Included Runs
FLAMINGOL400N1440
Basic
- Box-size: \(400\; \rm{Mpc}\)
- Dark matter particle mass: \(7.06 \times 10^{8}\; \rm{M}_\odot\)
- Gas particle mass: \(1.34 \times 10^{8}\; \rm{M}_\odot\)
- Snapshot \(z=0.00\), \(a=1.00\)
Particle Numbers
Cube root of Dark Matter particle number: 1440
| Gas | Dark Matter | Star | Black Hole |
|---|---|---|---|
| 2674975467 | 2985984000 | 300939671 | 6526307 |
Gravitational Softening
| Baryons | Dark Matter | ||
|---|---|---|---|
| Max Physical | Comoving | Max Physical | Comoving |
| \(2.85\; \rm{kpc}\) | \(11.2\; \rm{kpc}\) | \(2.85\; \rm{kpc}\) | \(11.2\; \rm{kpc}\) |
Star Formation
| Parameter | Value |
|---|---|
| Star Formation Model | PressureLaw |
| Temperature Ceiling | |
| Threshold SF \(n_{\rm H, max}\) | cm\(^{-3}\) |
Stellar Feedback
| Parameter | Value |
|---|---|
| SNII Energy | \(1 \times 10^{51}\; \rm{erg}\) |
| \(f_{\rm E, min}\) | \(0.502\) |
| \(f_{\rm E, max}\) | \(0.502\) |
| \(f_{\rm kinetic}\) | |
| SNII \(v_{\rm kick}\) | |
| SNII \(\Delta T\) |
Gas Cooling
COLIBRE
Entropy Floor
No entropy floor present
Chemistry
| Parameter | Value |
|---|---|
| Metal diffusion constant |
AGN feedback
| Parameter | Value |
|---|---|
| AGN Feedback Model | MinimumDistance |
| Use Deterministic Feedback | \(1\) |
| \(\Delta T\) | \(9.85 \times 10^{7}\; \rm{K}\) |
| Coupling efficiency | \(0.15\) |
| Radiative efficiency | \(0.1\) |
| BH Subgrid Seed Mass | \(1 \times 10^{5}\; \rm{M}_\odot\) |
| Seed Halo Mass | \(3.44 \times 10^{10}\; \rm{M}_\odot\) |
| Target number of particles to heat N\(_{\rm heat}\) | \(1\) |
| Are we using the boost factor | \(1\) |
| Value of \(\alpha\) for boost factor | |
| Value of \(\beta\) for boost factor | \(0.147\) |
| Value of \(n_{H,*}\) in cm\(^{-3}\) for boost factor | |
| Use sub-grid gas properties | |
| Minimum BH time-step | |
| Maximal Reposition Mass | \(1 \times 10^{20}\; \rm{M}_\odot\) |
| Black Hole Merger Threshold Type | \(2\) |
| Black Hole Merger Max Distance Ratio | \(3\) |
Code Setup
- Code info: SWIFT (temperature_bug_tracking) v0.9.0-1289-g5ffc569f-dirty 2021-12-02 23:12:03 +0100
- Compiler info: ICC (20.21.20201112) Intel(R) MPI Library 2018 Update 2 for Linux* OS (MPI std v3.1)
- Hydrodynamics: SPHENIX (Borrow+ 2020) Wendland C2 in 3D $\eta$ = 1.23 (57.27 $N_{ngb}$) $C_{\rm CFL}$ = 0.20
AAA Calibration
Stellar Mass Function (50 kpc aperture) with Eddington bias with extended ranges
50 kpc aperture GSMF, showing all galaxies with a fixed bin-width of 0.2 dex. Includes Eddington bias.
Halo gas fractions within $R_{500}$
Gas fractions within $R_{500}$ normalised by the cosmic mean. These are 'true' values, i.e. no cut or observational correction was applied.
Ages
Stellar mass - Stellar age relation (30 kpc aperture)
Stellar mass - Stellar age relation (100 kpc aperture)
Baryon Fractions
Halo baryon fractions within $R_{500}$
Baryon (gas + stars) fractions within $R_{500}$ normalised by the cosmic mean. These are 'true' values, i.e. no cut or observational correction was applied.
Halo gas fractions within $R_{500}$
Gas fractions within $R_{500}$ normalised by the cosmic mean. These are 'true' values, i.e. no cut or observational correction was applied.
Halo stellar fractions within $R_{500}$
Stellar fractions within $R_{500}$ normalised by the cosmic mean. These are 'true' values, i.e. no cut or observational correction was applied.
Halo gas masses within $R_{500}$
Gas masses within $R_{500}$. These are 'true' values, i.e. no cut or observational correction was applied.
Black Holes
Black Hole Dynanmical and Subgrid Masses
Relation between black hole particle (dynamical) masses and subgrid masses. The vertical dashed lines shows the primordial gas particle mass and the horizontal dashed lines corresponds to the black hole seed mass.
