// This code is generated by generate_code.py, do not modify it manually.
//! This module contains all the known columns in the ravedr5_on table.
use crate::traits::{Column, Table};
/// The Radial Velocity Experiment (RAVE): fifth data release (DR5). Stellar parameters from the "Cannon". RAVE DR5 is the fifth data release from a magnitude-limited (9 < I < 12 mag) survey of stars randomly selected in the Southern Hemisphere. The RAVE medium-resolution spectra (R ~ 7500) covering the Ca-triplet region (8410-8795 Angstrom) span the complete time frame from the start of RAVE observations in 2003 to their completion in 2013. Radial velocities from 520,781 spectra of 457,588 unique stars are presented, of which 255,922 stellar observations have parallaxes and proper motions from the Tycho-Gaia astrometric solution in Gaia DR1. For the main DR5 catalogue, stellar parameters (effective temperature, surface gravity, and overall metallicity) are computed using the RAVE DR4 stellar pipeline, but calibrated using recent K2 Campaign 1 seismic gravities and Gaia benchmark stars, as well as results obtained from high-resolution studies. Also included are temperatures from the Infrared Flux Method, and a catalogue of red giant stars in the de-reddened color {(J-{Ks})}_0 interval (0.50, 0.85) for which the gravities were calibrated based only on seismology. Further data products for subsamples of the RAVE stars include individual abundances for Mg, Al, Si, Ca, Ti, Fe, and Ni, and distances found using isochrones. Each RAVE spectrum is complemented by an error spectrum, which has been used to determine uncertainties on the parameters. Data retrieved using the VizieR catalogue access tool, CDS, Strasbourg, France (VizieR catalogue: III/279). Reference paper: https://ui.adsabs.harvard.edu/abs/2017AJ....153...75K/abstract (DOI: 10.3847/1538-3881/153/2/75)
#[allow(non_camel_case_types)]
pub struct ravedr5_on;
impl Table for ravedr5_on {
fn string(&self) -> String {
"ravedr5_on".to_string()
}
}
/// The columns in the ravedr5_on table.
#[allow(non_camel_case_types)]
#[derive(Debug, Clone, Copy, PartialEq, Eq, Hash, strum::Display)]
pub enum Col {
/// ! Target designation (RAVE_OBS_ID)
name,
/// ! RAVE designation(JHHMMSS.S+DDMMSS) (RAVEID)
rave,
/// Heliocentric radial velocity (HRV)
hrv,
/// Error on HRV (eHRV)
e_hrv,
/// ? Standard deviation in HRV from 10 resampled spectra (StdDev_HRV)
s_hrv,
/// ? Median absolute deviation in HRV from 10 resampled spectra (MAD_HRV)
s_med_hrv,
/// Tonry-Davis R correlation coefficient (CorrelationCoeff)
r,
/// Height of correlation peak (PeakHeight)
hcp,
/// Width of correlation peak (PeakWidth)
wcp,
/// Zero point correction applied HRV (CorrectionRV)
crv,
/// Measured HRV of sky (SkyRV)
hrvsky,
/// Error HRV of sky (eSkyRV)
e_hrvsky,
/// Correlation Coefficient R of sky (SkyCorrelationCoeff)
rsky,
/// ? Rotational Velocity from SPARV pipeline (Vrot_SPARV)
vrots,
/// Quality Flag for ZeroPoint correction (ZeroPointFLAG) (1)
zpflag,
/// 1st minimum distance (c1) (2)
c1,
/// 2nd minimum distance (c2) (2)
c2,
/// 3rd minimum distance (c3) (2)
c3,
/// 4th minimum distance (c4) (2)
c4,
/// 5th minimum distance (c5) (2)
c5,
/// 6th minimum distance (c6) (2)
c6,
/// 7th minimum distance (c7) (2)
c7,
/// 8th minimum distance (c8) (2)
c8,
/// 9th minimum distance (c9) (2)
c9,
/// 10th minimum distance (c10) (2)
c10,
/// 11th minimum distance (c11) (2)
c11,
/// 12th minimum distance (c12) (2)
c12,
/// 13th minimum distance (c13) (2)
c13,
/// 14th minimum distance (c14) (2)
c14,
/// 15th minimum distance (c15) (2)
c15,
/// 16th minimum distance (c16) (2)
c16,
/// 17th minimum distance (c17) (2)
c17,
/// 18th minimum distance (c18) (2)
