Å) | Obs λ (μm) | Rel. Flux | JWST |
| 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
| Line | Rest λ (Å) | Obs λ (μm) | Transition | JWST |
| 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
| Line | Rest λ (Å) | Obs λ (μm) | Transition | JWST |
| 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)
| Line | Rest λ (Å) | Obs λ (μm) | Notes | JWST |
| [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
| Line | Rest λ (Å) | Obs λ (μm) | Notes | JWST |
| [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
| Line | Rest λ (Å) | Obs λ (μm) | Notes | JWST |
| 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
| Line | Rest λ (Å) | Obs λ (μm) | Notes | JWST |
| [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
| Line | Rest λ (Å) | Obs λ (μm) | Notes | JWST |
| [ArIII]λ7136 |
7137.770 |
3.569 |
Ionization diag |
✓ |
| [ArIII]λ7751 |
7753.239 |
3.877 |
Ionization diag |
✓ |
Iron Lines (NIR)
| Line | Rest λ (Å) | Obs λ (μm) | Notes | JWST |
| [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)
| Line | Rest λ (Å) | Obs λ (μm) | Notes | JWST |
| 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)
| Line | Rest λ (Å) | Obs λ (μm) | Notes | JWST |
| 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
| Line | Rest λ (Å) | Obs λ (μm) | Diagnostic | JWST |
| 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
🛰️ 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.