Stellar Mass-Black Hole Mass relation (30 kpc Stellar Mass)
SMBHM relation for the 30 kpc stellar mass aperture.
Stellar Mass-Black Hole Mass relation (50 kpc Stellar Mass)
SMBHM relation for the 50 kpc stellar mass aperture.
Stellar Mass-Black Hole Mass relation (100 kpc Stellar Mass)
SMBHM relation. Note that the stellar velocity dispersion is measured in observations in a fixed 1 kpc aperture
Halo Mass-Black Hole Mass relation
Presented for comparison between schemes as halo mass varies significantly less between models and runs.
Stellar Velocity Dispersion-Black Hole Mass relation (10 kpc)
Note that the stellar velocity dispersion is measured in observations in a fixed 1 kpc aperture
Stellar Velocity Dispersion-Black Hole Mass relation (30 kpc)
Note that the stellar velocity dispersion is measured in observations in a fixed 1 kpc aperture
Black Holes Evolution
Black Hole Accretion History
Evolution of the accretion rate onto BHs per unit co-moving volume.
Black Hole Mass History
Evolution of the BH mass per unit co-moving volume.
Galaxy Sizes
Stellar Mass-Galaxy Size relation (100 kpc aperture)
Uses a 100 kpc 3D aperture.
Stellar Mass-(Projected) Galaxy Size relation (100 kpc aperture)
Uses stellar sizes calculated from a projected distribution within a 100 kpc aperture.
Stellar Mass-(Projected) Galaxy Size relation (100 kpc aperture)
Only shows active galaxies defined based on their sSFRs.
Stellar Mass-(Projected) Galaxy Size relation (100 kpc aperture)
Only shows passive galaxies defined based on their sSFRs.
Halo Mass Function
Halo Mass Function ($M_{200, crit}$)
Halo masses are masses within the over-density radius enclosing 200x the critical density.
Halo Mass Function ($M_{200, crit}$)
Halo masses are masses within the over-density radius enclosing 200x the critical density, using adaptive binning.
Histograms
Stellar Mass Histogram (100 kpc aperture)
Histogram of stellar masses using the same bins as the mass function.
Stellar Mass Histogram (100 kpc aperture, active)
Only for active galaxies.
Stellar Mass Histogram (100 kpc aperture, passive)
Only for passive galaxies.
Halo Mass Histogram (\(M_{200, crit}\))
All halo masses (200 crit).
Star Formation Rate Histogram (100 kpc aperture)
Histogram of star formation rates using the same bins as the star formation rates function.
Black Hole Mass Histogram (Max, subgrid)
Uses the same bins as in the black holes section.
Luminosity Function
u-band Luminosity Function (30 kpc aperture)
30 kpc aperture dust-free rest-frame luminosity function in the GAMA u-band, constructed using the Trayford et al. (2015) model, showing all galaxies with a fixed bin-width of 0.2 dex.
g-band Luminosity Function (30 kpc aperture)
30 kpc aperture dust-free rest-frame luminosity function in the GAMA g-band, constructed using the Trayford et al. (2015) model, showing all galaxies with a fixed bin-width of 0.2 dex.
r-band Luminosity Function (30 kpc aperture)
30 kpc aperture dust-free rest-frame luminosity function in the GAMA r-band, constructed using the Trayford et al. (2015) model, showing all galaxies with a fixed bin-width of 0.2 dex.
i-band Luminosity Function (30 kpc aperture)
30 kpc aperture dust-free rest-frame luminosity function in the GAMA i-band, constructed using the Trayford et al. (2015) model, showing all galaxies with a fixed bin-width of 0.2 dex.
z-band Luminosity Function (30 kpc aperture)
30 kpc aperture dust-free rest-frame luminosity function in the GAMA z-band, constructed using the Trayford et al. (2015) model, showing all galaxies with a fixed bin-width of 0.2 dex.
Y-band Luminosity Function (30 kpc aperture)
30 kpc aperture dust-free rest-frame luminosity function in the GAMA Y-band, constructed using the Trayford et al. (2015) model, showing all galaxies with a fixed bin-width of 0.2 dex.
J-band Luminosity Function (30 kpc aperture)
30 kpc aperture dust-free rest-frame luminosity function in the GAMA J-band, constructed using the Trayford et al. (2015) model, showing all galaxies with a fixed bin-width of 0.2 dex.
H-band Luminosity Function (30 kpc aperture)
30 kpc aperture dust-free rest-frame luminosity function in the GAMA H-band, constructed using the Trayford et al. (2015) model, showing all galaxies with a fixed bin-width of 0.2 dex.
K-band Luminosity Function (30 kpc aperture)
30 kpc aperture dust-free rest-frame luminosity function in the GAMA K-band, constructed using the Trayford et al. (2015) model, showing all galaxies with a fixed bin-width of 0.2 dex.
