**Maps**:

CAR maps at 0.04 arcminute resolution on an 11 degree by 11 degree patch of sky, centered at right ascension = 6 degrees and declination = 6 degrees. All except the lensing convergence map are in units of uK and convolved with the pixel window function. In the file names, `{FREQ}` is a placeholder for `030`, `090`, `148`, `219`, `277`, or `350` GHz.

- Lensed CMB T, Q, U maps: `cmbTQU0058_pixwin_11x11deg.fits`
- Unlensed CMB T, Q, U maps: `unlensed_cmbTQU0058_pixwin_11x11deg.fits` 
- Lensing convergence (kappa) map: `kappa_11x11deg.fits`
- kSZ map: `ksz_11x11deg.fits`
- tSZ maps at each frequency: `{FREQ}_tsz_pixwin_11x11deg.fits`
- CIB maps at each frequency: `{FREQ}_cib_pixwin_11x11deg.fits`
- Radio maps at each frequency: `{FREQ}_radio_pixwin_11x11deg.fits`
- Combined maps of kSZ, tSZ, CIB, radio + lensed CMB temperature (no polarization) at each frequency: `{FREQ}_cmbT0058_tsz_ksz_radio_cib_pixwin_11x11deg.fits`


**Catalogs**:

Catalogs of the CIB galaxies, radio galaxies, and SZ clusters within the simulated 121 square degree region.

- `cib_11x11deg.csv` : Catalog of CIB source positions (right ascension and declination, in degrees) and fluxes (in mJy) at 30, 90, 148, 219, 277, and 350 GHz
- `radio_11x11deg.csv` : Catalog of radio source positions (right ascension and declination, in degrees), redshifts, and fluxes (in mJy) at 1.4, 30, 90, 148, 219, 277, and 350 GHz
- `sz_11x11deg.csv` : Catalog of SZ clusters ; see https://lambda.gsfc.nasa.gov/simulation/full_sky_sims_readme_sz.html for a complete description


**Power spectra**:

Power spectra of the inner 100 square degree region of the lensed CMB (temperature and polarization), lensing convergence, kSZ, tSZ, CIB, and radio maps. The lensing convergence power spectrum is dimensionless; all other power spectra have units of uK^2. 

All maps are apodized along their edges over a 0.5 degree region before taking their power spectra, and the CAR pixel window is deconvolved from the CMB, kSZ, tSZ, CIB, and radio maps. The power spectra are then binned (using a uniform bin width of 200 and a maximum multipole of 21,000) and corrected for the mode-coupling induced by the apodization mask.

Files that end in `_cls.txt` contain power spectra as C_ell’s, i.e., not multiplied by any multipole, etc. factors. Files that end in `_dls.txt` contain power spectra as D_ell's, i.e., the C_ell's multiplied by ell * (ell + 1) / 2 * pi at each multipole ell before binning. In the file names, `{FREQ}` is a placeholder for `030`, `090`, `148`, `219`, `277`, or `350` GHz.

For the lensed CMB power spectra, the columns in the file are the binned multipoles and the binned TT, EE, BB, and TE power spectra. All other files contain two columns: the binned multipoles, and the binned power spectrum.

- `cmbTQU0058_cls.txt` and `cmbTQU0058_cls.txt`: Lensed CMB temperature and polarization power spectra
- `kappa_cls.txt`: Lensing convergence power spectrum
- `ksz_cls.txt` and `ksz_dls.txt`: kSZ power spectrum
- `{FREQ}_tsz_cls.txt` and `{FREQ}_tsz_dls.txt`: tSZ power spectrum at each frequency
- `{FREQ}_cib_cls.txt` and `{FREQ}_cib_dls.txt`: CIB power spectrum at each frequency
- `{FREQ}_radio_cls.txt` and `{FREQ}_radio_dls.txt`: radio power spectrum at each frequency