NASA SPHEREx · IPAC/IRSA DR1 · 0.75–5.0 µm
Module 03 · 8 min · Intermediate

Reading a Spectrum

How to interpret spectral graphs

Real spectrum: Orion Nebula, one cube pixel
DR1 cube
Extracting spectrum from the science cube… 0.0s

Hover to read values. Bars along the bottom show NHITS.

01

Axes

Wavelength (µm) runs left to right; surface brightness in MJy/sr runs up. The shape — slopes, dips, bumps — carries the physics.

02

Continuum vs features

Look for the smooth continuum first, then deviations that span several adjacent channels: absorption dips (ices, molecules) or emission bumps (PAHs, recombination lines).

03

Check the quality columns

NHITS tells you how many input pixels contributed; FLAGS tells you if a channel is suspect. A feature in flagged channels is not a feature yet.

Imagery & science data: NASA / Caltech-IPAC SPHEREx DR1 via IRSA. Catalogue overlay: d3-celestial (BSD-3).StellarScope · created by Vaishal Anil & Parthiv — Team The Abyss, NASA Space Apps 2026AI: IFM K2 Horizon · NVIDIA Nemotron · Spectral Scout v2 (ONNX)