Cassini/VIMS observations of Jupiter
<|begin_of_text|><|start_header_id|>system<|end_header_id|> You are a research archivist expert in dataset metadata. Answer the question truthfully.  <|eot_id|><|start_header_id|>user<|end_header_id|> Here is the Description of a dataset. Description:'This is a set of reduced data taken by Cassini VIMS at Jupiter.  Contained within is a series of VIMS data cubes, reduced using the VIMS team calibration system - the data was reduced for emission (and so values are in Wm-2 equivalent, rather than I/F).  Each of these cubes also has a 'backplane' IDL file, containing outputs from SPICE in IDL structures - 'back_1bar' is projected for the surface, 'back_515' is for the peak of the ionosphere, and 'back' is for 1000km above the surface.  (These backplanes were developed for Saturn, so ignore values for ring and Enceladus positioning.)This includes a wide array of information, either in single values or arrays for each structure: PHASE,EMISSION,INCIDENCE,RA,DEC,LAT,LON,SCLOC,SCVEL,RA_TARG,DEC_TARG,LAT_SUBPT,LON_SUBPT,LAT_SUNPT,LON_SUNPT,ALT,PHASE_TARG,EMISSION_TARG,INCIDENCE_TARG,SUN_E' . Please return only a json list of at most 3 Keywords corresponding to the Description:.<|eot_id|><|start_header_id|>assistant<|end_header_id|> {"Answer" : ["Jupiter"]} <|eot_id|>
 Here is the Description of a dataset. Description:'This is a set of reduced data taken by Cassini VIMS at Jupiter.  Contained within is a series of VIMS data cubes, reduced using the VIMS team calibration system - the data was reduced for emission (and so values are in Wm-2 equivalent, rather than I/F).  Each of these cubes also has a 'backplane' IDL file, containing outputs from SPICE in IDL structures - 'back_1bar' is projected for the surface, 'back_515' is for the peak of the ionosphere, and 'back' is for 1000km above the surface.  (These backplanes were developed for Saturn, so ignore values for ring and Enceladus positioning.)This includes a wide array of information, either in single values or arrays for each structure: PHASE,EMISSION,INCIDENCE,RA,DEC,LAT,LON,SCLOC,SCVEL,RA_TARG,DEC_TARG,LAT_SUBPT,LON_SUBPT,LAT_SUNPT,LON_SUNPT,ALT,PHASE_TARG,EMISSION_TARG,INCIDENCE_TARG,SUN_E' . Please return only a json list of at most 3 Keywords corresponding to the Description:.
This is a set of reduced data taken by Cassini VIMS at Jupiter.  Contained within is a series of VIMS data cubes, reduced using the VIMS team calibration system - the data was reduced for emission (and so values are in Wm-2 equivalent, rather than I/F).  Each of these cubes also has a 'backplane' IDL file, containing outputs from SPICE in IDL structures - 'back_1bar' is projected for the surface, 'back_515' is for the peak of the ionosphere, and 'back' is for 1000km above the surface.  (These backplanes were developed for Saturn, so ignore values for ring and Enceladus positioning.)This includes a wide array of information, either in single values or arrays for each structure: PHASE,EMISSION,INCIDENCE,RA,DEC,LAT,LON,SCLOC,SCVEL,RA_TARG,DEC_TARG,LAT_SUBPT,LON_SUBPT,LAT_SUNPT,LON_SUNPT,ALT,PHASE_TARG,EMISSION_TARG,INCIDENCE_TARG,SUN_E
Jupiter