2 datasets found
  1. Sloan Digital Sky Survey DR16

    • kaggle.com
    zip
    Updated Dec 30, 2019
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    Mukharbek Organokov (2019). Sloan Digital Sky Survey DR16 [Dataset]. https://www.kaggle.com/muhakabartay/sloan-digital-sky-survey-dr16
    Explore at:
    zip(6728394 bytes)Available download formats
    Dataset updated
    Dec 30, 2019
    Authors
    Mukharbek Organokov
    License

    Attribution-ShareAlike 4.0 (CC BY-SA 4.0)https://creativecommons.org/licenses/by-sa/4.0/
    License information was derived automatically

    Description

    Feedback: Mukharbek Organokov organokov.m@gmail.com

    Context

    Sloan Digital Sky Survey current DR16 Server Data release with Galaxies, Stars and Quasars.

    License: Creative Commons Attribution license (CC-BY) More datailes here. Find more here.

    Content

    The table results from a query which joins two tables:
    - "PhotoObj" which contains photometric data
    - "SpecObj" which contains spectral data.

    16 variables (double) and 1 additional variable (char) 'class'. A class object can be predicted from the other 16 variables.

    Variables description:
    objid = Object Identifier
    ra = J2000 Right Ascension (r-band)
    dec = J2000 Declination (r-band)
    u = better of deV/Exp magnitude fit (u-band)
    g = better of deV/Exp magnitude fit (g-band)
    r = better of deV/Exp magnitude fit (r-band)
    i = better of deV/Exp magnitude fit (i-band)
    z = better of deV/Exp magnitude fit (z-band)
    run = Run Number
    rerun = Rerun Number
    camcol = Camera column
    field = Field number
    specobjid = Object Identifier
    class = object class (galaxy, star or quasar object)
    redshift = Final Redshift
    plate = plate number
    mjd = MJD of observation
    fiberid = fiberID

    Comments

    • A four-color UVGR intermediate-band photometric system (Thuan-Gunn astronomic magnitude system) is discussed in [1]. The Sloan Digital Sky Survey (SDSS) photometric system, a new five-color (u′ g′ r′ i′ z′) wide-band CCD system is described in [2]
    • The variables 'run', 'rerun', 'camcol' and 'field' features which describe a field within an image taken by the SDSS. A field is basically a part of the entire image corresponding to 2048 by 1489 pixels. A field can be identified by: - run number, which identifies the specific scan, - the camera column, or "camcol," a number from 1 to 6, identifying the scanline within the run, and the field number. The field number typically starts at 11 (after an initial rampup time), and can be as large as 800 for particularly long runs. - An additional number, rerun, specifies how the image was processed.
    • The variable 'class' identifies an object to be either a galaxy (GALAXY), star (STAR) or quasar (QSO).
      ####References:
      [1] Thuan & Gunn (1976, PASP, 88,543)
      [2] Fukugita, M. et al, Astronomical J. v.111, p.1748

    Data server

    Data can be obtained using SkyServer SQL Search with the command below:
    -- This query does a table JOIN between the imaging (PhotoObj) and spectra
    -- (SpecObj) tables and includes the necessary columns in the SELECT to upload
    -- the results to the SAS (Science Archive Server) for FITS file retrieval.
    SELECT TOP 100000
    p.objid,p.ra,p.dec,p.u,p.g,p.r,p.i,p.z,
    p.run, p.rerun, p.camcol, p.field,
    s.specobjid, s.class, s.z as redshift,
    s.plate, s.mjd, s.fiberid
    FROM PhotoObj AS p
    JOIN SpecObj AS s ON s.bestobjid = p.objid
    WHERE
    p.u BETWEEN 0 AND 19.6
    AND g BETWEEN 0 AND 20

    Learn how to. Some examples. Full SQL Tutorial.

    Or perform a complicated, CPU-intensive query of SDSS catalog data using CasJobs, SQL-based interface to the CAS.

    Acknowledgements

    SDSS collaboration.

    Inspiration

    The Sloan Digital Sky Survey has created the most detailed three-dimensional maps of the Universe ever made, with deep multi-color images of one-third of the sky, and spectra for more than three million astronomical objects. It allows to learn and explore all phases and surveys - past, present, and future - of the SDSS.

  2. e

    Merger of BNV-D data (2008 to 2019) and enrichment

    • data.europa.eu
    zip
    Updated Jan 16, 2025
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    Patrick VINCOURT (2025). Merger of BNV-D data (2008 to 2019) and enrichment [Dataset]. https://data.europa.eu/data/datasets/5f1c3eca9d149439e50c740f?locale=en
    Explore at:
    zip(18530465)Available download formats
    Dataset updated
    Jan 16, 2025
    Dataset authored and provided by
    Patrick VINCOURT
    Description

    Merging (in Table R) data published on https://www.data.gouv.fr/fr/datasets/ventes-de-pesticides-par-departement/, and joining two other sources of information associated with MAs: — uses: https://www.data.gouv.fr/fr/datasets/usages-des-produits-phytosanitaires/ — information on the “Biocontrol” status of the product, from document DGAL/SDQSPV/2020-784 published on 18/12/2020 at https://agriculture.gouv.fr/quest-ce-que-le-biocontrole

