

The Planck Sky Model (PSM) is a complete and versatile set of programs and data, to be used for the simulation or the prediction of sky emission in the frequency range of typical CMB experiments, and in particular of the upcoming Planck sky mission. It has originally been developed as part of the activities of Planck component separation Working Group (or 'Working Group 2' - WG2), and of the ADAMIS team at APC.
The PSM software is developed with two main objectives in mind:
The model has has been developed mostly by members of the Planck collaboration as a simulation tool for Planck activities. The current version is "pre-launch", with no Planck observation used to model sky emission. There is, hence, no guaranteee that simulated maps obtained with the PSM will be fully compatible with Planck observations. Updating the model on the basis of Planck observations is one of the projects of the Planck collaboration (Project 1.11: Planck Sky Model ).
The software is developed mostly in the IDL programming language. It uses the HEALPix sky-pixellisation package (with calls to C++ binaries), the astron and mpfit libraries, and uses CAMB for specific CMB models. The package comes as a collection of component-specific simulation codes put together by driver routines, automating fastidious tasks like parameter processing and component map coaddition.
The PSM is being continuously developed. Visit the web site regularly for releases of simulation products and of the software package.
Global coordination and scientific responsibility
Package coordination
Main developers and contributors
The following people have contributed to the PSM project so far:
Acknowledgements
Beta-testers
The following releases of the PSM are available for download. The status specifies whether the release is RESTRICTED to the Planck collaboration, or OPEN to the scientific community at large. Check the appropriate release page for additional information about each particular release: general comments, limitation and known bugs, specific recommendations.
The OPEN releases are made available under the terms of the GNU General Public License as published by the Free Software Foundation (version 3 of the license, or any later version at the user option).
The current RECOMMENDED VERSION is v1.7.4.
| Date | Release page | Comments | Download user manual in pdf format | Status |
|---|---|---|---|---|
| 21 March 2012 | v1.7.5 | This is a minor update of v1.7.4. It tags specifically the version used for the observation of FFP4 simulations in average FFP4 frequency bands. The available RIMOs have been modified (temporarily; they probably need a complete revision). A new feature is a model of galactic magnetic field according to Fauvet et al. 2011, that can be used to generate templates of polarised galactic emission. | PSM_user_manual_v1_7_5.pdf | RESTRICTED |
| 16 March 2012 | v1.7.4 | Version essentially fixing bugs introduced in version 1.7.3: Corrected dust polarisation amplitude, fixed bugs for Gaussian CMB (which has been improved and tested more thoroughly). Also expanded the documentation, implemented relativistic SZ effect included for some SZ models, and updated the radio-frequency part of ultra-compact HII regions. Used for generating v2 of the FFP4 diffuse foregrounds. | PSM_user_manual_v1_7_4.pdf | RESTRICTED |
| 04 December 2011 | v1.7.3 | Version updated and released specifically for Planck FFP4 simulations. Not recommended (tested only for very limited configurations). | PSM_user_manual_v1_7_3.pdf | RESTRICTED |
| 28 September 2011 | v1.7.2 | This version is a minor update of v1.7.1. | PSM_user_manual_v1_7_2.pdf | RESTRICTED |
| 13 September 2011 | v1.7.1 | This version updates some templates for the Galaxy, corrects high multipole galactic emission and fixes a few minor bugs in v1.7.0-beta. | PSM_user_manual_v1_7_1.pdf | RESTRICTED |
| 25 August 2011 | v1.7.0-beta | This version is a major revision of the PSM, released internally to the Planck collaboration for beta-testing. | PSM_user_manual_v1_7_0-beta.pdf | RESTRICTED |