Metal Evolution
Gas Phase Metal Mass Density Evolution
Evolution of the metal mass in gas per unit co-moving volume.
Metal Mass Locked in Stars Density Evolution
Evolution of the metal mass locked in stars per unit co-moving volume.
Metal Mass Locked in Black Holes Density Evolution
Evolution of the metal mass locked in black holes per unit co-moving volume.
Metal Mass Fractions
Metal Mass Fraction Distribution
Metal mass fraction distribution shown for each simulation; solid lines show gas metallicity and dashed lines show the same for the stars.
Metallicity
Stellar mass - Gas metallicity relation (30 kpc aperture)
Only shown for star forming galaxies. A minimum metallicity of 12 + log O/H = 7.5 is imposed for the star-forming gas. All haloes are plotted, including subhaloes.
Stellar mass - Gas metallicity relation (100 kpc aperture)
Only shown for star forming galaxies. A minimum metallicity of 12 + log O/H = 7.5 is imposed for the star-forming gas. All haloes are plotted, including subhaloes.
Stellar mass - Star metallicity relation (100 kpc aperture)
Metallicity is measured in the same aperture as the stellar mass. Gallazzi data is corrected from their choice of solar metallicity (0.02) to ours (0.0126).
Stellar mass - Star metallicity relation (30 kpc aperture)
Metallicity is measured in the same aperture as the stellar mass. Gallazzi data is corrected from their choice of solar metallicity (0.02) to ours (0.0126).
Run Performance
Wall-clock time per gas particle updates.
Wall-clock time to run a time-step as a function of the number of gas particles updated. The tracks at the top correspond to steps where the tree is rebuilt, i/o is performed, FoF is run or other non-regular operations are done.
Cosmic time vs. wall-clock time
The cosmic time as a function of the wall-clock time.
The number of steps vs. wall-clock time
The cumulative number of the simulation time-steps as a function of the wall-clock time.
Number of steps vs. cosmic time
The cumulative number of the simulation time-steps as a function of the cosmic time.
Wall-clock time per time-bin
Total wall-clock time spent in each of the different simulation time-bins.
Star Formation History
Star Formation History
Star formation history plotted directly from the SFR.txt file produced by SWIFT.
Stellar Mass Evolution
Evolution of the stellar mass plotted directly from the statistics.txt file produced by SWIFT.
Star Formation Rates
Stellar Mass-Star Formation Rate (30 kpc Stellar Mass)
All galaxies, including those deemed to be passive (below 0.01 / Gyr sSFR), are included in the median line.
Stellar Mass-Star Formation Rate (50 kpc Stellar Mass)
All galaxies, including those deemed to be passive (below 0.01 / Gyr sSFR), are included in the median line.
Stellar Mass-Star Formation Rate (100 kpc Stellar Mass)
All galaxies, including those deemed to be passive (below 0.01 / Gyr sSFR), are included in the median line.
Specific Star Formation Rate - Stellar Mass (100 kpc) for active galaxies
Only active galaxies (threshold is above 0.01 / Gyr sSFR) are included in the median line.
Specific Star Formation Rate - Stellar Mass (50 kpc) for active galaxies
Only active galaxies (threshold is above 0.01 / Gyr sSFR) are included in the median line.
Specific Star Formation Rate - Stellar Mass (30 kpc) for active galaxies
Only active galaxies (threshold is above 0.01 / Gyr sSFR) are included in the median line.
Specific Star Formation Rate - Stellar Mass (100 kpc)
All galaxies (threshold is above 0.01 / Gyr sSFR) are included in the median line.
Specific Star Formation Rate - Stellar Mass (50 kpc)
All galaxies (threshold is above 0.01 / Gyr sSFR) are included in the median line.
Specific Star Formation Rate - Stellar Mass (30 kpc)
All galaxies (threshold is above 0.01 / Gyr sSFR) are included in the median line.
Specific Star Formation Rate (100 kpc) - Halo Mass
Only active galaxies (threshold is above 0.01 / Gyr sSFR) are included in the median line.
Specific Star Formation Rate (50 kpc) - Halo Mass
Only active galaxies (threshold is above 0.01 / Gyr sSFR) are included in the median line.
Specific Star Formation Rate (30 kpc) - Halo Mass
Only active galaxies (threshold is above 0.01 / Gyr sSFR) are included in the median line.
Specific Star Formation Rate (100 kpc) - Halo Mass
All galaxies are included in the median line.
Specific Star Formation Rate (50 kpc) - Halo Mass
All galaxies are included in the median line.
Specific Star Formation Rate (30 kpc) - Halo Mass
All galaxies are included in the median line.