    All the initial files (.csv transformed into.txt), the R code used to merge data and different output files are collected in a zip. enter image description here NB: 1) “YASCUB” for {year,AMM,Substance_active,Classification,Usage,Statut_“BioConttrol”}, substances not on the DGAL/SDQSPV list being coded NA. 2) The file of biocontrol products shall be cleaned from the duplicates generated by the marketing authorisations leading to several trade names.
    3) The BNVD_BioC_DY3 table and the output file BNVD_BioC_DY3.txt contain the fields {Code_Region,Region,Dept,Code_Dept,Anne,Usage,Classification,Type_BioC,Quantite_substance)}

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Share
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Click to copy link
Link copied
Close
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Mukharbek Organokov (2019). Sloan Digital Sky Survey DR16 [Dataset]. https://www.kaggle.com/muhakabartay/sloan-digital-sky-survey-dr16
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Sloan Digital Sky Survey DR16

Sloan Digital Sky Survey DR16 Server Data with Galaxies, Stars and Quasars

Explore at:
51 scholarly articles cite this dataset (View in Google Scholar)
zip(6728394 bytes)Available download formats
Dataset updated
Dec 30, 2019
Authors
Mukharbek Organokov
License

Attribution-ShareAlike 4.0 (CC BY-SA 4.0)https://creativecommons.org/licenses/by-sa/4.0/
License information was derived automatically

Description

Feedback: Mukharbek Organokov organokov.m@gmail.com

Context

Sloan Digital Sky Survey current DR16 Server Data release with Galaxies, Stars and Quasars.

License: Creative Commons Attribution license (CC-BY) More datailes here. Find more here.

Content

The table results from a query which joins two tables:
- "PhotoObj" which contains photometric data
- "SpecObj" which contains spectral data.

16 variables (double) and 1 additional variable (char) 'class'. A class object can be predicted from the other 16 variables.

Variables description:
objid = Object Identifier
ra = J2000 Right Ascension (r-band)
dec = J2000 Declination (r-band)
u = better of deV/Exp magnitude fit (u-band)
g = better of deV/Exp magnitude fit (g-band)
r = better of deV/Exp magnitude fit (r-band)
i = better of deV/Exp magnitude fit (i-band)
z = better of deV/Exp magnitude fit (z-band)
run = Run Number
rerun = Rerun Number
camcol = Camera column
field = Field number
specobjid = Object Identifier
class = object class (galaxy, star or quasar object)
redshift = Final Redshift
plate = plate number
mjd = MJD of observation
fiberid = fiberID

Comments

  • A four-color UVGR intermediate-band photometric system (Thuan-Gunn astronomic magnitude system) is discussed in [1]. The Sloan Digital Sky Survey (SDSS) photometric system, a new five-color (u′ g′ r′ i′ z′) wide-band CCD system is described in [2]
  • The variables 'run', 'rerun', 'camcol' and 'field' features which describe a field within an image taken by the SDSS. A field is basically a part of the entire image corresponding to 2048 by 1489 pixels. A field can be identified by: - run number, which identifies the specific scan, - the camera column, or "camcol," a number from 1 to 6, identifying the scanline within the run, and the field number. The field number typically starts at 11 (after an initial rampup time), and can be as large as 800 for particularly long runs. - An additional number, rerun, specifies how the image was processed.
  • The variable 'class' identifies an object to be either a galaxy (GALAXY), star (STAR) or quasar (QSO).
    ####References:
    [1] Thuan & Gunn (1976, PASP, 88,543)
    [2] Fukugita, M. et al, Astronomical J. v.111, p.1748

Data server

Data can be obtained using SkyServer SQL Search with the command below:
-- This query does a table JOIN between the imaging (PhotoObj) and spectra
-- (SpecObj) tables and includes the necessary columns in the SELECT to upload
-- the results to the SAS (Science Archive Server) for FITS file retrieval.
SELECT TOP 100000
p.objid,p.ra,p.dec,p.u,p.g,p.r,p.i,p.z,
p.run, p.rerun, p.camcol, p.field,
s.specobjid, s.class, s.z as redshift,
s.plate, s.mjd, s.fiberid
FROM PhotoObj AS p
JOIN SpecObj AS s ON s.bestobjid = p.objid
WHERE
p.u BETWEEN 0 AND 19.6
AND g BETWEEN 0 AND 20

Learn how to. Some examples. Full SQL Tutorial.

Or perform a complicated, CPU-intensive query of SDSS catalog data using CasJobs, SQL-based interface to the CAS.

Acknowledgements

SDSS collaboration.

Inspiration

The Sloan Digital Sky Survey has created the most detailed three-dimensional maps of the Universe ever made, with deep multi-color images of one-third of the sky, and spectra for more than three million astronomical objects. It allows to learn and explore all phases and surveys - past, present, and future - of the SDSS.

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