5 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. s

    Metrical, morphosyntactic, and syntactic analysis of the Rigveda

    • swissubase.ch
    Updated Sep 22, 2025
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    (2025). Metrical, morphosyntactic, and syntactic analysis of the Rigveda [Dataset]. http://doi.org/10.48656/yc4z-sa04
    Explore at:
    Dataset updated
    Sep 22, 2025
    Description

    The dataset contains: • the main data table, RV_data.csv, with morphosyntactic, syntactic and metrical information on each Rigvedic word form, and • a script, disticha.rmd, for the analysis of disticha in the main types of Rigvedic stanzas which were studied as an example for the application of the data table, resulting in the published article: Salvatore Scarlata and Paul Widmer, Syntactic evidence for metrical structure in Rigvedic stanzas, Indo-European Linguistics 13 (2025), 1-21, doi:10.1163/22125892-bja10041, issn: 2212-5892.

    In addition the dataset contains: • a further data table, RV-polylex.csv, wherein all compounded word forms are analyzed, and • some ancillary basic scripts for linking the two tables respectively for simplified representations: join.r resp. pivot01–03.r.

    Finally, the dataset contains: • a data table, RV-polylexREJECTS.csv, containing words for which it was not possible to assess them as compounded

  3. 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)}

  4. H

    Current Population Survey (CPS)

    • dataverse.harvard.edu
    • search.dataone.org
    Updated May 30, 2013
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    Anthony Damico (2013). Current Population Survey (CPS) [Dataset]. http://doi.org/10.7910/DVN/AK4FDD
    Explore at:
    CroissantCroissant is a format for machine-learning datasets. Learn more about this at mlcommons.org/croissant.
    Dataset updated
    May 30, 2013
    Dataset provided by
    Harvard Dataverse
    Authors
    Anthony Damico
    License

    CC0 1.0 Universal Public Domain Dedicationhttps://creativecommons.org/publicdomain/zero/1.0/
    License information was derived automatically

    Description

    analyze the current population survey (cps) annual social and economic supplement (asec) with r the annual march cps-asec has been supplying the statistics for the census bureau's report on income, poverty, and health insurance coverage since 1948. wow. the us census bureau and the bureau of labor statistics ( bls) tag-team on this one. until the american community survey (acs) hit the scene in the early aughts (2000s), the current population survey had the largest sample size of all the annual general demographic data sets outside of the decennial census - about two hundred thousand respondents. this provides enough sample to conduct state- and a few large metro area-level analyses. your sample size will vanish if you start investigating subgroups b y state - consider pooling multiple years. county-level is a no-no. despite the american community survey's larger size, the cps-asec contains many more variables related to employment, sources of income, and insurance - and can be trended back to harry truman's presidency. aside from questions specifically asked about an annual experience (like income), many of the questions in this march data set should be t reated as point-in-time statistics. cps-asec generalizes to the united states non-institutional, non-active duty military population. the national bureau of economic research (nber) provides sas, spss, and stata importation scripts to create a rectangular file (rectangular data means only person-level records; household- and family-level information gets attached to each person). to import these files into r, the parse.SAScii function uses nber's sas code to determine how to import the fixed-width file, then RSQLite to put everything into a schnazzy database. you can try reading through the nber march 2012 sas importation code yourself, but it's a bit of a proc freak show. this new github repository contains three scripts: 2005-2012 asec - download all microdata.R down load the fixed-width file containing household, family, and person records import by separating this file into three tables, then merge 'em together at the person-level download the fixed-width file containing the person-level replicate weights merge the rectangular person-level file with the replicate weights, then store it in a sql database create a new variable - one - in the data table 2012 asec - analysis examples.R connect to the sql database created by the 'download all microdata' progr am create the complex sample survey object, using the replicate weights perform a boatload of analysis examples replicate census estimates - 2011.R connect to the sql database created by the 'download all microdata' program create the complex sample survey object, using the replicate weights match the sas output shown in the png file below 2011 asec replicate weight sas output.png statistic and standard error generated from the replicate-weighted example sas script contained in this census-provided person replicate weights usage instructions document. click here to view these three scripts for more detail about the current population survey - annual social and economic supplement (cps-asec), visit: the census bureau's current population survey page the bureau of labor statistics' current population survey page the current population survey's wikipedia article notes: interviews are conducted in march about experiences during the previous year. the file labeled 2012 includes information (income, work experience, health insurance) pertaining to 2011. when you use the current populat ion survey to talk about america, subract a year from the data file name. as of the 2010 file (the interview focusing on america during 2009), the cps-asec contains exciting new medical out-of-pocket spending variables most useful for supplemental (medical spending-adjusted) poverty research. confidential to sas, spss, stata, sudaan users: why are you still rubbing two sticks together after we've invented the butane lighter? time to transition to r. :D

  5. h

    Table 2

    • hepdata.net
    Updated Oct 25, 2017
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    (2017). Table 2 [Dataset]. http://doi.org/10.17182/hepdata.78697.v2/t2
    Explore at:
    Dataset updated
    Oct 25, 2017
    Description

    Vertex reconstruction efficiency as a function of radial position $R$ for two $R$-hadron signal samples with $m_{\tilde{g}} = 1.2$ TeV,...

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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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