Star Formation Rate divided by Halo Mass (100 kpc) - Halo Mass
Only active galaxies (threshold is above 0.01 / Gyr sSFR) are included in the median line
Star Formation Rate divided by Halo Mass (50 kpc) - Halo Mass
Only active galaxies (threshold is above 0.01 / Gyr sSFR) are included in the median line
Star Formation Rate divided by Halo Mass (30 kpc) - Halo Mass
Only active galaxies (threshold is above 0.01 / Gyr sSFR) are included in the median line
Passive Fraction - Stellar Mass (100 kpc)
A galaxy is determined as being passive if it has a sSFR below 0.01 / Gyr.
Passive Fraction - Stellar Mass (50 kpc)
A galaxy is determined as being passive if it has a sSFR below 0.01 / Gyr.
Passive Fraction - Stellar Mass (30 kpc)
A galaxy is determined as being passive if it has a sSFR below 0.01 / Gyr.
Passive Fraction - Stellar Mass (100 kpc aperture, centrals)
A galaxy is determined as being passive if it has a sSFR below 0.01 / Gyr. This figure shows only the central galaxies (structure type 10).
Passive Fraction - Stellar Mass (50 kpc aperture, centrals)
A galaxy is determined as being passive if it has a sSFR below 0.01 / Gyr. This figure shows only the central galaxies (structure type 10).
Passive Fraction - Stellar Mass (30 kpc aperture, centrals)
A galaxy is determined as being passive if it has a sSFR below 0.01 / Gyr. This figure shows only the central galaxies (structure type 10).
Star Formation Rate Function (100 kpc aperture)
100 kpc aperture galaxy star formation rate function, showing all galaxies with a fixed bin-width of 0.2 dex.
Star Formation Rate Function (50 kpc aperture)
30 kpc aperture galaxy star formation rate function, showing all galaxies with a fixed bin-width of 0.2 dex.
Star Formation Rate Function (30 kpc aperture)
30 kpc aperture galaxy star formation rate function, showing all galaxies with a fixed bin-width of 0.2 dex.
Star Formation Rate Function (100 kpc aperture)
100 kpc aperture galaxy star formation rate function, showing all galaxies with an adaptive bin-width.
Star Formation Rate Function (50 kpc aperture)
30 kpc aperture galaxy star formation rate function, showing all galaxies with an adaptive bin-width
Star Formation Rate Function (30 kpc aperture)
30 kpc aperture galaxy star formation rate function, showing all galaxies with an adaptive bin-width
Stellar Mass Function
Stellar Mass Function (30 kpc aperture)
30 kpc aperture GSMF, showing all galaxies with a fixed bin-width of 0.2 dex. For 30kpc look at the Li and White (2009) data.
Stellar Mass Function (30 kpc aperture, adaptive)
30 kpc aperture GSMF, showing all galaxies with an adaptive bin-width. For 30kpc look at the Li and White (2009) data.
Stellar Mass Function (100 kpc aperture)
100 kpc aperture GSMF, showing all galaxies with a fixed bin-width of 0.2 dex.
Stellar Mass Function (100 kpc aperture, adaptive)
100 kpc aperture GSMF, showing all galaxies with an adaptive bin-width.
Stellar Mass Function (100 kpc aperture)
Only for passive galaxies.
Stellar Mass Function (100 kpc aperture)
Only for active galaxies.
Stellar Mass Function (50 kpc aperture)
50 kpc aperture GSMF, showing all galaxies with a fixed bin-width of 0.2 dex. For 50kpc, look at D'Souza (2015) data.
Stellar Mass Function (50 kpc aperture, adaptive)
50 kpc aperture GSMF, showing all galaxies with an adaptive bin-width. For 50kpc, look at D'Souza (2015) data.
Stellar Mass Function (30 kpc aperture) with Eddington bias
50 kpc aperture GSMF, showing all galaxies with a fixed bin-width of 0.2 dex. Includes Eddington bias.
Stellar Mass Function (50 kpc aperture) with Eddington bias
50 kpc aperture GSMF, showing all galaxies with a fixed bin-width of 0.2 dex. Includes Eddington bias.
Stellar Mass Function (100 kpc aperture) with Eddington bias
50 kpc aperture GSMF, showing all galaxies with a fixed bin-width of 0.2 dex. Includes Eddington bias.
Stellar Mass Function (50 kpc aperture) with Eddington bias with extended ranges
50 kpc aperture GSMF, showing all galaxies with a fixed bin-width of 0.2 dex. Includes Eddington bias.
Stellar Mass-Halo Mass
Stellar Mass-Halo Mass relation (100 kpc aperture)
Includes all haloes, including subhaloes.
Stellar Mass-Halo Mass relation (100 kpc aperture, centrals only)
Includes only central haloes.
Stellar Mass-Halo Mass relation (ratio, 100 kpc aperture, centrals only)
Includes only central haloes.
