You are here: Site Map
Site Map

Home

Grand public

Quelques ordres de grandeur de distances
Lexique général
Astronomie
Unités
Cosmologie
Électromagnétisme
Personnes
Physique générale
Relativité
La constante de Hubble
Que signifie exactement « L’univers est en expansion » ?
Le concept de distance dans un univers en expansion
L’univers est-il fini ou inifini ? A-t-il une « taille » ?
Le devenir de l’expansion de l’univers
L’histoire thermique de l’univers
Jusqu’à quelle époque peut-on remonter ?
Le fond diffus cosmologique
Pourquoi la nuit est-elle noire ?
Qu’est-ce qu’un horizon ?
La répartition de la matière dans l’univers
Quelles formes de matière existent aujourd’hui dans l’univers ?
Effet Doppler sonore et lumineux
Spectre électromagnétique
Spectres d’émission et d’absorbtion
Spectre de corps noir
L’échelle de luminosité apparente des objets astrophysiques
Effet Doppler - cas classique
Comment déterminer que la force de gravitation est proportionnelle à l’inverse du carré de la distance ?
Effet Doppler - cas relativiste
Retour sur le paradoxe d’Olbers
Les distances dans un univers en expansion
L’expansion de l’univers - un exemple Newtonien
L’expansion de l’univers - les équations de Friedmann
Comment l’expansion augmente-t-elle les distances sans dilater les objets ?
Pourquoi une constante cosmologique agit-elle comme une force répulsive ?
Expansion éternelle ou Big Crunch ?
La température de l’univers au cours de son évolution
La présence d’horizons dans l’univers selon son évolution
Le principe de relativité galiléenne et la mécanique classique
La gravitation universelle selon Newton
Un peu de Relativité Restreinte
Un peu de Relativité Générale

Science

What is the CMB and why is it useful
Maps and spectra
The physics behind what is observed
The present lore: the minimal cosmological model
The physics of CMB peaks - I. Influence of the baryon density
The physics of CMB peaks - II. Influence of the Dark Matter density
The physics of CMB peaks - III. Influence of what happens after recombination
The "initial conditions": The predictions from inflation
Why peaks?
Matter content of the universe
First order polarisation at reionisation
Temperature anisotropies at reionisation
Second order polarisation
Temperature anisotropies
ISW effect
RS effect and moving sctructures
Polarisation from galaxy clusters
Kinetic SZ and peculiar velocities
SZ parameters and relativistic corrections
The catalogue
The clustering properties
Dust emission in molecular clouds and star forming regions
Dust emission in the diffuse interstellar medium
The foreground X
The Free-Free Emission
The large-scale structure of the Milky-way
The synchrotron radiation
Dust polarization
The synchrotron in polarisation
Cold cores
HII regions
Dust grains
Laboratory measurements of dust properties
Theoritical developpements
Synchrotron

Instrument

News items

Horns @ 100 GHz
Polarisation Sensitive Bolometers
Spiderweb bolometers
Sensitive Thermometer
Instrument Working Group #13 - 5/6 January 2006
Calibration Report
COLDS thermometry graphs (CQM, cryotests)
Optical setup thermometers and PIOLIB
Saturne Parameter Names and RtaCalibration
FTS and sources design
FTS specifications
Data Acquisition and Quick Look Analysis : Instruction for CSL Computers
HFI CQM thermometers and PIOLIB
Calibration Data
Calibration meeting - December 13 2004
Calibration workshop - April 5-6 2005
HFI CQM calibration report
Intermediate results
IQR kick-off
IWG 2005 January 24-25 in Orsay
LongTrend Calibration Data
Bolometer balance
CESR Presentation RU Flow
HFI RU
Horloge REU
LAL contributions
VI Measurement
LG Action
Example of calibration sequence
Old Livelink documents
Local documents
HFI Transfer Function
Names from L1
Get and Install QLA
Get and Install the PIOLib
KST : Get, Install, Use
Browse CVS
Databases List
Get and Install all
How to acces ground tests data?
QLA computers
QLA_scripts_list
X-Win32
HFI Receiver Model
Spire Bolo_software
Calibration sequences
DPU compression algorithm
News
PFM calibration run performed schedule
1stRunCAR_Calibration 2006_03
PFM calib run : facility data
PFM Calib Run: Noise and Response Analysis
Calibration bolometers
Cold sources
Instrumented wheel
Integration with HFI CQM
Optical setup
Saturne
Focal Plane Unit

