JWST Galaxy Spectral Lines

Galaxy Spectral Lines Interactive Reference

JWST Galaxy Spectral Lines

JWST NIRCam spectroscopy reference for galaxy observations at any redshift
with WFSS at 3.1-5.0 μm through the F356W and F444W filters with grisms

📊 All wavelengths sourced from SDSS DR7 vacuum standards and NIST atomic database
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
F356W NIRCam (3.0-4.0 μm)
F444W NIRCam (3.8-5.0 μm)

Observable Lines

🔴 Emission Lines

Hydrogen Series

Balmer Series (n→2)
LineRest λ (Å)Obs λ (μm)Rel. FluxJWST
6564.614 3.28 1.00
4862.721 2.43 0.35
4341.68 2.17 0.17
4102.89 2.05 0.10
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 5.03 n=7→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 10.83 n=7→4

Oxygen Forbidden Lines

LineRest λ (Å)Obs λ (μm)Flux RatioJWST
[OII]λ3727 3727.092 1.86 Doublet
[OIII]λ4959 4960.295 2.48 1:3
[OIII]λ5007 5008.239 2.50 3:1

Nitrogen & Sulfur Lines

LineRest λ (Å)Obs λ (μm)NotesJWST
[NII]λ6549 6549.86 3.27 Weaker NII
[NII]λ6584 6585.27 3.29 Stronger NII
[SII]λ6718 6718.29 3.36 Density diag
[SII]λ6732 6732.68 3.37 Density diag

High Ionization Lines

LineRest λ (Å)Obs λ (μm)TypeJWST
Lyα 1215.24 0.61 Often absorbed
C IV 1549.48 0.77 High ionization
C III] 1908.734 0.95 Semi-forbidden
Mg II 2799.117 1.40 AGN diagnostic

🔵 Stellar Absorption Lines

Strong Stellar Features

LineRest λ (Å)Obs λ (μm)DiagnosticJWST
Ca II K 3934.777 1.97 Age indicator
Ca II H 3969.588 1.98 Age indicator
G-band 4305.61 2.15 CH molecular
Mg I b 5176.7 2.59 Metallicity
Na I D 5895.6 2.95 Interstellar
Ca II λ8500 8500.36 4.25 NIR triplet
Ca II λ8544 8544.44 4.27 NIR triplet
Ca II λ8664 8664.52 4.33 NIR triplet
Observable with current grism selection
Outside current grism coverage
F356W Coverage
F444W 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