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SAG, SAGE and Galacticus semi-analytic galaxies with emission line properties
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If you use these catalogues, please cite Favole et al. 2020, https://arxiv.org/pdf/1908.05626.pdf

For questions, bugs, queries --> ginevra.favole@port.ac.uk

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Emission lines provided:

LOII (erg s^-1) --> [OII] doublet 3727+3729 A
LOIII (erg s^-1) --> [OIII] 5007 A
LHa (erg s^-1) --> Halpha 6563 A
LHb (erg s^-1) --> Hbeta 4861 A

these are computed using the GET_EMLINES code (Orsi et al. 2014) based on the galaxy SFR and 
metallicity. SAG provides both instantaneous ("inst" in what follows) and average SFRs, while 
SAGE and Galacticus only have average values.

These catalogues satisfy the following minimal cuts (see Favole et al. 2020):

Mstar > 10^8.87 Msun
SFR > 0 yr^-1
fluxOII > 5*10^-18 erg cm^-2 s^-1

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Columns specified in the header, where "att"--> dust attenuated:

SAG: 
haloID, x, y, z, SFR, SFR_inst, Mu, Mg, metallicity, LOII, LOII_inst, LOII_att, LOII_inst_att, 
LHa, LHa_inst, LHa_att, LHa_inst_att, LHb, LHb_inst, LHb_att, LHb_inst_att, LOIII, LOIII_inst, 
LOIII_att, LOIII_inst_att 



SAGE: 
haloID, x, y, z, SFR, metallicity, LOII, LOII_att, LHa, LHa_att, LHb, LHb_att, LOIII, LOIII_att


Galacticus: 
haloID, x, y, z, SFR, Mu, Mg, metallicity, LOII, LOII_att, LHa, LHa_att, LHb, LHb_att, LOIII, LOIII_att