gaia_access 0.2.0

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 ppmxl_original_valid table.

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

/// PPMXL Catalogue  
/// Reference papers:  
/// PPMXL: Roeser et al. 2010, AJ 139, 2440  
/// PPMX: Roeser et al. 2008,A&A 488, 401  
/// Original Catalogue:  
/// VO access: http://vo.uni-hd.de/ppmxl
/// Catalogue curator:
/// SSDC - ASI Space Science Data Center
/// https://www.ssdc.asi.it/
#[allow(non_camel_case_types)]
pub struct ppmxl_original_valid;

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

/// The columns in the ppmxl_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 field was not in the original PPMXL catalogue, but was added for
    /// cross-match purposes.
    ppmxl_oid,
    /// Identifier (Q3C ipix of the USNO-B 1.0 object)
    ipix,
    /// J2000 right ascension with respect to the ICRS, epoch 2000.0
    ra,
    /// J2000 declination with respect to the ICRS, epoch 2000.0.
    dec,
    /// Mean error in RA*cos(DEC) at mean epoch.
    ra_error_epra,
    /// Mean error in DEC at mean epoch.
    dec_error_epde,
    /// Proper motion in RA*cos(DEC).
    pmra,
    /// Proper motion in Declination.
    pmde,
    /// Mean error in proper motion in RA*cos(DEC).
    pmra_error,
    /// Mean error in proper motion in DEC.
    pmde_error,
    /// Number of catalogs (epoch) used for proper motions.  
    /// May be blank (null) for stars coming from ARIHIP or Tycho-2 via PPMX
    /// (i.e. bit#1 is set in “fl”).
    n_epochs,
    /// Mean Epoch for RA.
    epra,
    /// Mean Epoch for DEC.
    epde,
    /// B mag from USNO-B, first epoch.  
    ///
    /// Magnitudes from USNO-B should be used with care, photometric calibration
    /// may be severely off for some plates.  
    /// For objects from PPMX (bit#1 set in “fl”), these magnitudes have a
    /// special meaning:  
    /// ————————————————————  
    /// Column [PPMX] Content  
    /// ————————————————————  
    /// b1mag [Cmag] Catalogue magnitude from source  
    /// b2mag [Bmag] Johnson B magnitude  
    /// r1mag [Rmag] calculated Ru (UCAC) magnitude from source  
    /// r2mag — (always empty)  
    /// imag [Vmag] Johnson V magnitude
    b1mag,
    /// B mag from USNO-B, second epoch.  
    ///
    /// Magnitudes from USNO-B should be used with care, photometric calibration
    /// may be severely off for some plates.  
    /// For objects from PPMX (bit#1 set in “fl”), these magnitudes have a
    /// special meaning:  
    /// ————————————————————  
    /// Column [PPMX] Content  
    /// ————————————————————  
    /// b1mag [Cmag] Catalogue magnitude from source  
    /// b2mag [Bmag] Johnson B magnitude  
    /// r1mag [Rmag] calculated Ru (UCAC) magnitude from source  
    /// r2mag — (always empty)  
    /// imag [Vmag] Johnson V magnitude
    b2mag,
    /// R mag from USNO-B, first epoch.  
    ///
    /// Magnitudes from USNO-B should be used with care, photometric calibration
    /// may be severely off for some plates.  
    /// For objects from PPMX (bit#1 set in “fl”), these magnitudes have a
    /// special meaning:  
    /// ————————————————————  
    /// Column [PPMX] Content  
    /// ————————————————————  
    /// b1mag [Cmag] Catalogue magnitude from source  
    /// b2mag [Bmag] Johnson B magnitude  
    /// r1mag [Rmag] calculated Ru (UCAC) magnitude from source  
    /// r2mag — (always empty)  
    /// imag [Vmag] Johnson V magnitude
    r1mag,
    /// R mag from USNO-B, second epoch.  
    ///
    /// Magnitudes from USNO-B should be used with care, photometric calibration
    /// may be severely off for some plates.  
    /// For objects from PPMX (bit#1 set in “fl”), these magnitudes have a
    /// special meaning:  
    /// ————————————————————  
    /// Column [PPMX] Content  
    /// ————————————————————  
    /// b1mag [Cmag] Catalogue magnitude from source  
    /// b2mag [Bmag] Johnson B magnitude  
    /// r1mag [Rmag] calculated Ru (UCAC) magnitude from source  
    /// r2mag — (always empty)  
    /// imag [Vmag] Johnson V magnitude
    r2mag,
    /// I mag from USNO-B.  
    ///
    /// Magnitudes from USNO-B should be used with care, photometric calibration
    /// may be severely off for some plates.  
    /// For objects from PPMX (bit#1 set in “fl”), these magnitudes have a
    /// special meaning:  
    /// ————————————————————  
    /// Column [PPMX] Content  
    /// ————————————————————  
    /// b1mag [Cmag] Catalogue magnitude from source  
    /// b2mag [Bmag] Johnson B magnitude  
    /// r1mag [Rmag] calculated Ru (UCAC) magnitude from source  
    /// r2mag — (always empty)  
    /// imag [Vmag] Johnson V magnitude
    imag,
    /// The flag is a bitwise or number (\Sigma 2^i) where each bit number (i)
    /// has the meaning:  
    /// #0 (1) = if set, one of the coordinates had an excessively large chi
    /// square.  
    /// #1 (2) = Row is from PPMX. These objects are mostly Tycho stars that
    /// were masked out of USNO-B. When this bit is set, the USNO magnitudes
    /// (b1mag through imag) have special meanings.  
    /// #2 (4) = Row is from PPMX and replaces a single row from USNO-B. This is
    /// done when the astrometry from PPMX was better (in terms of error
    /// estimates) than the astrometry of the corresponding PPMXL object.  
    /// #3 (8) = Row replaces multiple USNO-B1.0 objects. When PPMX contains an
    /// object that has more than one counterpart in PPMXL, all such
    /// counterparts are discarded on the assumption that they should have been
    /// matched in USNO-B1.0 or result from erroneous matches. For these rows,
    /// bit#1 is always 1.
    flags,
}

impl Column for Col {}

#[cfg(test)]
/// Collects all the known columns in the ppmxl_original_valid table.
pub fn collect_known(map: &mut std::collections::HashMap<String, Vec<String>>) {
    let mut col_strings = Vec::new();
    col_strings.push(Col::ppmxl_oid.to_string());
    col_strings.push(Col::ipix.to_string());
    col_strings.push(Col::ra.to_string());
    col_strings.push(Col::dec.to_string());
    col_strings.push(Col::ra_error_epra.to_string());
    col_strings.push(Col::dec_error_epde.to_string());
    col_strings.push(Col::pmra.to_string());
    col_strings.push(Col::pmde.to_string());
    col_strings.push(Col::pmra_error.to_string());
    col_strings.push(Col::pmde_error.to_string());
    col_strings.push(Col::n_epochs.to_string());
    col_strings.push(Col::epra.to_string());
    col_strings.push(Col::epde.to_string());
    col_strings.push(Col::b1mag.to_string());
    col_strings.push(Col::b2mag.to_string());
    col_strings.push(Col::r1mag.to_string());
    col_strings.push(Col::r2mag.to_string());
    col_strings.push(Col::imag.to_string());
    col_strings.push(Col::flags.to_string());
    map.insert(ppmxl_original_valid.string(), col_strings);
}