General description

As of March 2025, CAMELS host more than 2 petabytes of data from 16,960 cosmological simulations: 7,208 N-body and 9,752 hydrodynamic simulations. This project is the result of a large, collaborative effort and represents the most extensive suite of cosmological hydrodynamic simulations ever conducted.

The simulations are run with different codes (suites), cover different volumes and number of particles (generations), and sample different points in parameter space (sets), defined as the space formed from cosmological and astrophysical parameters and different initial conditions.

All CAMELS simulations share a few characteristics:

  • All simulations start at redshift \(z=127\) and finish at \(z=0\).

  • All simulations have the same mass and spatial resolution.

  • For each simulation we store multiple snapshots, halo/subhalo catalogs, and summary statistics (e.g. power spectra) see Data organization.

  • The N-body simulations only model the spatial phase-space distribution of total matter under the influence of gravity.

  • The hydrodynamic simulations account for gravity + (magento-)hydrodynamics + astrophysical processes (e.g. supernova and AGN feedback).

Organization

The simulations can be classified into:

  • Suites: depending on the code and subgrid physics model used to run them. CAMELS has 9 suites:

Suite

Code

Subgrid Physics Model

IllustrisTNG

AREPO

IllustrisTNG

SIMBA

GIZMO

SIMBA

Astrid

MP-Gadget

Astrid

Magneticum

OpenGadget

Magneticum-like

Swift-EAGLE

Swift

EAGLE

Ramses

Ramses

Enzo

Enzo

CROCODILE

Gadget4-Osaka

CROCODILE

Obsidian

GIZMO

Obsidian

  • Generations: depending on the volume and number of particles in the simulations. CAMELS has 3 generations:

Generation

Description

First generation

\(256^3\) dark matter + \(256^3\) initial fluid elements in a 25 Mpc/h box

Second generation

\(512^3\) dark matter + \(512^3\) initial fluid elements in a 50 Mpc/h box

Third generation

\(1024^3\) dark matter + \(1024^3\) initial fluid elements in a 100 Mpc/h box

  • Sets: depending on how their cosmological and astrophysical parameters, and initial random seed values are organized. CAMELS has 6 sets:

Set

Description

SB

Variations in cosmology, astrophysics, and initial conditions

LH

Variations in cosmology, astrophysics, and initial conditions

1P

Variations on a single cosmological or astrophysical parameter. Initial conditions fixed

CV

Fixed cosmology and astrophysics. Variations in initial conditions

EX

Fixed cosmology and initial conditions. Extreme variations in astrophysics

BE

Fixed cosmology, astrophysics, and initial conditions

See Organization for further details.

Simulations available

The tables below shows the number of available hydrodynamic and N-body simulations:

First generation hydrodynamic simulations

Set

Suite

SB

LH

1P

CV

EX

BE

Total

IllustrisTNG

2048

(28 params)

1000

(6 params)

113

(28 params)

27

4

27

3219

SIMBA

1000

(6 params)

113

(28 params)

27

4

27

1171

Astrid

1024

(7 params)

1000

(6 params)

25

(6 params)

27

4

2080

Magneticum

50

(6 params)

27

77

Swift-EAGLE

1000

(6 params)

25

(6 params)

27

1052

Ramses

512

(5 params)

13

(5 params)

27

552

Enzo

5

1

6

CROCODILE

128

(6 params)

25

(6 params)

27

180

Obsidian

27

27

All

3712

4050

319

217

12

54

8364

Second generation hydrodynamic simulations

Set

Suite

SB

1P

CV

EX

BE

Total

IllustrisTNG

1024

(35 params)

141

(35 params)

27

1192

SIMBA

Astrid

Magneticum

Swift-EAGLE

Ramses

21

(5 params)

27

48

Enzo

CROCODILE

16

105

(26 params)

27

148

Obsidian

All

1040

267

81

1388

First generation N-body simulations

Set

Suite

SB

LH

1P

CV

EX

BE

Total

IllustrisTNG

2048

(5 params)

1000

(2 params)

9

(5 params)

27

1

27

3112

SIMBA

1000

(2 params)

1064

Astrid

1024

(3 params)

1000

(2 params)

2088

Magneticum

64

Swift-EAGLE

64

Ramses

64

Enzo

64

CROCODILE

64

Obsidian

64

All

3072

3000

9

27

1

27

6136

Second generation N-body simulations

Set

Suite

SB

1P

CV

EX

BE

Total

IllustrisTNG

1024

(5 params)

21

(5 params)

27

1072

SIMBA

Astrid

Magneticum

Swift-EAGLE

Ramses

Enzo

CROCODILE

Obsidian

All

1024

21

27

1072

Note

CAMELS is designed so that each hydrodynamic simulation has a N-body counterpart. However, several hydrodynamic simulations may have the same N-body simulation. For instance, in the 1P set, simulations that only vary astrophysical parameters, will have the same N-body counterpart. This is the reason why in the above table, the number of N-body simulations may be lower than the corresponding number of hydrodynamic simulations.