Stellar Mass-Halo Mass relation (ratio, 100 kpc aperture, centrals only, stellar x-axis)
Includes only central haloes.
Stellar Mass-Halo Mass relation (50 kpc aperture)
Includes all haloes, including subhaloes.
Stellar Mass-Halo Mass relation (50 kpc aperture, centrals only)
Includes only central haloes.
Stellar Mass-Halo Mass relation (ratio, 50 kpc aperture, centrals only)
Includes only central haloes.
Stellar Mass-Halo Mass relation (ratio, 50 kpc aperture, centrals only, stellar x-axis)
Includes only central haloes.
Stellar Mass-Halo Mass relation (30 kpc aperture)
Includes all haloes, including subhaloes.
Stellar Mass-Halo Mass relation (30 kpc aperture, centrals only)
Includes only central haloes.
Stellar Mass-Halo Mass relation (ratio, 30 kpc aperture, centrals only)
Includes only central haloes.
Stellar Mass-Halo Mass relation (ratio, 30 kpc aperture, centrals only, stellar x-axis)
Includes only central haloes.
Stellar Mass-Halo Mass relation (100 kpc aperture, M$_{\rm BN98}$)
Includes all haloes, including subhaloes.
Stellar Mass-Halo Mass relation (50 kpc aperture, M$_{\rm BN98}$)
Includes all haloes, including subhaloes.
Stellar Mass-Halo Mass relation (30 kpc aperture, M$_{\rm BN98}$)
Includes all haloes, including subhaloes.
Stellar Mass-Halo Mass relation (100 kpc aperture, centrals only, M$_{\rm BN98}$)
Includes only central haloes.
Stellar Mass-Halo Mass relation (50 kpc aperture, centrals only, M$_{\rm BN98}$)
Includes only central haloes.
Stellar Mass-Halo Mass relation (30 kpc aperture, centrals only, M$_{\rm BN98}$)
Includes only central haloes.
Stellar Mass-Halo Mass relation (ratio, 100 kpc aperture, $M_{\rm BN98}$, centrals only, stellar x-axis)
Includes only central haloes.
Stellar Mass-Halo Mass relation (ratio, 50 kpc aperture, $M_{\rm BN98}$, centrals only, stellar x-axis)
Includes only central haloes.
Stellar Mass-Halo Mass relation (ratio, 30 kpc aperture, $M_{\rm BN98}$, centrals only, stellar x-axis)
Includes only central haloes.
Stellar Mass-Halo Mass relation (ratio, 100 kpc aperture, $M_{\rm BN98}$, centrals only)
Includes only central haloes.
Stellar Mass-Halo Mass relation (ratio, 50 kpc aperture, $M_{\rm BN98}$, centrals only)
Includes only central haloes.
Stellar Mass-Halo Mass relation (ratio, 30 kpc aperture, $M_{\rm BN98}$, centrals only)
Includes only central haloes.
Tully-Fisher
Tully-Fisher (stellar mass, 100 kpc)
The Tully-Fisher relation based on stellar mass.
Tully-Fisher (stellar mass, 30 kpc)
The Tully-Fisher relation based on stellar mass.
Stellar Mass Function (50 kpc aperture) with Eddington bias with extended ranges
50 kpc aperture GSMF, showing all galaxies with a fixed bin-width of 0.2 dex. Includes Eddington bias.
Halo gas fractions within $R_{500}$
Gas fractions within $R_{500}$ normalised by the cosmic mean. These are 'true' values, i.e. no cut or observational correction was applied.
Halo baryon fractions within $R_{500}$
Baryon (gas + stars) fractions within $R_{500}$ normalised by the cosmic mean. These are 'true' values, i.e. no cut or observational correction was applied.
Halo gas fractions within $R_{500}$
Gas fractions within $R_{500}$ normalised by the cosmic mean. These are 'true' values, i.e. no cut or observational correction was applied.
Halo stellar fractions within $R_{500}$
Stellar fractions within $R_{500}$ normalised by the cosmic mean. These are 'true' values, i.e. no cut or observational correction was applied.
Halo gas masses within $R_{500}$
Gas masses within $R_{500}$. These are 'true' values, i.e. no cut or observational correction was applied.
Black Hole Dynanmical and Subgrid Masses
Relation between black hole particle (dynamical) masses and subgrid masses. The vertical dashed lines shows the primordial gas particle mass and the horizontal dashed lines corresponds to the black hole seed mass.
Stellar Mass-Black Hole Mass relation (30 kpc Stellar Mass)
SMBHM relation for the 30 kpc stellar mass aperture.
Stellar Mass-Black Hole Mass relation (50 kpc Stellar Mass)
SMBHM relation for the 50 kpc stellar mass aperture.
Stellar Mass-Black Hole Mass relation (100 kpc Stellar Mass)
SMBHM relation. Note that the stellar velocity dispersion is measured in observations in a fixed 1 kpc aperture
Halo Mass-Black Hole Mass relation
Presented for comparison between schemes as halo mass varies significantly less between models and runs.
