Planck-Euclid


Overview

The Planck satellite was a European Space Agency (ESA) survey mission to measure the anisotropy and polarization of the cosmic microwave background (CMB) radiation. Planck was launched on May 14th, 2009 and ceased operations on October 23rd, 2013. The analysis of the full set of data and the derivation of the scientific results of the mission is still in progress. The first major Planck data release was in March 2013, the second one was in February-July 2015, and the final results are to be published in 2017.

The CMB is radiation from the early universe. It was emitted when the universe was about 400 000 years old. Its intensity and polarization varies over the sky, and these variations reflect the properties and structure of the early universe as well as the later history of the universe through which this radiation has traveled.

We have developed data analysis methods for Planck, and participate in analyzing the Planck data and in preparing the scientific publications from Planck.

Euclid is the next ESA cosmology satellite, to be launched in December 2020. It will photograph over one third of the sky in visible and near-infared wavelengths, obtaining images of over a billion galaxies and spectra of tens of millions of galaxies. Using the redshifts of galaxies and the distortion of galaxy images caused by gravitational lensing by the intervening matter, Euclid will produce a 3-dimensional map of the distribution of visible and dark matter over a sizable part of the observable universe. The main goal of Euclid is to help solve the Dark Energy Problem: What is causing the acceleration of the expansion of the universe - is it a new form of energy, called dark energy, or does gravity deviate at cosmological distances from Einstein's theory of General Relativity.

Finland provides one of the nine Euclid Science Data Centers, the SDC-FI. This is based on virtual machines running on CSC's Pouta Cloud Service. We participate in producing simulated Euclid data and in developing data analysis methods for Euclid.

Project leader: Hannu Kurki-Suonio


Personnel

Hannu Kurki-Suonio, Planck Scientist, lecturer, project leader, C328
E-mail: hannu.kurki-suoniohelsinki.fi

Elina Keihänen, Planck Scientist, Academy Researcher, PhD, C329
E-mail: elina.keihanenhelsinki.fi

Jussi Väliviita, Planck Scientist, PhD, A329
E-mail: jussi.valiviitahelsinki.fi

Viola Allevato, PhD, D316
E-mail: viola.allevatohelsinki.fi

Charles Kirkpatrick, PhD, D316
E-mail: charles.kirkpatrickhelsinki.fi

Matti Savelainen, Planck Scientist, PhD, A329
E-mail: matti.savelainenhelsinki.fi

Anna-Stiina Suur-Uski, Planck Scientist, PhD, C329
E-mail: anna-stiina.suur-uskihelsinki.fi

Ghassem Gozaliasl, PhD, D315
E-mail: ghassem.gozaliaslhelsinki.fi

Valtteri Lindholm, Graduate Student, A314
E-mail: valtteri.lindholmhelsinki.fi

Kimmo Kiiveri, Graduate Student, A314
E-mail: kimmo.kiiverihelsinki.fi


Links

University of Helsinki Physics Department Planck pages
European Space Agency Planck pages
Planck Science Team pages
Euclid Consortium pages