The value of the cosmological, astrophysical, and initial random seed of the different simulations can be found Parameters.

Codes

All N-body simulations have been run with the Gadget-III code, while the hydrodynamic simulations have been run with different codes: AREPO, GIZMO, MP-Gadget, OpenGadget, Swift, Ramses, Gadget4-Osaka, and Enzo. See Codes for details on the different codes and subgrid physics models available in CAMELS.

Redshifts

Important

A reorganization of the data was performed in 2024 in order to enhance its uniformity and simplicity. This will require slight changes to existing codes that access the data.

  • Snapshot numbers in the IllustrisTNG and SIMBA suites, where simulations have only 34 snapshots, have been updated to match the numbering in the Astrid suite (and some TNG simulations) that have 91 snapshots. For example, where 33 used to be the z=0 snapshot, now it is 90 uniformly for all suites.

All simulations have 91 snapshots. This file contains the scale factors of the snapshots. The user can click below to see the redshift, scale factor, and snapshot number for the different snapshots:

Click here to see the relation between the snapshot number and the redshift

Redshift

Scale Factor

34 snapshots

91 snapshots

14.99

0.063

000

13.34

0.070

001

11.98

0.077

002

11.20

0.082

003

10.48

0.087

004

9.69

0.094

005

9.00

0.100

006

8.49

0.105

007

8.01

0.111

008

7.60

0.116

009

7.24

0.121

010

6.89

0.127

011

6.56

0.132

012

6.28

0.137

013

6.01

0.143

000

014

5.75

0.148

015

5.50

0.154

016

5.23

0.161

017

5.00

0.167

001

018

4.80

0.172

019

4.61

0.178

020

4.45

0.183

021

4.30

0.189

022

4.15

0.194

023

4.01

0.200

002

024

3.87

0.205

025

3.73

0.211

026

3.62

0.216

027

3.49

0.223

003

028

3.36

0.229

029

3.24

0.236

030

3.12

0.242

031

3.01

0.249

004

032

2.90

0.257

033

2.80

0.263

005

034

2.72

0.269

035

2.63

0.276

006

036

2.54

0.282

037

2.46

0.289

007

038

2.38

0.296

039

2.30

0.303

008

040

2.22

0.310

041

2.15

0.318

009

042

2.07

0.325

043

2.00

0.333

010

044

1.93

0.341

045

1.86

0.349

011

046

1.80

0.358

047

1.73

0.366

012

048

1.67

0.375

049

1.60

0.384

013

050

1.54

0.393

051

1.48

0.403

014

052

1.43

0.412

053

1.37

0.422

015

054

1.30

0.434

055

1.26

0.443

016

056

1.20

0.455

057

1.14

0.466

017

058

1.09

0.478

059

1.05

0.489

018

060

1.00

0.501

061

0.95

0.513

019

062

0.90

0.525

063

0.86

0.538

020

064

0.82

0.550

065

0.77

0.564

021

066

0.73

0.577

067

0.69

0.591

022

068

0.65

0.605

069

0.61

0.620

023

070

0.58

0.635

071

0.54

0.650

024

072

0.50

0.665

073

0.47

0.681

025

074

0.43

0.698

075

0.40

0.714

026

076

0.37

0.731

077

0.34

0.749

027

078

0.30

0.771

079

0.27

0.789

028

080

0.24

0.808

081

0.21

0.827

029

082

0.18

0.847

083

0.15

0.867

030

084

0.13

0.888

085

0.10

0.910

031

086

0.07

0.931

087

0.05

0.954

032

088

0.02

0.977

089

0.00

1.000

033

090


Note

The exact redshifts of a given snapshot may be slighty different to the above ones. For instance, there are small differences between the exact redshifts of the snapshots in the Astrid and SIMBA suites. In the simulations of the IllustrisTNG suite these numbers can also be slightly different, since AREPO can only write snapshots in the highest time steps in the hierarchy.

Warning

We have moved some snapshots to tape. If you need these please reach out.