Stellar Velocity Dispersion-Black Hole Mass relation (10 kpc)
Note that the stellar velocity dispersion is measured in observations in a fixed 1 kpc aperture
Stellar Velocity Dispersion-Black Hole Mass relation (30 kpc)
Note that the stellar velocity dispersion is measured in observations in a fixed 1 kpc aperture
Stellar Mass-(Projected) Galaxy Size relation (100 kpc aperture)
Uses stellar sizes calculated from a projected distribution within a 100 kpc aperture.
Stellar Mass-(Projected) Galaxy Size relation (100 kpc aperture)
Only shows active galaxies defined based on their sSFRs.
Stellar Mass-(Projected) Galaxy Size relation (100 kpc aperture)
Only shows passive galaxies defined based on their sSFRs.
Halo Mass Function ($M_{200, crit}$)
Halo masses are masses within the over-density radius enclosing 200x the critical density.
Halo Mass Function ($M_{200, crit}$)
Halo masses are masses within the over-density radius enclosing 200x the critical density, using adaptive binning.
Stellar Mass Histogram (100 kpc aperture)
Histogram of stellar masses using the same bins as the mass function.
Star Formation Rate Histogram (100 kpc aperture)
Histogram of star formation rates using the same bins as the star formation rates function.
u-band Luminosity Function (30 kpc aperture)
30 kpc aperture dust-free rest-frame luminosity function in the GAMA u-band, constructed using the Trayford et al. (2015) model, showing all galaxies with a fixed bin-width of 0.2 dex.
g-band Luminosity Function (30 kpc aperture)
30 kpc aperture dust-free rest-frame luminosity function in the GAMA g-band, constructed using the Trayford et al. (2015) model, showing all galaxies with a fixed bin-width of 0.2 dex.
r-band Luminosity Function (30 kpc aperture)
30 kpc aperture dust-free rest-frame luminosity function in the GAMA r-band, constructed using the Trayford et al. (2015) model, showing all galaxies with a fixed bin-width of 0.2 dex.
i-band Luminosity Function (30 kpc aperture)
30 kpc aperture dust-free rest-frame luminosity function in the GAMA i-band, constructed using the Trayford et al. (2015) model, showing all galaxies with a fixed bin-width of 0.2 dex.
z-band Luminosity Function (30 kpc aperture)
30 kpc aperture dust-free rest-frame luminosity function in the GAMA z-band, constructed using the Trayford et al. (2015) model, showing all galaxies with a fixed bin-width of 0.2 dex.
Y-band Luminosity Function (30 kpc aperture)
30 kpc aperture dust-free rest-frame luminosity function in the GAMA Y-band, constructed using the Trayford et al. (2015) model, showing all galaxies with a fixed bin-width of 0.2 dex.
J-band Luminosity Function (30 kpc aperture)
30 kpc aperture dust-free rest-frame luminosity function in the GAMA J-band, constructed using the Trayford et al. (2015) model, showing all galaxies with a fixed bin-width of 0.2 dex.
H-band Luminosity Function (30 kpc aperture)
30 kpc aperture dust-free rest-frame luminosity function in the GAMA H-band, constructed using the Trayford et al. (2015) model, showing all galaxies with a fixed bin-width of 0.2 dex.
K-band Luminosity Function (30 kpc aperture)
30 kpc aperture dust-free rest-frame luminosity function in the GAMA K-band, constructed using the Trayford et al. (2015) model, showing all galaxies with a fixed bin-width of 0.2 dex.
Gas Phase Metal Mass Density Evolution
Evolution of the metal mass in gas per unit co-moving volume.
Metal Mass Locked in Stars Density Evolution
Evolution of the metal mass locked in stars per unit co-moving volume.
Metal Mass Locked in Black Holes Density Evolution
Evolution of the metal mass locked in black holes per unit co-moving volume.
Metal Mass Fraction Distribution
Metal mass fraction distribution shown for each simulation; solid lines show gas metallicity and dashed lines show the same for the stars.
Stellar mass - Gas metallicity relation (30 kpc aperture)
Only shown for star forming galaxies. A minimum metallicity of 12 + log O/H = 7.5 is imposed for the star-forming gas. All haloes are plotted, including subhaloes.
Stellar mass - Gas metallicity relation (100 kpc aperture)
Only shown for star forming galaxies. A minimum metallicity of 12 + log O/H = 7.5 is imposed for the star-forming gas. All haloes are plotted, including subhaloes.
Stellar mass - Star metallicity relation (100 kpc aperture)
Metallicity is measured in the same aperture as the stellar mass. Gallazzi data is corrected from their choice of solar metallicity (0.02) to ours (0.0126).
