Left: SXI images in detector coordinates showing the two OBSIDs used in the SXI analysis. The blue square shows the SXS FoV. The arrow in the left-hand panel shows the direction N 132 D drifted in the focal plane during that OBSID, with black crosses marking the source center in intervals of one hour. N 132 D was in the SXS FoV for only 3.7 ks of OBSID 100041010, and for none of OBSID 100041020. The remnant was still visible in SXI due to that detector’s larger FoV. Right: Attitude of Hitomi during the first 7 ks of OBSID 100041010. The solid line shows ANG_DIST, the angular distance in arcminutes between the intended pointing and the actual pointing. Bins show the good time intervals of the default data filtering, which requires ANG_DIST < 1|$ {^{\prime}_{.}} $|5, and the additional ∼ 43% of time added by relaxing this criterion to 2|$ {^{\prime}_{.}} $|2. Blank times are excluded because of Earth’s occultation or the South Atlantic Anomaly passage. (Color online)