Table 1.
Open in new tab

Overview of the different samples, including the mass limits, Mlim, expressed in units of |$h^{-1}\, {\rm M}_{ {\odot} }$|⁠, the corresponding number of particles, Np, the mean number density, |$\bar{n}$|⁠, and the bias ratio to the corresponding Minerva parent sample, 〈(ξapp/ξMin)1/2〉. The sample names ‘mass’, ‘dens’, and ‘bias’, indicate if the samples were constructed by matching the mass threshold, number density, or clustering amplitude of the parent halo samples from Minerva.

CodeSample name|$M_{\rm lim}\left(h^{-1}\,{\rm M}_{ {\odot} }\right)$|Np|$\bar{n}\left(h^3\, {\rm Mpc}^{-3}\right)$|Bias ratio
Minervamass11.12 × 1013422.12 × 10−41.00
Minervamass22.67 × 10131005.42 × 10−51.00
ice-colamass11.12 × 1013422.06 × 10−40.99
ice-coladens11.09 × 1013412.12 × 10−40.98
ice-colabias11.17 × 1013441.93 × 10−41.00
ice-colamass22.67 × 10131005.81 × 10−50.99
ice-coladens2, bias22.77 × 10131045.45 × 10−51.00
halogenmass1, dens1, bias11.12 × 1013422.14 × 10−41.00
halogenmass2, dens22.67 × 10131005.40 × 10−50.98
halogenbias22.91 × 10131094.61 × 10−51.00
peak patchamass22.67 × 10131004.45 × 10−51.04
peak patchdens2, bias22.35 × 101388.35.44 × 10−51.00
pinocchiomass11.12 × 1013421.95 × 10−41.02
pinocchiodens11.04 × 101339.12.15 × 10−41.00
pinocchiobias11.06 × 101339.92.09 × 10−41.00
pinocchiomass22.67 × 10131005.35 × 10−51.03
pinocchiodens22.63 × 101398.65.48 × 10−51.03
pinocchiobias22.42 × 101390.76.27 × 10−51.00
CodeSample name|$M_{\rm lim}\left(h^{-1}\,{\rm M}_{ {\odot} }\right)$|Np|$\bar{n}\left(h^3\, {\rm Mpc}^{-3}\right)$|Bias ratio
Minervamass11.12 × 1013422.12 × 10−41.00
Minervamass22.67 × 10131005.42 × 10−51.00
ice-colamass11.12 × 1013422.06 × 10−40.99
ice-coladens11.09 × 1013412.12 × 10−40.98
ice-colabias11.17 × 1013441.93 × 10−41.00
ice-colamass22.67 × 10131005.81 × 10−50.99
ice-coladens2, bias22.77 × 10131045.45 × 10−51.00
halogenmass1, dens1, bias11.12 × 1013422.14 × 10−41.00
halogenmass2, dens22.67 × 10131005.40 × 10−50.98
halogenbias22.91 × 10131094.61 × 10−51.00
peak patchamass22.67 × 10131004.45 × 10−51.04
peak patchdens2, bias22.35 × 101388.35.44 × 10−51.00
pinocchiomass11.12 × 1013421.95 × 10−41.02
pinocchiodens11.04 × 101339.12.15 × 10−41.00
pinocchiobias11.06 × 101339.92.09 × 10−41.00
pinocchiomass22.67 × 10131005.35 × 10−51.03
pinocchiodens22.63 × 101398.65.48 × 10−51.03
pinocchiobias22.42 × 101390.76.27 × 10−51.00

Note. aAs the halo masses corresponding to our low-mass threshold are not correctly resolved in the peak patch catalogues, only the high-mass threshold (mass2) is considered in this case.

Table 1.
Open in new tab

Overview of the different samples, including the mass limits, Mlim, expressed in units of |$h^{-1}\, {\rm M}_{ {\odot} }$|⁠, the corresponding number of particles, Np, the mean number density, |$\bar{n}$|⁠, and the bias ratio to the corresponding Minerva parent sample, 〈(ξapp/ξMin)1/2〉. The sample names ‘mass’, ‘dens’, and ‘bias’, indicate if the samples were constructed by matching the mass threshold, number density, or clustering amplitude of the parent halo samples from Minerva.

CodeSample name|$M_{\rm lim}\left(h^{-1}\,{\rm M}_{ {\odot} }\right)$|Np|$\bar{n}\left(h^3\, {\rm Mpc}^{-3}\right)$|Bias ratio
Minervamass11.12 × 1013422.12 × 10−41.00
Minervamass22.67 × 10131005.42 × 10−51.00
ice-colamass11.12 × 1013422.06 × 10−40.99
ice-coladens11.09 × 1013412.12 × 10−40.98
ice-colabias11.17 × 1013441.93 × 10−41.00
ice-colamass22.67 × 10131005.81 × 10−50.99
ice-coladens2, bias22.77 × 10131045.45 × 10−51.00
halogenmass1, dens1, bias11.12 × 1013422.14 × 10−41.00
halogenmass2, dens22.67 × 10131005.40 × 10−50.98
halogenbias22.91 × 10131094.61 × 10−51.00
peak patchamass22.67 × 10131004.45 × 10−51.04
peak patchdens2, bias22.35 × 101388.35.44 × 10−51.00
pinocchiomass11.12 × 1013421.95 × 10−41.02
pinocchiodens11.04 × 101339.12.15 × 10−41.00
pinocchiobias11.06 × 101339.92.09 × 10−41.00
pinocchiomass22.67 × 10131005.35 × 10−51.03
pinocchiodens22.63 × 101398.65.48 × 10−51.03
pinocchiobias22.42 × 101390.76.27 × 10−51.00
CodeSample name|$M_{\rm lim}\left(h^{-1}\,{\rm M}_{ {\odot} }\right)$|Np|$\bar{n}\left(h^3\, {\rm Mpc}^{-3}\right)$|Bias ratio
Minervamass11.12 × 1013422.12 × 10−41.00
Minervamass22.67 × 10131005.42 × 10−51.00
ice-colamass11.12 × 1013422.06 × 10−40.99
ice-coladens11.09 × 1013412.12 × 10−40.98
ice-colabias11.17 × 1013441.93 × 10−41.00
ice-colamass22.67 × 10131005.81 × 10−50.99
ice-coladens2, bias22.77 × 10131045.45 × 10−51.00
halogenmass1, dens1, bias11.12 × 1013422.14 × 10−41.00
halogenmass2, dens22.67 × 10131005.40 × 10−50.98
halogenbias22.91 × 10131094.61 × 10−51.00
peak patchamass22.67 × 10131004.45 × 10−51.04
peak patchdens2, bias22.35 × 101388.35.44 × 10−51.00
pinocchiomass11.12 × 1013421.95 × 10−41.02
pinocchiodens11.04 × 101339.12.15 × 10−41.00
pinocchiobias11.06 × 101339.92.09 × 10−41.00
pinocchiomass22.67 × 10131005.35 × 10−51.03
pinocchiodens22.63 × 101398.65.48 × 10−51.03
pinocchiobias22.42 × 101390.76.27 × 10−51.00

Note. aAs the halo masses corresponding to our low-mass threshold are not correctly resolved in the peak patch catalogues, only the high-mass threshold (mass2) is considered in this case.

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