Extensive land use and geographic data at the tax lot level in comma-separated values (CSV) file format. The PLUTO files contain more than seventy fields derived from data maintained by city agencies. All previously released versions of this data are available at BYTES of the BIG APPLE- Archive

The New Horizons Pluto Encounter Surface Composition data set contains map data from the Multispectral Visible Imaging Camera instrument and the Linear Etalon Imaging Spectral Array instrument on New Horizons during the Pluto encounter mission phase. Color, albedo, and absorption map data products are included for the CH4, N2, CO, and H2O species. This is VERSION 1.0 of this data set.

Map of Pluto's incidence-angle-average bolometric hemispherical albedo (local energy-balance albedo, equal to one minus absorption). The map is based on analyses of New Horizons Long Range Reconnaissance Imager (LORRI) and Multispectral Visible Imaging Camera (MVIC) images of Pluto in 2015.

This dataset represents a compilation of data from various government agencies throughout the City of New York. The underlying geography is derived from the Tax Lot Polygon feature class that is part of the Department of Finance's Digital Tax Map (DTM). The tax lots have been clipped to the shoreline, as defined by NYCMap planimetric features. The attribute information is from the Department of City Planning's PLUTO data. The attribute data pertains to tax lot and building characteristics and geographic, political and administrative information for each tax lot in New York City.The Tax Lot Polygon feature class and PLUTO are derived from different sources. As a result, some PLUTO records do not have a corresponding tax lot in the Tax Lot polygon feature class at the time of release. These records are included in a separate non-geographic PLUTO Only table. There are a number of reasons why there can be a tax lot in PLUTO that does not match the DTM; the most common reason is that the various source files are maintained by different departments and divisions with varying update cycles and criteria for adding and removing records. The attribute definitions for the PLUTO Only table are the same as those for MapPLUTO. DCP Mapping Lots includes some features that are not on the tax maps. They have been added by DCP for cartographic purposes. They include street center 'malls', traffic islands and some built streets through parks. These features have very few associated attributes.To report problems, please open a GitHub issue or email DCPOpendata@planning.nyc.gov.DATES OF INPUT DATASETS:Department of City Planning - E-Designations: 2/5/2021Department of City Planning - Zoning Map Index: 7/31/2019Department of City Planning - NYC City Owned and Leased Properties: 11/15/2020Department of City Planning - NYC GIS Zoning Features: 2/5/2021Department of City Planning - Polictical and Administrative Districts: 11/17/2020Department of City Planning - Geosupport version 20D: 11/17/2020Department of Finance - Digital Tax Map: 1/30/2021Department of Finance - Mass Appraisal System (CAMA): 2/10/2021Department of Finance - Property Tax System (PTS): 2/6/2021Landmarks Preservation Commission - Historic Districts: 2/4/2021Landmarks Preservation Commission - Individual Landmarks: 2/4/2021Department of Information Telecommunications & Technology - Building Footprints: 2/10/2021Department of Parks and Recreation - GreenThumb Garden Info: 1/4/2021

Extensive land use and geographic data at the tax lot level in GIS format (ESRI Shapefile). Contains more than seventy fields derived from data maintained by city agencies, merged with tax lot features from the Department of Finance’s Digital Tax Map, clipped to the shoreline. All previously released versions of this data are available at BYTES of the BIG APPLE- Archive

This data set contains global color maps, image cubes, and absorption band maps created from calibrated data taken during the PLUTO mission phase by the Linear Etalon Imaging Spectral Array (LEISA) instrument and the Multispectral Visible Imaging Camera (MVIC) instrument on the New Horizons spacecraft. Image cubes are provided per instrument and target body, covering the surfaces of Pluto, Charon, Nix, Hydra, and Kerberos. Color maps and absorption band maps for N2, CO, CH4, and H2O are provided for both Pluto and Charon.

This data set contains derived geology and geophysical maps of Pluto and Charon derived from data taken by the New Horizons Multispectral Visible Imaging Camera (MVIC) and the Long-range Reconnaissance Imager (LORRI) instruments during the Pluto Encounter mission phase.

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.

