Description of the calibration corrections to fix the error introduced by differences in the shutter opening direction. Problem ------------ The double-bladed shutter utilized by the camera has a delay in its slide mechanism that introduces an offset in the actual exposure time, compared to the commanded exposure time. It was originally reported that exposures with the forward shutter direction were 1.65 ms shorter than the commanded exposure time, while images with the reverse shutter direction were as commanded. During the recalibration of the NAVCAM instrument as part of the Stardust NExT extended mission, it was found that the original offsets were incorrect. During the recalibration (which will be fully documented in the Stardust NExT archive) it was found that offsets are present in both the forward and reverse directions. For exposures with a forward shutter direction, the exposure time is 0.40 ms longer than the commanded time, while those in the reverse direction have an exposure time 1.34 ms shorter than the commanded time. It was also previously reported that the parity (where all even frame numbers have one shutter direction and odd numbers have the other) only changed when a bias frame was taken, since the shutter blades didn't fire. It was subsequently found, however, that the shutter resets to the forward direction when the NAVCAM power is cycled, potentially changing the parity in a sequence of images. Furthermore, there are occasions when an image wasn't obtained for some reason, which also has the potential for changing the parity. Descriptions of the images are included in the DATASET.CAT file and the PIIMGLOG.ASC document, where information can be found about bias frames and potentially missed images. Questions about the Parity ----------------------------- A list of all Stardust images is included in the file SHUTTER_PARITY_LIST.ASC in the documents directory, interspersed with the times of NAVCAM power cycles and notes about bias frames and potentially missed images. The parity of each image, as well as can be determined, is noted in this document. There are still ambiguities, where it is not known if an image was skipped (thus changing the parity) or if it was obtained but not downloaded (thus maintaining the parity). The information in this document is used to determine how to apply the exposure corrections with regards to the shutter direction. As can be seen in this document, the shutter direction is known for most of the images. However, there are several groups of data where a "missing" image introduces an ambiguity in the shutter direction of subsequent images (e.g., it is not known whether the shutter triggered or not). Fortunately, most of the ambiguous sequences consist of long exposure images (>1000 ms). Exposures this long are essentially unaffected by the difference in actual and commanded exposure time (the <0.1% effect is well within the calibration errors of the instrument). The one potential exception to this case involves the Anne Frank images, where only every third image was saved in the frames 374 through 426. It is possible that the shutter did not fire on one of the unsaved images, changing the parity. Tests performed at the SBN suggest that this is not the case, and that the shutter direction listed in the SHUTTER_PARITY_LIST.ASC is indeed correct, though this is not absolutely confirmed. (It should be noted that these images are not calibrated, and many of them are partially saturated, minimizing the problems related to the true exposure time.) Exposure Time Corrections -------------------------- Because of the ambiguous long-exposure images, combined with the fact that the shutter exposure correction is negligible for long exposures, it was decided that, for consistency, corrections would only be applied to the shorter exposures where they actually affect the photometric measurements. Thus, the exposure times for all images with commanded exposure times shorter than 1000 ms have been corrected for the shutter timing offsets. The following corrections are applied to each image as relevant, given the information in the SHUTTER_PARITY_LIST.ASC document. For the following steps, the commanded exposure time is converted to the actual exposure time by an increase of 0.4 ms for images with the 'F' designation, and a decrease of 1.34 ms for images denoted 'R'. 1) The EXPOSURE keyword in the FITS header is corrected to the actual exposure time. 2) The EXP_CMND keyword is added to the FITS header to denote the originally commanded exposure time. 3) The EXPOSURE_DURATION keyword in the PDS label is corrected to the actual exposure time. 4) In the datasets containing calibrated images, the flux levels are adjusted to account for the difference in exposure times (e.g. flux levels are multiplied by t_cmnd/t_actual).