Data Set Overview
  =================
 
    This dataset contains data generated by MIRO during the Lutetia
    Flyby mission phase of Rosetta and also data obtained during the
    IFP Noise Figure Test of Active Payload Checkout 12, which fell
    in the same Mission Phase. These data cover the following periods
    and activities:
 
    (All are in 2010, so Year is omitted from dates.)
 
    Start Time       Stop Time         Activity
   (mm-ddThh:mm)   (mm-ddThh:mm)
 
    04-30T16:30     04-30T18:17     PC12 IFP Noise Figure Test
    07-10T05:45     07-10T15:45     Approach observations of Lutetia
    07-10T15:45                     Closest Approach to Lutetia
    07-10T15:45     07-10T16:45     Recession observations of Lutetia
    07-11T03:45     07-11T06:15     Observations of dark sky
 
  Author List
  ===========
 
    The author list in the CITATION_DESC includes only those persons
    who worked on preparing this archive dataset for delivery.  The
    full list of all persons involved in the MIRO experiment is
    (taken from the GULKISETAL2007 reference):
    S. Gulkis, Frerking, M., Crovisier, J., Beaudin, G., Hartogh, P.,
    Encrenaz, P., Koch, T., Kahn, C., Salinas, Y., Nowicki, R.,
    Irigoyen, R., Janssen, M., Stek, P., Hofstadter, M., Allen, M.,
    Backus, C., Kamp, L., Jarchow, C., Steinmetz, E., Deschamps, A.,
    Krieg, J., Gheudin, M., Bockelee-Morvan, D., Biver, N., Encrenaz,
    T., Despois, D., Ip, W., Lellouch, E., Mann, I., Muhleman, D.,
    Rauer, H., Schloerb, P., and Spilker, T.
 
  Geometry Information
  ====================
 
    The MIRO data file labels contain vectors specifying the position
    of the Sun and Target body relative to the spacecraft and the
    velocity of the Target body relative to the spacecraft.  The value
    s of the keywords SC_SUN_POSITION_VECTOR,
    SC_TARGET_POSITION_VECTOR and SC_TARGET_VELOCITY_VECTOR are
    related to the ECLIPJ2000 reference frame.  The values of
    SUB_SPACECRAFT_LATITUDE and SUB_SPACECRAFT_LONGITUDE are northern
    latitude and eastern longitude in the standard planetocentric IAU
     frame.  All values are computed for the the midpoint
    of the observations.  Distances are given in , velocities in
    , angles in .
 
    This information was obtained using the following NAIF/SPICE
    kernel files:
 
    ROS_LUTETIA_RSOC_V01.TPC
    ORHR_______________00109.BSP
    ORHS_______________00109.BSP
    de405.bsp
 
    The vectors were retrieved using the NAIF call SPKEZ() with a
    correction for one-way light time and stellar aberration using a
    Newtonian formulation.

These data were not processed in any way
    other than being decommutated from the raw telemetry stream, so no
    processing errors are expected.  For a discussion of the
    reliability of the MIRO instrument itself, see the documentation
    included with this and subsequent mission archives.