2020_band6_dust_selected_sample_faint_readme.txt
------------------------------------------------
VERSION: 2020/09/21

This table contains the properties of the Faint 1.2 mm dust continuum selected
sample from the ALMA Spectroscopic Survey of the Hubble Ultra Deep Field Large
Program.

When using information from this table, please cite:

- [A20] Aravena et al., 2020, ApJ, in press; https://arxiv.org/abs/2006.04284
- [GL20] Gonzalez-Lopez et al. 2020, ApJ, in press; https://arxiv.org/abs/2002.07199
- [B20] Boogaard et al., 2020, ApJ, in press; https://arxiv.org/abs/2009.04348

Magphys quantities are provided with symmetric errors, folding an additional
0.1 dex (following [A20] and [B20]).  To be precise, for quantity Q (where Q is
Mstar, SFR, etc.), with Q_xx being the xxth percentile:

  Q  = Q_50
  dQ =  sqrt((0.5 * (Q_84 - Q_16))**2 + 0.1**2)


Sources without a counterpart have their values indicated by nan.

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


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

ID_1mm				Short ASPECS 1mm ID
ID_3mm				Short ASPECS 3mm ID (blank values are indicated by -1)
ID_LONG				Long ASPECS 1mm ID (ASPECS-LP-Faint.1mm.CXX; XX=1-26)
RA				Right Ascension (J2000)
DEC				Right Ascension (J2000)
fnu_1mm				1.2 mm continuum flux [uJy]
efnu_1mm			1.2 mm continuum flux [uJy]
fnu_3mm				3.0 mm continuum flux [uJy] (when 0.0, efnu_3mm denotes a 5 sigma upper limit)
efnu_3mm			3.0 mm continuum flux [uJy]
z_best				Redshift
lgMstar				Stellar mass from Magphys [log Msun]
dlgMstar			Stellar mass error from Magphys [log Msun]
lgSFR				Star formation rate from Magphys [log Msun yr-1]
dlgSFR				Star formation rate error from Magphys [log Msun yr-1]
lgLdust				Infrared Luminosity from Magphys [log Ldust]
dlgLdust			Infrared Luminosity error from Magphys [log Ldust]
lgMmol_SED			Molecular gas mass from Magphys assuming a gas-to-dust of 200 (see [A20]) [log Msun]
dlgMmol_SED			Molecular gas mass error from Magphys assuming a gas-to-dust of 200 (see [A20]) [log Msun]
lgMmol_RJ			Molecular gas mass from the 1.2 mm dust continuum (see [A20] or [B20]) [log Msun]
dlgMmol_RJ			Molecular gas mass error from the 1.2 mm dust continuum (see [A20] or [B20]) [log Msun]