I am trying to identify galxies hosting ANG. What is the best way to do it?
I was checking the data specifications but couldn't find any label (like "subhalo hosts AGN") in the groups catalogue.
Does it make sense to use the "GFM_AGNRadiation " column (from the PartType0 snapshot), and check wether it has a positive value?
No the GFM_AGNRadiation is a bit tangential, it would be better to use the accretion rate onto the black hole itself.
You're right this isn't stored "per subhalo", so for a given subhalo you have to actually load its black hole particle. This isn't such a trouble though, since there are so few black hole particles in the entire simulation.
Once you've loaded the BHs, you can use the BH_Mdot to convert to a bolometric luminosity using a simple model like Eqn. 5 of Nelson+ (2019).
Note this is very simple, it neglects things like obscuration effects, short duty cycles, specific observational details like energy bandpasses. If you are comparing to observations, you may want to think carefully about these and what might need to be done to produce an "observationally realistic AGN criterion" from the accretion rate (or accretion rate history).
Thank you, Dylan,
I think your suggestion will be enough for my purposes (I just need a binary output). I will try it and come back to you if I need more feedback ;)