Stellar mass - Star metallicity relation (30 kpc aperture)
Metallicity is measured in the same aperture as the stellar mass. Gallazzi data is corrected from their choice of solar metallicity (0.02) to ours (0.0126).
Wall-clock time per gas particle updates.
Wall-clock time to run a time-step as a function of the number of gas particles updated. The tracks at the top correspond to steps where the tree is rebuilt, i/o is performed, FoF is run or other non-regular operations are done.
The number of steps vs. wall-clock time
The cumulative number of the simulation time-steps as a function of the wall-clock time.
Number of steps vs. cosmic time
The cumulative number of the simulation time-steps as a function of the cosmic time.
Wall-clock time per time-bin
Total wall-clock time spent in each of the different simulation time-bins.
Star Formation History
Star formation history plotted directly from the SFR.txt file produced by SWIFT.
Stellar Mass Evolution
Evolution of the stellar mass plotted directly from the statistics.txt file produced by SWIFT.
Stellar Mass-Star Formation Rate (30 kpc Stellar Mass)
All galaxies, including those deemed to be passive (below 0.01 / Gyr sSFR), are included in the median line.
Stellar Mass-Star Formation Rate (50 kpc Stellar Mass)
All galaxies, including those deemed to be passive (below 0.01 / Gyr sSFR), are included in the median line.
Stellar Mass-Star Formation Rate (100 kpc Stellar Mass)
All galaxies, including those deemed to be passive (below 0.01 / Gyr sSFR), are included in the median line.
Specific Star Formation Rate - Stellar Mass (100 kpc) for active galaxies
Only active galaxies (threshold is above 0.01 / Gyr sSFR) are included in the median line.
Specific Star Formation Rate - Stellar Mass (50 kpc) for active galaxies
Only active galaxies (threshold is above 0.01 / Gyr sSFR) are included in the median line.
Specific Star Formation Rate - Stellar Mass (30 kpc) for active galaxies
Only active galaxies (threshold is above 0.01 / Gyr sSFR) are included in the median line.
Specific Star Formation Rate - Stellar Mass (100 kpc)
All galaxies (threshold is above 0.01 / Gyr sSFR) are included in the median line.
Specific Star Formation Rate - Stellar Mass (50 kpc)
All galaxies (threshold is above 0.01 / Gyr sSFR) are included in the median line.
Specific Star Formation Rate - Stellar Mass (30 kpc)
All galaxies (threshold is above 0.01 / Gyr sSFR) are included in the median line.
Specific Star Formation Rate (100 kpc) - Halo Mass
Only active galaxies (threshold is above 0.01 / Gyr sSFR) are included in the median line.
Specific Star Formation Rate (50 kpc) - Halo Mass
Only active galaxies (threshold is above 0.01 / Gyr sSFR) are included in the median line.
Specific Star Formation Rate (30 kpc) - Halo Mass
Only active galaxies (threshold is above 0.01 / Gyr sSFR) are included in the median line.
Star Formation Rate divided by Halo Mass (100 kpc) - Halo Mass
Only active galaxies (threshold is above 0.01 / Gyr sSFR) are included in the median line
Star Formation Rate divided by Halo Mass (50 kpc) - Halo Mass
Only active galaxies (threshold is above 0.01 / Gyr sSFR) are included in the median line
Star Formation Rate divided by Halo Mass (30 kpc) - Halo Mass
Only active galaxies (threshold is above 0.01 / Gyr sSFR) are included in the median line
Passive Fraction - Stellar Mass (100 kpc)
A galaxy is determined as being passive if it has a sSFR below 0.01 / Gyr.
Passive Fraction - Stellar Mass (50 kpc)
A galaxy is determined as being passive if it has a sSFR below 0.01 / Gyr.
Passive Fraction - Stellar Mass (30 kpc)
A galaxy is determined as being passive if it has a sSFR below 0.01 / Gyr.
Passive Fraction - Stellar Mass (100 kpc aperture, centrals)
A galaxy is determined as being passive if it has a sSFR below 0.01 / Gyr. This figure shows only the central galaxies (structure type 10).
Passive Fraction - Stellar Mass (50 kpc aperture, centrals)
A galaxy is determined as being passive if it has a sSFR below 0.01 / Gyr. This figure shows only the central galaxies (structure type 10).
Passive Fraction - Stellar Mass (30 kpc aperture, centrals)
A galaxy is determined as being passive if it has a sSFR below 0.01 / Gyr. This figure shows only the central galaxies (structure type 10).
Star Formation Rate Function (100 kpc aperture)
100 kpc aperture galaxy star formation rate function, showing all galaxies with a fixed bin-width of 0.2 dex.
Star Formation Rate Function (50 kpc aperture)
30 kpc aperture galaxy star formation rate function, showing all galaxies with a fixed bin-width of 0.2 dex.
