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unimach.yml
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title: UniverseMachine
synopsis: Empirical model developed by P. Behroozi and collaborators
descr: >
These lightcones have been populated using the UniverseMachine empirical model. For more details please see <a class="underline" target="_blank" href='http://adsabs.harvard.edu/abs/2018arXiv180607893B'>Behroozi et al.</a> (2019) and <a class="underline" href="https://arxiv.org/abs/2102.00108">Somerville et al. </a> (2020).<br></br>
Data Release: v1 2019-07-26.<br></br>
Data also available at <a class="underline" target="_blank" href="https://www.peterbehroozi.com/data.html">peterbehroozi.com</a>.
index: unimach
count: 250614266
order: 'candels-2'
pipeline: |
ctx['X'] = 1.47059*ctx['X'];
ctx['Y'] = 1.47059*ctx['Y'];
ctx['Z'] = 1.47059*ctx['Z'];
ctx['M'] = 1.0e-10*ctx['M'];
ctx['MP'] = 1.0e-10*ctx['MP'];
ctx['R'] = 0.00147059*ctx['R']*ctx['Scale'];
ctx['SM'] = 1.0e-10*ctx['SM'];
ctx['ICL'] = 1.0e-10*ctx['ICL'];
ctx['obs_SM'] = 1.0e-10*ctx['obs_SM'];
key: ID # i think? maybe need field?
fields:
- name: field
dict: candels_field
flag: top
- name: realization
dict: candels_realization
flag: top
- name: RA
dict: ppos_x
type: float
units: 'deg'
- name: Dec
dict: ppos_y
type: float
units: 'deg'
- name: Z(los)
dict: redshift
type: float
descr: Redshift including redshift-space distortions.
- name: Z(cosmo)
dict: true_redshift
type: float
descr: Cosmological redshift---i.e., without redshift-space distortions.
- name: Scale
type: float
descr: Scale factor of the timestep from which the halo was taken
- name: ID
dict: candels_gal_id # also halo_id
type: long
descr: Halo ID (unique across all timesteps)
- name: DescID
type: long
descr: ID of descendant halo (or -1 at z = 0)
- name: UPID
type: long
descr: -1 for central halos, otherwise, ID of largest parent halo
- name: ""
title: Position
units: 'Mpc'
sub:
- name: 'X'
title: 'X'
dict: pos_x
type: float
descr: 'Position of halo relative to axes of lightcone (distance along lightcone) in comoving Mpc/h'
- name: 'Y'
title: 'Y'
dict: pos_y
type: float
descr: 'Position of halo relative to axes of lightcone (distance perpendicular to lightcone X-axis) in comoving Mpc/h'
- name: 'Z'
title: 'Z'
dict: pos_z
type: float
descr: 'Position of halo relative to axes of lightcone (distance perpendicular to lightcone X-axis) in comoving Mpc/h'
- name: ""
title: Velocity
units: 'km/s'
dict: vel
sub:
- name: VX
# title: '\(V_x\)'
type: float
descr: 'Peculiar velocity in physical (i.e., non-comoving) km/s, relative to lightcone axes'
dict: vel_x
- name: VY
# title: '\(V_y\)'
type: float
descr: 'Peculiar velocity in physical (i.e., non-comoving) km/s, relative to lightcone axes'
dict: vel_y
- name: VZ
# title: '\(V_z\)'
type: float
descr: 'Peculiar velocity in physical (i.e., non-comoving) km/s, relative to lightcone axes'
dict: vel_z
- name: M
dict: M
type: float
descr: Halo mass (Bryan & Norman (BN98) 1998 virial mass)
units: '\(10^{10}M_\odot\)'
- name: V
type: float
descr: 'Halo \(v_{max}\) (physical)'
units: 'km/s'
- name: MP
type: float
descr: Halo peak historical mass (BN98 virial mass)
units: '\(10^{10}M_\odot\)'
- name: VMP
type: float
descr: Halo vmax at the time when peak mass was reached
units: 'km/s'
- name: R
dict: R
type: float
descr: 'Halo raidus (BN98 vir, co-moving kpc/h)'
units: 'Mpc'
- name: Rank1
type: float
descr: 'Halo rank (see UniverseMachine paper)'
units: '\(\Delta v_{max}\)'
- name: SM
dict: M_stellar
type: float
descr: True stellar mass
units: '\(10^{10}M_\odot\)'
- name: ICL
type: float
descr: True intracluster stellar mass
units: '\(10^{10}M_\odot\)'
- name: SFR
dict: SFR
type: float
descr: True star formation rate
units: '\(M_\odot/yr\)'
- name: obs_SM
type: float
descr: Observed stellar mass, including random & systematic errors
units: '\(10^{10}M_\odot\)'
- name: obs_SFR
type: float
descr: Observed star formation rate (SFR), including random & systemic errors
units: '\(M_\odot/yr\)'
- name: SSFR
type: float
descr: Observed SSFR
- name: "SM/HM"
type: float
descr: SM/HM ratio
- name: obs_UV
dict: UV1500_rest
type: float
descr: Observed UV Magnitude
units: '\(M_{1500} AB\)'
- name: A_UV
type: float
descr: UV attenuation from dust
units: 'AB Mag'