Operations

Data Processing

People/Contacts
Other links
What is L2
L2 Mailing lists
Level-S interface meeting
Novelty meeting (Toulouse, FRB, CM, JPB)
L2 monthly meeting at IAP
Component Separation WG: coordinators kickoff meeting (Padova)
LFI Consortium meeting (Rindberg Castle, D)
Cluster & Secondaries Anisotoripies WG coordinators kickoff meeting (Garching)
HFI Consortium meeting (Cardiff, UK)
L2 monthly meeting (IAP)
Massive Datasets WG kickoff meeting (IAP)
Systematic Effects WG coordination meeting
L2 Monthly meeting (IAP)
Planck Science Team (ESTEC)
L2 Monthly Meeting
Special L3/L2 meeting at IC-London
DPC-L2: March Monthly Meeting
Pipeline integration meeting @ IAS
Pipeline integration meeting
L2 Monthly/Integration Meeting at IAP: pipeline integration
HFI/LFI Consortium Meeting @ Santander
L2 Monthly Meeting at IAP: final preps for DPC Review
Pictures
L2 Monthly Meeting at IAP: 1,2D GUIs, Noveltis, Astrometry
L2 Monthly Meeting at IAP: PIOlib, LS2L2, hands-on
L2 Monthly Meeting at IAP: Joint MIG, Calib, SEWG meeting
GPH424 - Mapmaking - coordination meeting
L2 Monthly Meeting at IAP: Science and algorythms
L1/L2/Cal/SEWG/MIG Meeting
L2 Monthly Meeting at IAP: Integration, hands-on
PISTOU acceptance meeting with NOVELTIS
DPC-L2 Monthly Meeting
Porquerolle Island Meeting
Joint L2/L3 Meeting at IAP
Breadboard Model Acceptance
2nd Planck Symposium @ Orsay
Dataflow meeting #1
Integration Meeting #1
Integration Meeting #2
Dataflow Meeting #2
Integration Meeting #3
Dataflow (mini) Meeting #4
Dataflow Meeting #5
Integration Meeting #4
Dataflow (mini) Meeting #7 (TBC)
Integration Meeting #5
IAS Meeting
Integration Meeting #6
L2 Meeting Apr04
PGSSG meeting
DPC Review
Integration Meeting #7
Integration Meeting #8
L2 Meeting Jun.04
IAP Coll. Jul04
Goutelas Sep04
L2 Meeting Oct.04
L2 Meeting - 9.Dec.04
L2 - 05.Jan.05
Planck Consortium
L2 - 17.Feb.05
L2 - 22.Mar.05
L2 - 21.Apr.05
L2 - Jun.05
L2 - Oct.05
L2 - Nov.05
L2 - Dec 05
L2 Feb 06
L2 Mar 06
Jun 06
Core Team at IAP
Ecole Planck à Cargèse
Core Team
Benchmark validation
Tags announce
Package creation
Browse CVS repository
Browse Releases
Browse Pipelines
Introduction
Overview of the L2
The L2 development environment
Guidelines for developers
CVS and CMT summary
The HFI-DMC
ThinC
Supported libraries
Infrastructure support (FAQ)
Other useful documents
MapCUMBA
COLIBRI
Installing Proc locally
Pointing Library
PolSpice
ThinC
PIOlib Overview
C Reference
C++ Reference
F90 Reference
IDL Reference
PIOLIB Tools
Admin Database
Database User Guide
DDL specification
DDL.xsd
DMC
DMC queries GUI
Download
HFI-DMC Development
IMO
MetaDB
Module Definition
PIOLIB installation
Pipeline and module configuration
Pipeline and Module Run
Pipeline Definition
Proposed query list
ReleaseData
Transfer Function test and debug
V02-01-03 test report
Pistou Home
screen shots
ccIn2p3 how-to
Definitions and conventions
Documentation
Presentations
SimIns
Simulations for DM development and testing
Compilation environments
Magique II Batch Queue System
magique II description
magique II latest news
magique II monitoring commands
The cc-in2p3
Getting help with magique III
Getting started with magique III
magique III Batch Queue System
magique III hardware brief introduction
magique III latest news
magique III performance
magique III software
Monitoring your jobs with magique III
Monthly reports
Past documents
Teleconf summaries
CVS Package Documentation kit
Updating External Sites
What is Level 3?
People
Links
HFI DPC Internal Review, March 2004

Core Team

2009/09/09 CT#22 @ IAP
2009/01/05 CT#18 @ IAP
2008/03/13-14 CT#13@IAP
2008/01/10-11 CT#12@IAS
2007/11/5-9 Joint CT#1@Bologna
2007/09/13-14 CT#10@IAP
2007/06/14-15 CT#09@IAP&IAS
2007/04/12-13 CT#08@Alcatel-Cannes
2007/02/15-16 CT#07@IAS
2006/11/16-17 Planck Calibration Workshop @ ESTEC
2006/12/11-12 CT#06@IAP
2006/09/28-29 CT#05@IAS
2006/06/01-02 CT#03@IAS
2006/03/30-31 CT#02@IAS
Task list
Calibration report
HFI SVR - TCR report
CSL FM
Analyzing Pointing Simulations
Main beams from F. Noviello
Main beams from J. Brossard
CTWG3 Actions
CTWG3 Calibration Results
CTWG3 Introduction
CTWG3 Links
CTWG3 Peoples
CTWG3 Reference Documents
CTWG3 related Meetings
All pixels spectral response (version 1.01).
First sample of Spectra.
Relative photometric pixel gain depending on the color of the incident spectrum
CTWG9 CTA7 meeting, May 2008
CTWG9 News
CTWG9 people
hold a meeting !
Material of interest

Hosted sites

Simulations
WG2 grand challenge: first results
Guidelines for producing component models
Gaussian CMB
Non-Gaussian CMB
Sunyaev-Zel’dovich Effect
Galactic Diffuse Emission
Point Sources
2003 Nov 24-25 Coordinators Meeting at IAP
2004-07-3 Meeting @ IAP
Meeting November 2005 at IAP
2002 Feb 4 & 5 - coordination meeting
Planck Working Sub-group 6.4: Follow-up with HERSCHEL.
Planck Working Sub-group 6.5: Simulations of Compact Source Fields and Cosmic Background.
November 25-26, 2002 Meeting.
Simulations of Planck HFI fields
Simulations of Herschel PACS and SPIRE fields
Images of Planck HFI Mock Maps
Paris-Orsay CMB Seminar Series
CMBNET Large Dataset Analysis Meeting
Inscription en ligne
Bulletin numero 1
Bulletin numero 2
Programme
Informations pratiques
Inscriptions à l’école Planck de Cargese
Les présentations
Les photos de François Pajot
Les photos de Hervé Dole
Les photos de Nicolas Ponthieu