This data set contains Calibrated data taken by the New Horizons         Long Range Reconnaissance Imager                                       instrument during the                                                    Pluto encounter                                                        mission phase.  This is VERSION 3.0 of this data set.                    This data set contains LORRI observations taken during the               the Approach (Jan-Jul, 2015), Encounter, Departure, and                  Transition mission sub-phases, including flyby observations              taken on 14 July, 2015, and departure and calibration data               through late October, 2016. Departure observations include               a ring search of the Pluto system and 1994 JR1 observations.             This data set completes the Pluto mission phase deliveries for           LORRI.                                                                   This is version 3.0 of this dataset. Changes since version 2.0 include   the addition of data downlinked between the end of January, 2016 and the end of October, 2016, completing the delivery of all data covering the   Pluto Encounter and subsequent Calibration Campaign. It includes multi-  map observations from the Approach phase, observations of the moons, hi- res, full-frame observations from Pluto Encounter and Departure, sliver  maps, and ring search observations.  There may be some overlap between   prior datasets and this dataset, due to only partial, windowed, or lossy data in prior datasets.  Observations at closest approach to Pluto are   marked with _CA in the Request ID. This dataset also includes functional tests from the Calibration Campaign, including a regular observation of  NGC3532. Finally it includes the first set of distant KBO observations.  Also, updates were made to the calibration files, documentation, and     catalog files.                                                           There were minor changes to the level 2 LORRI calibration process, as    well as to the LORRI calibration constants for the final Pluto P3 PDS    delivery.                                                                The process change involves gap removal during calibration.  Files       with gaps come in many flavors, depending on where the gap lies within   the image. This update recognizes some additional possiblities, mainly   that the gap might be close to the bottom or top of the image (and       therefore the previous algorithm would fail because it filled the gap    with median pixel info from both above and below the gap). The new       algorithm will take the info from one side of the gap exclusively,       when appropriate.