X-ray extinction from interstellar dust - Prospects of observing carbon, sulfur, and other trace elements

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Table 1

Parameters of the instruments used in the simulations at the energy of the elements studied in this work.

Element	R		Inst.
	E/ΔE	cm²
C	2540	369	Arcus
Al	621	11 022	XIFU
S	986(352)	5949(209)	XIFU(Resolve)
Ca	1611(575)	3734(271)	XIFU(Resolve)
Ti	1984	2742	XIFU
Ni	3331	704	XIFU

Notes. The energy resolution is 2.5 and 5 eV for XIFU and Resolve, respectively. Arcus resolution is defined by its resolving power R ~3000 over the 0.5–1 keV band.

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