Dataset Overview
  =================

      This CODMAC level 4 data set contains
      solar stray light corrected, radiometric calibrated and geometric
      distortion corrected (resampled) image data in W/m^2/sr/nm,
      acquired by the OSIRIS Narrow Angle Camera on the Rosetta spacecraft
      during the ROSETTA EXTENSION 1 mission phase, covering the period
      from 2016-01-12T23:25:00.000 to 2016-02-09T23:24:59.000

      All header keywords are defined and described in the OSIRIS SIS:
      \DOCUMENT\SIS\OSIRIS_SIS_V05.PDF.


      Note that the data part of the FITs files in the /DATA/FIT directory is
      identical to the data part of the PDS files in the /DATA/IMG directory.
      FITs files are delivered only for CODMAC levels 2,3, and 4 datasets.
      No FITs files are delivered for CODMAC level 5 datasets.

  Credit Line
  =================
      To be used for image display (presentations, public exposure, etc.)
      and figure captions (e.g., in scientific articles).

      ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA

  Acknowledgment
  =================
      Full acknowledgment (e.g., in acknowledgment section of scientific
      article).

      The authors acknowledge the OSIRIS Principal Investigator H. Sierks
      (MPS, Goettingen, Germany) and the OSIRIS Team for providing images
      and related datasets and the ESA Rosetta Project to enable the
      science of the mission.

  Essential Reading
  =================

      The following documents, located on the dataset DOCUMENT folder, are
      essential for the understanding and interpretation of this dataset:

      KELLER_ET_AL_2007_V01.PDF:   Gives an overview of the science goals
                                   of the OSIRIS instrument and an overview
                                   of the instrument hardware.

      OSIRIS_SIS_V05.PDF:          Describes the OSIRIS PDS header

      SCIENCE_USER_GUIDE_V03.PDF:  Describes the intention behind the
                                   acquisition of each image and its planned
                                   scientific purpose.

  Related Datasets
  =================
      The following PDS datasets are related:

      RO-C-OSINAC-2-EXT1-67PCHURYUMOV-M25-V3.0
      RO-C-OSINAC-3-EXT1-67PCHURYUMOV-M25-V3.0
      RO-C-OSINAC-4-EXT1-67P-M25-REFLECT-V1.0
      RO-C-OSINAC-4-EXT1-67P-M25-STR-REFL-V1.0
      RO-C-OSINAC-4-EXT1-67PCHURYUMOV-M25-V2.0
      RO-C-OSINAC-5-EXT1-67P-M25-GEO-V1.0
      RO-C-OSIWAC-2-EXT1-67PCHURYUMOV-M25-V3.0
      RO-C-OSIWAC-3-EXT1-67PCHURYUMOV-M25-V3.0
      RO-C-OSIWAC-4-EXT1-67P-M25-REFLECT-V1.0
      RO-C-OSIWAC-4-EXT1-67P-M25-STR-REFL-V1.0
      RO-C-OSIWAC-4-EXT1-67P-M25-STRLIGHT-V1.0
      RO-C-OSIWAC-4-EXT1-67PCHURYUMOV-M25-V2.0
      RO-C-OSIWAC-5-EXT1-67P-M25-GEO-V1.0


      Please note that different datasets can contain different number of
      images. For details see OSIRIS_CAL_PIPELINE_V06.PDF
      and SCIENCE_USER_GUIDE_V03.PDF.

  Change log
  ==========

      V1.0 Lien corrected dataset after October 2018 PSA/PDS
           external peer review.

Essential Reading
  =================
      The following documents, located on the dataset DOCUMENT folder, are
      essential for the understanding and interpretation of this dataset:

      TUBIANA_ET_AL_2015_V01.PDF:  Describes the quality of calibration