gaia_access 0.1.1

Access the Gaia ESA Archive for astronomical data.
Documentation 
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// This code is generated by generate_code.py, do not modify it manually.

//! This module contains all the known columns in the sdssdr9_original_valid table.

use crate::traits::{Column, Table};

/// SDSS DR9 Catalogue, primary object only, extracted from photoObj fits
/// files.  
/// Reference paper: Ahn et al. 2012, ApJS 203,21  
/// Original catalogue: http://data.sdss3.org/sas/dr9/boss/photoObj/
/// Catalogue curator:
/// SSDC - ASI Space Science Data Center
/// https://www.ssdc.asi.it/
#[allow(non_camel_case_types)]
pub struct sdssdr9_original_valid;

impl Table for sdssdr9_original_valid {
    fn string(&self) -> String {
        "sdssdr9_original_valid".to_string()
    }
}

/// The columns in the sdssdr9_original_valid table.
#[allow(non_camel_case_types)]
#[derive(Debug, Clone, Copy, PartialEq, Eq, Hash, strum::Display)]
pub enum Col {
    /// Incremental unique numeric identifier (increasing with declination).
    /// This is the only field which was not in the original SDSS DR9 catalogue,
    /// but was added for cross-match purposes.
    sdssdr9_oid,
    /// A number identifying an object in the image catalog for DR9. It is a
    /// bit-encoded integer of run, rerun, camcol, field, object.  
    /// The bits are assigned in objid as follows:
    ///
    /// -   63 0, unassigned
    ///
    /// -   59-62 skyVersion resolved sky version
    ///
    /// -   48-58 rerun, number of pipeline rerun
    ///
    /// -   32-47 run, run number
    ///
    /// -   29-31 camcol, camera column (1-6)
    ///
    /// -   28 0, unassigned
    ///
    /// -   16-27 field, field number within run
    ///
    /// -   0-15 id, object number within field
    obj_id,
    /// Each unique source in the SDSS catalog is identified by the thingId.
    /// Each source may have been observed more than once in multiple runs, and
    /// might therefore have multiple detections listed in the catalog. Only one
    /// detection is considered primary.
    thing_id,
    /// J2000 Right Ascension (from r-band, or best other band if r-band if too
    /// faint or saturated in r).
    ra,
    /// J2000 Declination (from r-band, or best other band if r-band if too
    /// faint or saturated in r).
    dec,
    /// Error in RA*cos(DEC)
    ra_error,
    /// Error in DEC.
    dec_error,
    /// Modified Julian Date, used to indicate the date that a given piece of
    /// SDSS data (image or spectrum) was taken.
    mjd,
    /// For isolated stars, which are well-described by the point spread
    /// function (PSF), the optimal measure of the total flux is determined by
    /// fitting a PSF model to the object.
    u_mag,
    /// PSF magnitude error.
    u_mag_error,
    /// For isolated stars, which are well-described by the point spread
    /// function (PSF), the optimal measure of the total flux is determined by
    /// fitting a PSF model to the object.
    g_mag,
    /// PSF magnitude error.
    g_mag_error,
    /// For isolated stars, which are well-described by the point spread
    /// function (PSF), the optimal measure of the total flux is determined by
    /// fitting a PSF model to the object.
    r_mag,
    /// PSF magnitude error.
    r_mag_error,
    /// For isolated stars, which are well-described by the point spread
    /// function (PSF), the optimal measure of the total flux is determined by
    /// fitting a PSF model to the object.
    i_mag,
    /// PSF magnitude error.
    i_mag_error,
    /// For isolated stars, which are well-described by the point spread
    /// function (PSF), the optimal measure of the total flux is determined by
    /// fitting a PSF model to the object.
    z_mag,
    /// PSF magnitude error.
    z_mag_error,
    /// Distinguishes stars (type=6) and galaxies (type=3) based on their
    /// morphology. It is quantified on the basis of the difference between the
    /// PSF and model magnitudes.
    objc_type,
    /// Clean photometry flag for point sources (1=clean, 0=unclean).
    clean_flag,
}

impl Column for Col {}

#[cfg(test)]
pub fn collect_known(map: &mut std::collections::HashMap<String, Vec<String>>) {
    let mut col_strings = Vec::new();
    col_strings.push(Col::sdssdr9_oid.to_string());
    col_strings.push(Col::obj_id.to_string());
    col_strings.push(Col::thing_id.to_string());
    col_strings.push(Col::ra.to_string());
    col_strings.push(Col::dec.to_string());
    col_strings.push(Col::ra_error.to_string());
    col_strings.push(Col::dec_error.to_string());
    col_strings.push(Col::mjd.to_string());
    col_strings.push(Col::u_mag.to_string());
    col_strings.push(Col::u_mag_error.to_string());
    col_strings.push(Col::g_mag.to_string());
    col_strings.push(Col::g_mag_error.to_string());
    col_strings.push(Col::r_mag.to_string());
    col_strings.push(Col::r_mag_error.to_string());
    col_strings.push(Col::i_mag.to_string());
    col_strings.push(Col::i_mag_error.to_string());
    col_strings.push(Col::z_mag.to_string());
    col_strings.push(Col::z_mag_error.to_string());
    col_strings.push(Col::objc_type.to_string());
    col_strings.push(Col::clean_flag.to_string());
    map.insert(sdssdr9_original_valid.string(), col_strings);
}