PDS_VERSION_ID = PDS3 RECORD_TYPE = STREAM OBJECT = TEXT PUBLICATION_DATE = 2013-07-15 NOTE = "This file describes known errors or deficiencies in this archive volume set." END_OBJECT = TEXT END Please send comments by e-mail or U.S. mail to the PPI Node PDS Operator: This volume was produced for the Planetary Data System (PDS) at the Small Bodies node. The data, and associated metadata were supplied by Dr. Maria Teresa Capria at the Istituto Nazionale Astrofisica (INAF). The volume was assembled at the Dawn Science Center (DSC), by Joseph N. Mafi. Users are encouraged to provide feedback on any errors or omissions are found in the data or documentation. For questions or problems regarding PDS standards or volume organization please contact Dr. Carol Neese at the PDS Small Bodies Node: Email neese@psi.edu Telephone 520-622-6300 Mail Carol Neese Planetary Science Institute 1700 E. Ft. Lowell, Ste. 106 Tuscon, AZ 85719-2395 USA For question regarding the data please contact Dr. Maria Teresa Capria at INAF: Email mariateresa.capria@iaps.inaf.it Telephone +39-06-4993-4452 Mail Area di Ricerca di Tor Vergata via del Fosso del Cavaliere, 100 00133 Rome ITALY The PDS assumes no legal liability for errors on this disk. All users are encouraged to verify the correctness of the data prior to submitting any publications or other work based on these data. Please report errors on this disk to the Small Bodies Node of the PDS through the ERRATA reporting procedures described above. The 'Known Discrepancies' section below lists know deviations from PDS archiving standards found on this volume. ============================================================================== Known Discrepancies ============================================================================== MD5_CHECKSUM.TXT - This file does not have the required PDS label. It contains a list of the MD5 checksum of every file on this volume and is provided for data assurance purposes. Housekeeping Data File Record Length During the commisioning of the VIR instrument, several non-standard instrument modes were exercised. These modes have "SUBMODE NAMES" that are longer than the modes that are actually used for science data acquisition. Rather than convert all of the existing data sets (including Vesta) to match these few observations, we've decided to allow these files to have a slightly different format (record length, column start bytes) from the other files. These files are housekeeping data tables in the DATA/20071211_STARCAL directory. The impacted files are: VIR_VIS_1A_1_250697988_HK_2.TAB, VIR_VIS_1A_1_250698683_HK_2.TAB VIR_VIS_1A_1_250699236_HK_2.TAB, VIR_VIS_1A_1_250699571_HK_2.TAB VIR_VIS_1A_1_250700374_HK_2.TAB, VIR_VIS_1A_1_250700809_HK_2.TAB VIR_VIS_1A_1_250701244_HK_2.TAB, VIR_VIS_1A_1_250701489_HK_2.TAB