2020_boogaard_line_data_readme.txt
----------------------------------
VERSION: 2020/09/21

This table contains the spectral line information for CO and [CI] from the ALMA
Spectroscopic Survey in the Hubble Ultra Deep Field Large Program.  These data
are obtained by simultaneous Gaussian fits of all observed transitions of a
specific source in aperture matched spectra from ASPECS-LP and VLASPECS
([R20]), as reported in [B20], Table 6.  Note values in this table may differ
from the line fluxes derived by [GL19], as discussed in [B20].

When using information from this table, please cite:

- [B20] Boogaard et al., 2020, ApJ, in press; https://arxiv.org/abs/2009.04348

Additional references
- [R20] Riechers et al., 2020, ApJ, 896, L21


If a specific transition was not covered by ASPECS or VLASPECS, values equal to
nan are reported.

For more information, please contact Leindert Boogaard [boogaard@strw.leidenuniv.nl]


Description of columns
----------------------

ID_1mm			Short ASPECS 1mm continuum ID [GL20] (blank values are indicated by -1)
ID_3mm			Short ASPECS 3mm line search ID [GL19] (blank values are indicated by -1)
ID_9mm			Short VLASPECS 9mm ID [R20] (blank values are indicated by -1)
z			Redshift
z_err			Redshift error
fwhm			Full width at half maximum [km s-1]
fwhm_err		Full withh at half maximum error [km s-1]
XX_Y_Z_freq		Frequency for transition XX(Y-Z) from species XX [GHz]
XX_Y_Z_freq_err		Frequency error for transition XX(Y-Z) from species XX [GHz]
XX_Y_Z_Sdv		Line flux for transition XX(Y-Z) from species XX [mJy km s-1]
XX_Y_Z_Sdv_err		Line flux error for transition XX(Y-Z) from species XX [mJy km s-1]
XX_Y_Z_Lprime		Line luminosity for transition XX(Y-Z) from species XX [K km s-1 pc2]
XX_Y_Z_Lprime_err	Line luminosity for transition XX(Y-Z) from species XX [K km s-1 pc2]