c18,
/// 19th minimum distance (c19) (2)
c19,
/// 20th minimum distance (c20) (2)
c20,
/// ? Effective temperature (TEFF) (3)
teff,
/// ? Log gravity (LOGG) (3)
logg,
/// ? Abundance of Fe (FE_H) (3)
fe_h,
/// ? Abundance of O (O_H) (3)
o_h,
/// ? Abundance of Mg (MG_H) (3)
mg_h,
/// ? Abundance of Al (AL_H) (3)
al_h,
/// ? Abundance of Si (SI_H) (3)
si_h,
/// ? Abundance of Ca (CA_H) (3)
ca_h,
/// ? Abundance of Ni (NI_H) (3)
ni_h,
/// ? Error on effective temperature (e_TEFF) (3)
e_teff,
/// ? Error on log gravity (E_LOGG) (3)
e_logg,
/// ? Error on [Fe/H] (E_FE_H) (3)
e_fe_h,
/// ? Error on [O/H] (E_O_H) (3)
e_o_h,
/// ? Error on [Mg/H] (E_MG_H) (3)
e_mg_h,
/// ? Error on [Al/H] (E_AL_H) (3)
e_al_h,
/// ? Error on [Si/H] (E_SI_H) (3)
e_si_h,
/// ? Error on [Ca/H] (E_CA_H) (3)
e_ca_h,
/// ? Error on [Ni/H] (E_NI_H) (3)
e_ni_h,
/// ? Signal to noise ratio (SNR) (3)
snr,
/// ? Chi-square (R_CHI_SQ) (3)
rchisq,
/// Quality flag (QC) (3)
qc,
/// Right ascension (J2000.0, Ep=J2000) (RAdeg)
ra,
/// Declination (J2000.0, Ep=J2000) (DEdeg)
dec,
}
impl Column for Col {}
#[cfg(test)]
/// Collects all the known columns in the ravedr5_on table.
pub fn collect_known(map: &mut std::collections::HashMap<String, Vec<String>>) {
let mut col_strings = Vec::new();
col_strings.push(Col::name.to_string());
col_strings.push(Col::rave.to_string());
col_strings.push(Col::hrv.to_string());
col_strings.push(Col::e_hrv.to_string());
col_strings.push(Col::s_hrv.to_string());
col_strings.push(Col::s_med_hrv.to_string());
col_strings.push(Col::r.to_string());
col_strings.push(Col::hcp.to_string());
col_strings.push(Col::wcp.to_string());
col_strings.push(Col::crv.to_string());
col_strings.push(Col::hrvsky.to_string());
col_strings.push(Col::e_hrvsky.to_string());
col_strings.push(Col::rsky.to_string());
col_strings.push(Col::vrots.to_string());
col_strings.push(Col::zpflag.to_string());
col_strings.push(Col::c1.to_string());
col_strings.push(Col::c2.to_string());
col_strings.push(Col::c3.to_string());
col_strings.push(Col::c4.to_string());
col_strings.push(Col::c5.to_string());
col_strings.push(Col::c6.to_string());
col_strings.push(Col::c7.to_string());
col_strings.push(Col::c8.to_string());
col_strings.push(Col::c9.to_string());
col_strings.push(Col::c10.to_string());
col_strings.push(Col::c11.to_string());
col_strings.push(Col::c12.to_string());
col_strings.push(Col::c13.to_string());
col_strings.push(Col::c14.to_string());
col_strings.push(Col::c15.to_string());
col_strings.push(Col::c16.to_string());
col_strings.push(Col::c17.to_string());
col_strings.push(Col::c18.to_string());
col_strings.push(Col::c19.to_string());
col_strings.push(Col::c20.to_string());
col_strings.push(Col::teff.to_string());
col_strings.push(Col::logg.to_string());
col_strings.push(Col::fe_h.to_string());
col_strings.push(Col::o_h.to_string());
col_strings.push(Col::mg_h.to_string());
col_strings.push(Col::al_h.to_string());
col_strings.push(Col::si_h.to_string());
col_strings.push(Col::ca_h.to_string());
col_strings.push(Col::ni_h.to_string());
col_strings.push(Col::e_teff.to_string());
col_strings.push(Col::e_logg.to_string());
col_strings.push(Col::e_fe_h.to_string());
col_strings.push(Col::e_o_h.to_string());
col_strings.push(Col::e_mg_h.to_string());
col_strings.push(Col::e_al_h.to_string());
col_strings.push(Col::e_si_h.to_string());
col_strings.push(Col::e_ca_h.to_string());
col_strings.push(Col::e_ni_h.to_string());
col_strings.push(Col::snr.to_string());
col_strings.push(Col::rchisq.to_string());
col_strings.push(Col::qc.to_string());
col_strings.push(Col::ra.to_string());
col_strings.push(Col::dec.to_string());
map.insert(ravedr5_on.string(), col_strings);
}