Table S1 is a comma-delimited text file (.csv) that contains a list of all craters between 7-to-25 km, their feature identification number (FID), their longitude and latitude in decimal degrees, and the unit abbreviation for the geologic unit they were assigned to.These data are associated with a Singer et al. manuscript submitted to the Journal of Geophysical Research - Planets. The title is "Pluto Geologic Map: Use of Crater Data to Understand Age Relationships". Publication information, including a DOI, will be updated upon completion of the peer review process.Abstract: Pluto’s surface displays a wide variety of geologic units from smooth plains to extremely rugged mountainous expanses. These terrains range in age from young, actively resurfaced regions (no observable craters even in the highest-resolution New Horizons images) to old, heavily cratered, eroded regions. Here we expand upon the crater data analysis and the independent crater data set used in the production of a 1:7M scale geologic map of Pluto that is to be published by the United States Geologic Survey (USGS). We present both relative ages based on crater spatial density (number of craters in a given size bin per km2) and also quantitative ages (e.g., 2 Ga) using the estimated impactor flux onto Pluto. The techniques presented here were developed specifically for the information available from a USGS geologic map, where smaller craters are mapped as points only (no specific diameter information per crater). We developed a new type of visualization, called a distributed R-plot, to understand the relative ages of the geologic units. The uncertainties in the current knowledge of the Kuiper belt populations and impactor flux at Pluto propagate to large uncertainties in the estimated quantitative ages (~a factor of two). However, both relative and quantitative ages from crater analysis were still valuable tools in developing the sequence of geologic events. Pluto has large areas of crater-free young terrains (13 units making up ~27% of mapped higher-resolution surface area), with widely varying morphologies, indicating a variety of resurfacing mechanisms, both exogenic and endogenic, likely active into Pluto’s recent past or present.

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 2.0 of this data set. This data set contains LORRI observations taken during the the Approach (Jan-Jul, 2015) and Encounter mission sub-phases, including flyby observations taken on 14 July, 2015; the data are limited to those downlinked from the spacecraft as of the end of January, 2016. The rest of the downlinked data for this mission phase will be delivered in a future data set. Refer to the data set description above and the sequence table provided in the documentation for more detail about which observations are present in this data set. This is version 2.0 of this data set. Changes since version 1.0 include data downlinked between the end of July, 2015 and the end of January, 2016. These include Pluto Charon, Nix and Hydra observations from Approach, the day of the flyby, and Departure, lossless downlinks of images downlinked with lossy compression in version 1.0, Nix orbit determination observations, Multi-maps and VIS-UV maps taken in coordination with ALICE, High-phase and departure imaging, satellite photometry, non-critical navigation imaging, Kerberos and Styx imaging, KBO 1994 JR1 observations and departure ring-search observations taken in November, 2015, Charon dark side lit by Pluto-shine, and several other observations. The lossy images from Version 1.0 were recalibrated, including expanding the 'bad' pixel designation of 8x8 boxes affected by the first 34 pixels of header information in the calibrated quality map. Also, updates were made to the documentation and catalog files, primarily to resolve liens from the V1.0 peer review.

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.

This data set contains Calibrated data taken by the NASA New Horizons mission's Long Range Reconnaissance Imager (LORRI) instrument during the Pluto encounter mission phase. This is Version 3.0 of this data set and contains LORRI observations taken during 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 the Trans-Neptunian Object 15810 Arawn (1994 JR1) observations. This data set completes the Pluto mission phase deliveries for LORRI. This dataset includes all data covering the Pluto Encounter and the subsequent Calibration Campaign. It includes multi-map observations from the Approach phase, observations of the moons of Pluto (Charon, Nix, Hydra, Kerberos, and Styx), high-resolution, full-frame observations from Pluto Encounter and Departure, sliver maps, and ring search observations.

This is a companion dataset to PLUTO and MapPLUTO. PLUTO and MapPLUTO are created using the best available data from a number of city agencies. To further improve data quality, the Department of City Planning (DCP) applies changes to selected field values. DCPEdited is set to "1" in PLUTO if the record contains any changed values.

All previously released versions of this data are available at BYTES of the BIG APPLE- Archive

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 2.0 of this data set. This data set contains LORRI observations taken during the the Approach (Jan-Jul, 2015) and Encounter mission sub-phases, including flyby observations taken on 14 July, 2015; the data are limited to those downlinked from the spacecraft as of the end of January, 2016. The rest of the downlinked data for this mission phase will be delivered in a future data set. Refer to the data set description above and the sequence table provided in the documentation for more detail about which observations are present in this data set. This is version 2.0 of this data set. Changes since version 1.0 include data downlinked between the end of July, 2015 and the end of January, 2016. These include Pluto Charon, Nix and Hydra observations from Approach, the day of the flyby, and Departure, lossless downlinks of images downlinked with lossy compression in version 1.0, Nix orbit determination observations, Multi-maps and VIS-UV maps taken in coordination with ALICE, High-phase and departure imaging, satellite photometry, non-critical navigation imaging, Kerberos and Styx imaging, KBO 1994 JR1 observations and departure ring-search observations taken in November, 2015, Charon dark side lit by Pluto-shine, and several other observations. The lossy images from Version 1.0 were recalibrated, including expanding the 'bad' pixel designation of 8x8 boxes affected by the first 34 pixels of header information in the calibrated quality map. Also, updates were made to the documentation and catalog files, primarily to resolve liens from the V1.0 peer review.

