Table 2.

Distribution of the Opportunity Data Set on the Various Pancam Filters^a

Opportunity	λ	Ν	Ν1	Ν2	Ν3	Ν4	g	i
L7	432 nm	2,495	1,974	1,951	1,098	1013	10.6°–127.6°	0.7°–85.7°
R1	436 nm	1,539	1,397	1,390	802	754	11.0°–127.5°	0.9°–86.0°
L6	482 nm	1,872	1,485	1,471	877	827	10.6°–127.6°	0.2°–81.2°
L5	535 nm	2,373	1,891	1,888	1,021	952	10.5°–127.5°	0.2°–81.1°
L4	601 nm	1,637	1,359	1,355	890	830	10.5°–127.4°	0.2°–85.6°
L3	673 nm	1,067	879	875	547	517	10.5°–127.3°	0.3°–80.9°
L2	753 nm	2,527	2,011	2,009	1,126	1049	10.4°–127.2°	0.3°–85.5°
R2	754 nm	1,683	1,533	1,533	783	737	15.3°–128.2°	1.0°–81.6°
R3	803 nm	1,053	950	950	534	502	15.3°–125.5°	1.3°–81.7°
R4	864 nm	1,107	998	998	561	526	15.3°–125.6°	1.5°–81.8°
R5	904 nm	1,076	974	974	541	508	15.3°–125.7°	1.7°–81.9°
R6	934 nm	1,294	1,175	1,175	691	647	15.2°–125.8°	1.9°–82.0°
R7	1009 nm	1,490	1,357	1,357	846	791	15.2°–128.2°	1.9°–86.2°
Total		21,213	17,983	17,926	10,317	9653	10.4°–128.2°	0.2°–86.2°

^a N: Total data set for sols 1–3600. N1: Datapoints with a shadowed region available and no other serious problems. N2: Datapoints in N1 with an accepted single‐image fit. N3: Datapoints in N2, but only for sols 1–1220. N4: Datapoints in N3 after removal of data with the sun less than 30° from the specular point. The columns g and i show the range of phase and incidence angles for the N4 data set.