HEALPix maps¶
The FLAMINGO simulation lightcone outputs include full-sky projected maps of particle properties (such as mass or x-ray luminosity) in concentric spherical shells around each observer. When a particle crosses the observer’s lightcone we determine which radial shell it is in and accumulate its contribution to the appropriate maps.
These maps use the HEALPix pixelisation scheme to divide the sky into pixels of equal area. The maps are provided at two resolutions. The highest resolution maps have an angular resolution of about 13 arcseconds (\(N_\mathrm{side}=16384\)). Since these large maps can be difficult to work with, we also provide down-sampled maps with an angular resolution of about 50 arcseconds (\(N_\mathrm{side}=4096\)).
Projected gas mass in 10 concentric spherical shells around an
observer in the L1_m8 simulation. The observer is at the
centre of the sphere. The outer sphere has a comoving radius of
approximately 2 Gpc. The full FLAMINGO outputs consist of
68 shells with a maximum
comoving radius of 7.9 Gpc (\(z = 5\)).
Mollweide projected full sky map of the thermal Sunyaev-Zel’dovich effect as quantified by the Compton y parameter for the redshift interval \(0 < z < 0.05\).
HEALPix maps of a range of physical quantities are available. For more information see the documentation links below and appendix A of Schaye et al (2023).
- Directory layout
- File format
- Shell redshifts
- Map descriptions
- Reading the maps
- Integrated lightcones
- Rotations
- Weak lensing convergence maps
- ROSAT convolved X-ray All-Sky maps
- AGN Point Source Maps
- Integrated Thermal SZ Maps
- Integrated Kinetic SZ Maps
- Integrated Relativistically Corrected Thermal SZ Maps
- Integrated Cosmic Infrared Background Maps
- Integrated Radio Point Source Maps
- Integrated Anisotropic Screening (optical depth \(\tau\)) Maps