Planck Public Data Release 3 Mission Ancillary Data
This page contains cosmological parameters, likelihoods, power spectra, noise covariance matrices, polarization leakage corrections maps, beams, instrument models, mask files, planet intensities and dates on which positions on the sky were observed. In addition, a listing of all PR3 data products is provided. Planck mission products and the observation date files are described in the resources listed on the Planck documentation page.
A description of the HEALPix map format and a suite of software tools are available at the HEALPix site, http://healpix.sourceforge.net.Cosmology Data
Data set | Notes | Cosmological Parameters | Mean cosmological parameters with confidence intervals from Planck (download) |
Base Parameters Base Power Spectrum TT, binned TT, unbinned TE, binned TE, unbinned EE, binned EE, unbinned BB | Power spectra | Cosmological Parameters: Full Grid | Zip file with full-grid of likelihoods for cosmological parameters (11 GB) | CosmoParams_lensonly_R3.01 | LCDM Parameters from Planck lensing reconstruction only (1.1 GB) | CosmoParams_base-plikHM_R3.01 | LCDM parameters from temperature and polarization (PLIK cross Half-mission; 30 ≤ l ≤ 2500), with various combinations of low-L data (471 MB) | CosmoParams_base-plikHM-TTTEEE-lowl-lowE_R3.00 | LCDM parameters using the baseline likelihoods (PLIK, cross Half-mission, with 30≤l≤2508 in TT and 30≤l≤1996 for TE and EE, including lensing, cleaned HFI low-l (2<l<29) (63 MB) | COM_CosmoParams_base-plikHM-zre6p5_R3.01 | LCDM parameters with hard priors on redshift of reionization z_re>6.5 (267 MB) |
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Noise Covariance Matrices: 030 044 070 | NSIDE=16 tarfiles, 1 per frequency. File sizes are 2.5GB. |
Simulations of CMB Maps (External link to NERSC) | CMB simulation data available from NERSC |
Product Lists
The data products supplied in PR3 are listed in two sets, the first for those derived from LFI data only, and the second for those either based on HFI data or the combination of LFI and HFI data.
Product type | Format | LFI | HFI |
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All Sky Maps | HEALPix maps | ✔ | ✔ |
Multi-frequency Catalog of Non-thermal Sources | FITS binary table | ✔ | |
Correction Maps | HEALPix maps | ✔ | ✔ |
Noise Covariance Matrices | HEALPix maps | ✔ | |
Source Masks | HEALPix maps | ✔ | ✔ |
NPIPE All Sky Maps | HEALPix maps | ✔ | ✔ |
Planck Instrument Models
Reduced Instrument Model (RIMO): LFI; HFI | Includes effective frequencies and throughputs |
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HFI_RIMO_Beams | HFI Beam Window Functions |
Correction Maps
Data set - check this later | Notes |
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LFI File List LFI Download | Correction maps in HEALPix format for the LFI Frequencies. Need to be applied to frequency maps. |
HFI File List HFI Download | Correction has already been applied to frequency maps. Corrections maps are in matrix below. |
Planck HFI Bias Maps | ||||
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HFI | ||||
Frequency (GHz) | 100 | 217 | 353 | |
CO noise ratio | 100 | 217 | 353 | |
CO nominal | 100 | 217 | 353 | |
CO signal ratio | 100 | 217 | 353 |
Foreground Masks
Data set | Notes |
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COM_Mask_CMB-common-Mask-Int_2048_R3.00 | 2018 Component Separation Common mask in Intensity. |
COM_Mask_CMB-common-Mask-Pol_2048_R3.00 | 2018 Component Separation Common mask in Polarization. |
COM_Mask_CMB-HM-Misspix-Mask-Int_2048_R3.00 | 2018 Component Separation Half Mission Missing Pixels mask in Intensity. |
COM_Mask_CMB-HM-Misspix-Mask-Pol_2048_R3.00 | 2018 Component Separation Half Mission Missing Pixels mask in Polarization. |
COM_Mask_CMB-Inpainting-Mask-Int_2048_R3.00 | 2018 Component Separation Inpainting Common mask in Intensity. |
COM_Mask_CMB-Inpainting-Mask-Pol_2048_R3.00 | 2018 Component Separation Inpainting Common mask in Polarization. |
COM_Mask_CMB-OE-Misspix-Mask-Int_2048_R3.00 | 2018 Component Separation Odd-Even Missing Pixels mask in Intensity. |
COM_Mask_CMB-OE-Misspix-Mask-Pol_2048_R3.00 | 2018 Component Separation Odd-Even Missing Pixels mask in Polarization. |
COM_Mask_Likelihood-polarization-100-hm1_2048_R3.00 | 2018 mask used in the Plik likelihood for the Half-mission 1 (HM1) Q and U polarization maps at 100 GHz. |
COM_Mask_Likelihood-polarization-100-hm2_2048_R3.00 | 2018 mask used in the Plik likelihood for the Half-mission 2 (HM2) Q and U polarization maps at 100 GHz. |
COM_Mask_Likelihood-polarization-143-hm1_2048_R3.00 | 2018 mask used in the Plik likelihood for the Half-mission 1 (HM1) Q and U polarization maps at 143 GHz. |
COM_Mask_Likelihood-polarization-143-hm2_2048_R3.00 | 2018 mask used in the Plik likelihood for the Half-mission 2 (HM2) Q and U polarization maps at 143 GHz. |
COM_Mask_Likelihood-polarization-217-hm1_2048_R3.00 | 2018 mask used in the Plik likelihood for the Half-mission 1 (HM1) Q and U polarization maps at 217 GHz. |
COM_Mask_Likelihood-polarization-217-hm2_2048_R3.00 | 2018 mask used in the Plik likelihood for the Half-mission 2 (HM2) Q and U polarization maps at 217 GHz. |
COM_Mask_Likelihood-temperature-100-hm1_2048_R3.00 | 2018 mask used in the Plik likelihood for the Half-mission 1 (HM1) intensity map at 100 GHz. |
COM_Mask_Likelihood-temperature-100-hm2_2048_R3.00 | 2018 mask used in the Plik likelihood for the Half-mission 2 (HM2) intensity map at 100 GHz. |
COM_Mask_Likelihood-temperature-143-hm1_2048_R3.00 | 2018 mask used in the Plik likelihood for the Half-mission 1 (HM1) intensity map at 143 GHz. |
COM_Mask_Likelihood-temperature-143-hm2_2048_R3.00 | 2018 mask used in the Plik likelihood for the Half-mission 2 (HM2) intensity map at 143 GHz. |
COM_Mask_Likelihood-temperature-217-hm1_2048_R3.00 | 2018 mask used in the Plik likelihood for the Half-mission 1 (HM1) intensity map at 217 GHz. |
COM_Mask_Likelihood-temperature-217-hm2_2048_R3.00 | 2018 mask used in the Plik likelihood for the Half-mission 2 (HM2) intensity map at 217 GHz. |
Effective Beams
Data set | Acknowledgements | Notes |
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Effective Beams | S. Mitra et al. 2011. Fast Pixel Space Convolution for Cosmic Microwave Background Surveys with Asymmetric Beams and Complex Scan Strategies: FEBeCop | Unformatted Planck effective beams by sky position and frequency for use with EffConv. These are based on processing the full mission data while those for PR1 were only based on the nominal mission data. |