{"@type": "dcat:Dataset", "accessLevel": "public", "bureauCode": ["026:00"], "contactPoint": {"@type": "vcard:Contact", "fn": "Planetary Data System", "hasEmail": "mailto:pds-operator@jpl.nasa.gov"}, "description": "This data set contains Raw 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.", "identifier": "urn:nasa:pds:context_pds3:data_set:data_set.nh-p-lorri-2-pluto-v3.0;urn:nasa:pds:context_pds3:data_set:data_set.nh-p-lorri-2-pluto-v3.0::1.0", "keyword": ["__"], "license": "https://www.usa.gov/government-works", "modified": "2026-04-06", "programCode": ["026:000"], "publisher": {"@type": "org:Organization", "name": "Small Bodies"}, "theme": ["Planetary Science"], "title": "NEW HORIZONS  LORRI PLUTO ENCOUNTER  RAW V3.0"}