Star Formation Rate Function (30 kpc aperture)
30 kpc aperture galaxy star formation rate function, showing all galaxies with a fixed bin-width of 0.2 dex.
Star Formation Rate Function (100 kpc aperture)
100 kpc aperture galaxy star formation rate function, showing all galaxies with an adaptive bin-width.
Star Formation Rate Function (50 kpc aperture)
30 kpc aperture galaxy star formation rate function, showing all galaxies with an adaptive bin-width
Star Formation Rate Function (30 kpc aperture)
30 kpc aperture galaxy star formation rate function, showing all galaxies with an adaptive bin-width
Stellar Mass Function (30 kpc aperture)
30 kpc aperture GSMF, showing all galaxies with a fixed bin-width of 0.2 dex. For 30kpc look at the Li and White (2009) data.
Stellar Mass Function (30 kpc aperture, adaptive)
30 kpc aperture GSMF, showing all galaxies with an adaptive bin-width. For 30kpc look at the Li and White (2009) data.
Stellar Mass Function (100 kpc aperture)
100 kpc aperture GSMF, showing all galaxies with a fixed bin-width of 0.2 dex.
Stellar Mass Function (100 kpc aperture, adaptive)
100 kpc aperture GSMF, showing all galaxies with an adaptive bin-width.
Stellar Mass Function (50 kpc aperture)
50 kpc aperture GSMF, showing all galaxies with a fixed bin-width of 0.2 dex. For 50kpc, look at D'Souza (2015) data.
Stellar Mass Function (50 kpc aperture, adaptive)
50 kpc aperture GSMF, showing all galaxies with an adaptive bin-width. For 50kpc, look at D'Souza (2015) data.
Stellar Mass Function (30 kpc aperture) with Eddington bias
50 kpc aperture GSMF, showing all galaxies with a fixed bin-width of 0.2 dex. Includes Eddington bias.
Stellar Mass Function (50 kpc aperture) with Eddington bias
50 kpc aperture GSMF, showing all galaxies with a fixed bin-width of 0.2 dex. Includes Eddington bias.
Stellar Mass Function (100 kpc aperture) with Eddington bias
50 kpc aperture GSMF, showing all galaxies with a fixed bin-width of 0.2 dex. Includes Eddington bias.
Stellar Mass Function (50 kpc aperture) with Eddington bias with extended ranges
50 kpc aperture GSMF, showing all galaxies with a fixed bin-width of 0.2 dex. Includes Eddington bias.
Stellar Mass-Halo Mass relation (ratio, 100 kpc aperture, centrals only)
Includes only central haloes.
Stellar Mass-Halo Mass relation (ratio, 100 kpc aperture, centrals only, stellar x-axis)
Includes only central haloes.
Stellar Mass-Halo Mass relation (ratio, 50 kpc aperture, centrals only)
Includes only central haloes.
Stellar Mass-Halo Mass relation (ratio, 50 kpc aperture, centrals only, stellar x-axis)
Includes only central haloes.
Stellar Mass-Halo Mass relation (ratio, 30 kpc aperture, centrals only)
Includes only central haloes.
Stellar Mass-Halo Mass relation (ratio, 30 kpc aperture, centrals only, stellar x-axis)
Includes only central haloes.
Stellar Mass-Halo Mass relation (100 kpc aperture, M$_{\rm BN98}$)
Includes all haloes, including subhaloes.
Stellar Mass-Halo Mass relation (50 kpc aperture, M$_{\rm BN98}$)
Includes all haloes, including subhaloes.
Stellar Mass-Halo Mass relation (30 kpc aperture, M$_{\rm BN98}$)
Includes all haloes, including subhaloes.
Stellar Mass-Halo Mass relation (100 kpc aperture, centrals only, M$_{\rm BN98}$)
Includes only central haloes.
Stellar Mass-Halo Mass relation (50 kpc aperture, centrals only, M$_{\rm BN98}$)
Includes only central haloes.
Stellar Mass-Halo Mass relation (30 kpc aperture, centrals only, M$_{\rm BN98}$)
Includes only central haloes.
Stellar Mass-Halo Mass relation (ratio, 100 kpc aperture, $M_{\rm BN98}$, centrals only, stellar x-axis)
Includes only central haloes.
Stellar Mass-Halo Mass relation (ratio, 50 kpc aperture, $M_{\rm BN98}$, centrals only, stellar x-axis)
Includes only central haloes.
Stellar Mass-Halo Mass relation (ratio, 30 kpc aperture, $M_{\rm BN98}$, centrals only, stellar x-axis)
Includes only central haloes.
Stellar Mass-Halo Mass relation (ratio, 100 kpc aperture, $M_{\rm BN98}$, centrals only)
Includes only central haloes.
Stellar Mass-Halo Mass relation (ratio, 50 kpc aperture, $M_{\rm BN98}$, centrals only)
Includes only central haloes.