Table 1.

Summary of the different runs used in this work. Column 1: run name; column 2: initial mass function (IMF) chosen; column 3: box size in comoving Mpc h−1; column 4: total number of particles (NTOT = NGAS + NDM); column 5: mass of the dark matter particles; column 6: initial mass of the gas particles; column 7: plummer-equivalent comoving gravitational softening length; column 8: type of feedback implemented. See Section 2.2 for more details on the parameters used for the different feedback recipes. (a) In this simulation the effect of metal-line cooling is included. (b) In this simulation we adopt variable momentum-driven galactic winds. In all the other simulations galactic winds are energy driven and the wind velocity is constant (Section 2.1).

RunIMFBox sizeNTOTMDMMGASComoving softeningFeedback
(Mpc h−1)(M h−1)(M h−1)(kpc h−1)
Kr24_eA_sWKroupa242 × 28833.64× 1077.32 × 1064.0Early AGN + Strong winds
Ch24_lA_wWChabrier242 × 28833.64× 1077.32 × 1064.0Late AGN + Weak winds
Sa24_eA_wWSalpeter242 × 28833.64× 1077.32 × 1064.0Early AGN + Weak winds
Ch24_eA_sWChabrier242 × 28833.64× 1077.32 × 1064.0Early AGN + Strong winds
Ch24_lA_sWChabrier242 × 28833.64× 1077.32 × 1064.0Late AGN + Strong winds
Ch24_eA_vsWChabrier242 × 28833.64× 1077.32 × 1064.0Early AGN + Very strong winds
Ch24_NFChabrier242 × 28833.64× 1077.32 × 1064.0No feedback
Ch24_Zc_eA_sWaChabrier242 × 28833.64× 1077.32 × 1064.0Early AGN + Strong winds
Ch24_eA_MDWbChabrier242 × 28833.64× 1077.32 × 1064.0Early AGN +
Momentum-driven winds
Ch18_lA_wWChabrier182 × 38436.47× 1061.30 × 1062.0Late AGN + Weak winds
Ch12_eA_sWChabrier122 × 38431.92× 1063.86 × 1051.5Early AGN + Strong winds
RunIMFBox sizeNTOTMDMMGASComoving softeningFeedback
(Mpc h−1)(M h−1)(M h−1)(kpc h−1)
Kr24_eA_sWKroupa242 × 28833.64× 1077.32 × 1064.0Early AGN + Strong winds
Ch24_lA_wWChabrier242 × 28833.64× 1077.32 × 1064.0Late AGN + Weak winds
Sa24_eA_wWSalpeter242 × 28833.64× 1077.32 × 1064.0Early AGN + Weak winds
Ch24_eA_sWChabrier242 × 28833.64× 1077.32 × 1064.0Early AGN + Strong winds
Ch24_lA_sWChabrier242 × 28833.64× 1077.32 × 1064.0Late AGN + Strong winds
Ch24_eA_vsWChabrier242 × 28833.64× 1077.32 × 1064.0Early AGN + Very strong winds
Ch24_NFChabrier242 × 28833.64× 1077.32 × 1064.0No feedback
Ch24_Zc_eA_sWaChabrier242 × 28833.64× 1077.32 × 1064.0Early AGN + Strong winds
Ch24_eA_MDWbChabrier242 × 28833.64× 1077.32 × 1064.0Early AGN +
Momentum-driven winds
Ch18_lA_wWChabrier182 × 38436.47× 1061.30 × 1062.0Late AGN + Weak winds
Ch12_eA_sWChabrier122 × 38431.92× 1063.86 × 1051.5Early AGN + Strong winds
Table 1.

Summary of the different runs used in this work. Column 1: run name; column 2: initial mass function (IMF) chosen; column 3: box size in comoving Mpc h−1; column 4: total number of particles (NTOT = NGAS + NDM); column 5: mass of the dark matter particles; column 6: initial mass of the gas particles; column 7: plummer-equivalent comoving gravitational softening length; column 8: type of feedback implemented. See Section 2.2 for more details on the parameters used for the different feedback recipes. (a) In this simulation the effect of metal-line cooling is included. (b) In this simulation we adopt variable momentum-driven galactic winds. In all the other simulations galactic winds are energy driven and the wind velocity is constant (Section 2.1).

RunIMFBox sizeNTOTMDMMGASComoving softeningFeedback
(Mpc h−1)(M h−1)(M h−1)(kpc h−1)
Kr24_eA_sWKroupa242 × 28833.64× 1077.32 × 1064.0Early AGN + Strong winds
Ch24_lA_wWChabrier242 × 28833.64× 1077.32 × 1064.0Late AGN + Weak winds
Sa24_eA_wWSalpeter242 × 28833.64× 1077.32 × 1064.0Early AGN + Weak winds
Ch24_eA_sWChabrier242 × 28833.64× 1077.32 × 1064.0Early AGN + Strong winds
Ch24_lA_sWChabrier242 × 28833.64× 1077.32 × 1064.0Late AGN + Strong winds
Ch24_eA_vsWChabrier242 × 28833.64× 1077.32 × 1064.0Early AGN + Very strong winds
Ch24_NFChabrier242 × 28833.64× 1077.32 × 1064.0No feedback
Ch24_Zc_eA_sWaChabrier242 × 28833.64× 1077.32 × 1064.0Early AGN + Strong winds
Ch24_eA_MDWbChabrier242 × 28833.64× 1077.32 × 1064.0Early AGN +
Momentum-driven winds
Ch18_lA_wWChabrier182 × 38436.47× 1061.30 × 1062.0Late AGN + Weak winds
Ch12_eA_sWChabrier122 × 38431.92× 1063.86 × 1051.5Early AGN + Strong winds
RunIMFBox sizeNTOTMDMMGASComoving softeningFeedback
(Mpc h−1)(M h−1)(M h−1)(kpc h−1)
Kr24_eA_sWKroupa242 × 28833.64× 1077.32 × 1064.0Early AGN + Strong winds
Ch24_lA_wWChabrier242 × 28833.64× 1077.32 × 1064.0Late AGN + Weak winds
Sa24_eA_wWSalpeter242 × 28833.64× 1077.32 × 1064.0Early AGN + Weak winds
Ch24_eA_sWChabrier242 × 28833.64× 1077.32 × 1064.0Early AGN + Strong winds
Ch24_lA_sWChabrier242 × 28833.64× 1077.32 × 1064.0Late AGN + Strong winds
Ch24_eA_vsWChabrier242 × 28833.64× 1077.32 × 1064.0Early AGN + Very strong winds
Ch24_NFChabrier242 × 28833.64× 1077.32 × 1064.0No feedback
Ch24_Zc_eA_sWaChabrier242 × 28833.64× 1077.32 × 1064.0Early AGN + Strong winds
Ch24_eA_MDWbChabrier242 × 28833.64× 1077.32 × 1064.0Early AGN +
Momentum-driven winds
Ch18_lA_wWChabrier182 × 38436.47× 1061.30 × 1062.0Late AGN + Weak winds
Ch12_eA_sWChabrier122 × 38431.92× 1063.86 × 1051.5Early AGN + Strong winds
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