PDS_VERSION_ID = PDS3 RECORD_TYPE = STREAM OBJECT = TEXT PUBLICATION_DATE = 2008-07-28 /* Label Generated */ NOTE = "Description of the contents of the document directory." END_OBJECT = TEXT END "document" Directory Contents The document directory contains documentation files, where available, for the data set in this volume. All document files will have an accompanying label file to describe content and structure. Label files have the same name as the main document file, with an extension of ".lbl". docinfo.txt - The file you are reading. ads.txt - The file sent to Abstract Data Service (ADS). ads.lbl - The label for ads.txt. checksum.tab - A table of checksums for all the data files. checksum.lbl - The label for checksum.tab. 0graphics.asc - "Description of Occultation Graphics", This document is a description of the graphics images of the asteroid occultation observations, supplied with this data set. The graphics images themselves are .jpg files with filenames which concatenate the asteroid name, asteroid number or provisional designation, and occultation date. 0graphics.lbl - The label file for the document "Description of Occultation Graphics" described above. 100hekate2004feb12.jpg 1021flammario2005apr11.jpg 1024hale2002feb26.jpg 1024hale2004mar23.jpg [836 more files not listed] - "Graphics of Asteroid Occultation Observations", Graphics of Asteroid occultation observations. March 2008. These plots of the occultation observations have a filename convention concatenating the asteroid number, asteroid name or provisional designation, and occultation date. The heading for each plot gives the following information: Line 1 Object identification, event date, ellipse size and orientation, and associated uncertainties. Line 2 The offset of the shadow from the center of the earth, and associated uncertainty values. Line 3 [Only when a double star is involved.] The separation and Position angle of the components of the double star, with associated uncertainty. Important. In all lines, an uncertainty value is only given if there has been a meaningful calculation of the particular quantity. Where there is no uncertainty value, usually the particular value has been assumed. The coding used in the plots is as follows: Event type * Disappearance events are plotted in Red. * Reappearance events are plotted in Green * Miss events are plotted in grey. * For some events, the predicted central path is plotted. This is drawn using a purple dashed line. Observing method * Events recorded visually are plotted with a '+' * Video/CCD observations are plotted with a small square. * Miss events are plotted with a 'x'. Plot style The plot is drawn in a manner that depends on the detail that is derived from the observations. * For the best-observed events, the observations are drawn without any best-fit ellipse, or joining pairs of observations. This better enables the irregulaities in the asteroid profile to be visible. * For well-observed events, a best-fit ellipse is drawn through the observations. The ellipse illustrates the shape of the asteroid. * For poorly-observed events, a gray line joins the events of each observer. That is, it shows the time during which the star was invisible to the observer. Double stars. For a small number of events, a double star is involved. When this occurs, the plot includes a representation of the double star, drawn on the same projected scale as the plot of the asteroid. graphics_of_asteroid_occult.lbl - The label file for the document "Graphics of Asteroid Occultation Observations" described above.