The content and description of each column of LAMOST full quasar catalog are nearly the same as in Ai et al. (2016); Dong et al. (2018) and Yao et al. (2019), and is also provided below. Since the LAMOST quasar catalogs are published seperately, the values in some columns in one catalog may be unavailable in others. The value is set to in this case, unless mentioned otherwise.
Column Name | Data Format | Description |
---|---|---|
ObsID | Integer | Unique Spectra ID |
Designation | String | LAMOST designation hhmmss.ss+ddmmss (J2000) |
RA | Double | Right ascension in decimal degrees (J2000) |
Dec | Double | Declination in decimal degrees (J2000) |
MJD | Long | Modified Julian Day of observation |
planID | String | Spectroscopic plan name |
spID | Long | Spectrograph identification |
fiberID | Long | Spectroscopic fiber number |
z_vi | Double | Redshift by visual inspection |
zWarning | Integer | Flag of redshift from visual inspection. 1 = not robust. |
Mi_z2 | Double | Absolute -band magnitude. 2006) | -corrected to following Richards et al. (
NspecOBS | Integer | Number of spectroscopic observations for the quasar. When there are more than one observation for the object, the line properties are obtained from only one of the observations in which the fiber pointing position is nearest to the position in the input quasar candidate catalog |
SNR_spec | Double | Median S/N per pixel in the wavelength regions of [4000-5700]Å and [6200, 9000]Å. |
BAL_flag | Integer | Flag of broad absorption features. BAL_FLAG=1 indicates broad absorption features are present. |
FWHM_BROAD_HA | Double | FWHM of broad H in units of km/s |
EW_BROAD_HA | Double | Equivalent width of broad H in units of Å |
FWHM_NARROW_HA | Double | FWHM of narrow H in units of km/s |
EW_NARROW_HA | Double | Equivalent width of broad H in units of Å |
EW_NII_6585 | Double | equivalent width of [NII]6563 in units of Å |
EW_SII_6718 | Double | equivalent width of [SII]6718 in units of Å |
EW_SII_6732 | Double | equivalent width of [SII]6732 in units of Å |
EW_FE_HA | Double | Rest-frame equivalent width of iron emissions in 6000-6500 Å |
LINE_NPIX_HA | Long | Number of good pixels for the spectrum in region of rest-frame 6400-6765 Å |
LINE_MED_SN_HA | Double | Median S/N per pixel for the spectrum in region of rest-frame 6400-6765 Å |
LINE_FLAG_HA | Integer | Flag indicates reliability of the emission line fitting results in H region upon visual inspections. 0=reliable; -1=unreliable. This value is set to be −9999 if H is not measured due to lack of good pixels in the fitting wavelength region. |
FWHM_BROAD_HB | Double | FWHM of broad H in units of km/s |
EW_BROAD_HB | Double | Equivalent width of broad H in units of Å |
FWHM_NARROW_HB | Double | FWHM of narrow H in units of km/s |
EW_NARROW_HB | Double | Equivalent width of narrow H in units of Å |
FWHM_OIII_5007 | Double | FWHM of [OIII]5007 in units of km/s |
EW_OIII_5007 | Double | Equivalent width of [OIII]5007 in units of Å |
EW_FE_HB | Double | Rest-frame equivalent width of iron emissions in 4685-4435 Å |
LINE_NPIX_HB | Long | Number of good pixels for the spectrum in region of rest-frame 4750-4950 Å. |
LINE_MED_SN_HB | Double | Median S/N per pixel for the spectrum in region of rest-frame 4750-4950 Å. |
LINE_FLAG_HB | Integer | Flag indicates reliability of the emission line fitting results in H region upon visual inspections. 0=reliable; -1=unreliable. This value is set to be −9999 if H is not measured due to lack of good pixels in the fitting wavelength region. |
FWHM_MGII | Double | FWHM of the total MgII emission line in units of km/s |
EW_MGII | Double | Equivalent width of the total MgII emission line in units of Å |
FWHM_BROAD_MGII | Double | FWHM of the total broad MgII emission line in units of km/s |
EW_BROAD_MGII | Double | Equivalent width of the total broad MgII emission line in units of Å |
FWHM_BROAD_MGII_2796 | Double | FWHM of the broad MgII2796 emission line in units of km/s. |
FWHM_NARROW_MGII_2796 | Double | FWHM of the narrow MgII2796 emission line in units of km/s. |
EW_FE_MGII | Double | Rest-frame equivalent width of iron emissions in 2200-3090 Å. |
LINE_NPIX_MGII | Long | Number of good pixels for the spectrum in region of rest-frame 2700-2900 Å. |
LINE_MED_SN_MGII | Double | Median S/N per pixel for the spectrum in region of rest-frame 2700-2900 Å. |
LINE_FLAG_MGII | Integer | Flag indicates reliability of the emission line fitting results in MgII region upon visual inspections. 0=reliable; -1=unreliable. This value is set to be −9999 if MgII is not measured due to lack of good pixels in the fitting wavelength region. |
FWHM_CIV | Double | FWHM of the total CIV emission line in units of km/s. |
EW_CIV | Double | Equivalent width of the total CIV emission line in units of Å |
FWHM_BROAD_CIV | Double | FWHM of the broad CIV emission line in units of km/s. |
EW_BROAD_CIV | Double | Equivalent width of the broad CIV emission line in units of Å |
FWHM_NARROW_CIV | Double | FWHM of the narrow CIV emission line in units of km/s. |
EW_NARROW_CIV | Double | Equivalent width of the narrow CIV emission line in units of Å |
LINE_NPIX_CIV | Long | Number of good pixels for the spectrum in region of rest-frame 1500-1600 Å |
LINE_MED_SN_CIV | Double | Median S/N per pixel for the spectrum in region of rest-frame 1500-1600 Å |
LINE_FLAG_CIV | Integer | Flag indicates reliability of the emission line fitting results in C IV region upon visual inspections. 0=reliable; -1=unreliable. This value is set to be −9999 if C IV is not measured due to lack of good pixels in the fitting wavelength region. |
ALPHA_LAMBDA_1 | Double | Wavelength power-law index, , from 1300 to 4661 Å. |
ALPHA_LAMBDA_2 | Double | Wavelength power-law index, , redward of 4661 Å. |
MODEL_PHOT_REDCHI2 | Double | Reduced chi-square in SDSS photometry modeling. −9999 if not fitted. |
LOGL5100 | Double | Monochromatic luminosities at 5100 Å. |
LOGL3000 | Double | Monochromatic luminosities at 3000 Å. |
LOGL1350 | Double | Monochromatic luminosities at 1300 Å. |
LOGBH_HB | Double | Virial black hole masses (in ) based on Hβ. |
LOGBH_MGII | Double | Virial black hole masses (in ) based on MgII. |
LOGBH_CIV | Double | Virial black hole masses (in ) based on C IV. |