Figure 3 from Wayne—A Simulator for HST WFC3 IR Grism Spectroscopy

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Wayne—A Simulator for HST WFC3 IR Grism Spectroscopy

2017 The Astrophysical Journal Supplement Series 231 13.

Caption: Figure 3.

WFC3 G102 and G141 grism sensitivity as calculated by Kuntschner et al. (2011). This step quantifies the conversion from flux to electrons.