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N132D Data Cube
Large Magellanic Cloud Supernova Remnant · Schematic Model

N132D Data Cube

Treat the remnant's emission as a three-dimensional (x, y, E) cube. Every X-ray instrument slices it into resolution cells of different shapes: some fine in space and coarse in energy, others the reverse. RGS is the most unusual — it couples energy and the y direction onto a single coordinate.

Top-down · x–y imaging planeLooking down the E axis
XMM RGS
0.4 keV2.0 keV
0.0 s
24°
300°

y–E plane

Summed over x

Integrated spectrum