Table 2.

Mastcam-Z Effective Wavelengths^a, Band Passes^b, Spectral Leakage^c, and Reference DN Level^d ($F_{\mathit{ref}}$)

Left Mastcam-Z				Right Mastcam-Z
Filter	${\lambda }_{\mathit{eff}}\pm \mathit{HWHM}$ (nm)	Leakage	$F_{\mathit{ref}}(DN)$	Filter	${\lambda }_{\mathit{eff}}\pm \mathit{HMWM}$ (nm)	Leakage	$F_{\mathit{ref}}(DN)$
L0R	630±43	0.43%	6185	R0R	631±43	0.4%	6151
L0Ge	544±41	0.26%	7212	R0Ge	544±42	0.36%	6984
L0B	480±46	1.1%	6834	R0B	480±46	1.2%	6821
L1f	800±9	0.66%	392	R1f	800±9	0.63%	396
L2f	754±10	0.6%	596	R2	866±10	0.62%	219
L3f	677±11	0.84%	1171	R3	910±12	0.61%	165
L4f	605±9	0.67%	1250	R4	939±12	0.64%	114
L5f	528±11	0.46%	1645	R5	978±10	0.63%	47
L6f	442±12	1.0%	1425	R6	1022±19	0.48%	59
L7	590±88,ND6g	–	–	R7	880±10, ND5g	–	–

^aEffective Wavelength (${\lambda }_{\mathit{eff}}$) is defined as the weighted average of wavelength with the normalized system spectral response ($\overline{r_{\lambda ,k}}$, see Sect. 3.5) and solar radiance at the top of the atmosphere ($S_{o_{ph}}$) in units of [$\frac{ph}{s{m}^{2}srnm}$]: ${\lambda }_{\mathit{eff}}=\frac{\int \overline{r_{\lambda ,k}}{S}_{o_{ph}}\lambda d\lambda }{\int \overline{r_{\lambda ,k}}{S}_{o_{ph}}d\lambda }$. The system spectral response includes the effects of the optics, filters, and detector quantum efficiency (see Sect. 3.5)

^bBandpasses are provided as the Half-Width-Half-Maximum (HWHM), which is defined as one-half the difference between the two wavelengths at which the response is half of the peak in-band response

^cSpectral Leakage is defined as the percentage ratio of the integrated out-of-band response to the integrated in-band-response of $\overline{r_{\lambda ,k}}$. For purposes herein, the in-band to out-of-band cutoff is defined as the closest wavelengths on either side of ${\lambda }_{\mathit{eff}}$ that correspond to 1% of the peak in-band response

^dThe reference DN level ($F_{ref,k}$) is defined as the above-bias signal of a 10 ms exposure observing, through filter k, a perfectly diffuse and white sunlit surface on Mars at zero-incidence when Mars is at perihelion (1.38 AU) and ignoring atmospheric attenuation (see Sect. 4.1.6)

^eThere are two identical green filters per 2 × 2 Bayer unit cell (see Fig. 3)

^fFilters where the narrowband response partially or completely blocks one or more of the Bayer RGB filter responses

^gNDX refers to a ${10}^{-X}$ neutral density coating for solar imaging