38226 Global exporters importers export import shipment records of Pluto with prices, volume & current Buyer's suppliers relationships based on actual Global export trade database.

This data set contains Raw data taken by the New Horizons Multispectral Visible Imaging Camera instrument during the Pluto encounter mission phase. This is VERSION 2.0 of this data set. This data set contains MVIC observations taken during the the Approach (Jan-Jul, 2015) and Encounter mission sub-phases, including flyby observations taken on 14 July, 2015. This is version 2.0 of this data set. Version 1.0 included data downlinked between the end of July, 2015 through the end of October 2015. Changes since version 1.0 include additional data downlinked between October, 2015 and the end of January, 2016. These observations include Charon, Nix and Hydra observations from the day of encounter, Pluto and Charon Multi-maps and Multi-longitudes from Approach, full-frame versions of observations downlinked as sub-framed (windowed) versions for version 1.0, Kerberos and Styx observations, Pluto High-phase and Color observations, and departure Ring-search observations taken in November, 2015. Also, updates were made to the documentation and catalog files, primarily to resolve liens from the V1.0 peer review.

This data set contains Calibrated data taken by the New Horizons Multispectral Visible Imaging Camera instrument during the Pluto encounter mission phase. This is VERSION 2.0 of this data set. This data set contains MVIC observations taken during the the Approach (Jan-Jul, 2015) and Encounter mission sub-phases, including flyby observations taken on 14 July, 2015. This is version 2.0 of this data set. Version 1.0 included data downlinked between the end of July, 2015 through the end of October 2015. Changes since version 1.0 include additional data downlinked between October, 2015 and the end of January, 2016. These observations include Charon, Nix and Hydra observations from the day of encounter, Pluto and Charon Multi-maps and Multi-longitudes from Approach, full-frame versions of observations downlinked as sub-framed (windowed) versions for version 1.0, Kerberos and Styx observations, Pluto High-phase and Color observations, and departure Ring-search observations taken in November, 2015. Also, updates were made to the documentation and catalog files, primarily to resolve liens from the V1.0 peer review.

This data set contains Calibrated data taken by the New Horizons Multispectral Visible Imaging Camera instrument during the Pluto encounter mission phase. This is VERSION 3.0 of this data set. This data set contains MVIC 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. This data set completes the Pluto mission phase deliveries for MVIC. It includes multi- map observations from the Approach phase, observations of the moons, hires, full-frame observations from Pluto Encounter and Departure, and ring search observations. This dataset also includes functional tests from the Calibration Campaign, including calibration observations of the M6 and M7 clusters, and HD205905.

GIS shapefile of extensive land use and geographic data at the tax lot level. The PLUTO files contain more than seventy fields derived from data maintained by city agencies. Essentially, displays a plethora of plot data including size, tax lot, and other publicly available information. MapPLUTO merges PLUTO tax lot data with tax lot features from the Department of Finance’s Digital Tax Map (DTM), clipped to the shoreline. It contains extensive land use and geographic data at the tax lot level in ESRI shape file format and dbase table format.

This data set contains Raw data taken by the New Horizons Linear Etalon Imaging Spectral Array instrument during the Pluto encounter mission phase. This is VERSION 2.0 of this data set. This data set contains LEISA observations taken during the the Approach (Jan-Jul, 2015) and Encounter mission sub-phases, including flyby observations taken on 14.July, 2015; the data are limited to those downlinked from the spacecraft as of the end of January, 2016. The rest of the downlinked data for this mission phase will be delivered in a future data set. Refer to the data set description above and the sequence table provided in the documentation for more detail about which observations are present in this data set. This is version 2.0 of this data set. Changes since version 1.0 include data downlinked between the end of July, 2015 and the end of January, 2016. These include Pluto observations around the time of the flyby, the Charon hi-resolution observations and co-observations with LORRI, Multi-map observations on 02.July, and Multi departure longitude observations. Also, updates were made to the documentation and catalog files, primarily to resolve liens from the V1.0 peer review.