Photo Gallery
Photometric Classification of SNIA
April 28 - 29, 2016 | Chicago, IL
PHOTO ALBUM

The Kavli Institute for Cosmological Physics (KICP) at the University of Chicago is hosting a workshop on the Photometric Classification of SNIA on April 28-29, 2016. This workshop will focus on Photometric classification methods and validation techniques for large SNIA data samples. The emphasis will be on defining samples that can be used to measure cosmological parameters, rate vs redshift, and SN-host correlations.

COSMO-2014: International Conference on Particle Physics and Cosmology
August 25 - 29, 2014 | Chicago, IL
PHOTO ALBUM

The Kavli Institute for Cosmological Physics (KICP) at the University of Chicago will host the International Conference on Particle Physics and Cosmology (COSMO 2014) on August 25-29, 2014, held at the University of Chicago's Gleacher Center.

The Dark Energy Spectrometer
May 30 - 31, 2012 | Chicago, IL
PHOTO ALBUM

The Kavli Institute for Cosmological Physics (KICP) at the University of Chicago will host The Dark Energy Spectrometer workshop on May 30-31 to discuss DESpec, a conceptual next generation dark energy project to enable massive spectroscopic surveys in the southern hemisphere. It would naturally synergize with the Dark Energy Survey (DES), which will start taking data later this year, and with LSST in the longer term. The goal of this meeting is to review past and present work on DESpec and to make plans for how to proceed. We will briefly review the current state of the instrument design and then identify the next steps in the project, including describing the R&D necessary to proceed with theory, survey strategy, and instrument definition. The goal of the workshop will be to begin to assemble the DESpec team, define the project's mission statement, and plan how to proceed in the coming year.

Supernova Hub workshop: "Photometric Identification of Supernova"
March 16 - 17, 2012 | Chicago, IL
PHOTO ALBUM

The workshop will focus on methods for identifying type Ia Supernvae (SNIa) without spectroscopy. The emphasis will be on using these photometric SNIa for Hubble Diagram analyses in PannStarrs, the Dark Energy Survey (DES) and the Large Synoptic Survey Telescope (LSST).