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International Space Science Institute (ISSI)Hallerstrasse 6
3012 Bern
Switzerland

Phone +41 31 684 48 96
Email issi@issibern.ch

Our scientific opportunities support the community through six distinct modes of operation. Links to proposal templates or on-line submission forms are provided for each individual tool.

Find explanations, forms of applications and an overview of current and past activities.

Conceptual overview of the Local Distance Network, a many routes approach. Different methods for distance determination may connect the absolute scale determined by geometric means to H0. Background rectangles indicate from left to right where Rung 1, Rung 2, and Rung 3 of a traditional distance ladder would fall. Graphic by Fabio Crameri, ISSI, based on original from Casertano et al. (2025). Figure available from https://s-ink.org/local-distance-network
Conceptual overview of the Local Distance Network, a many routes approach. Different methods for distance determination may connect the absolute scale determined by geometric means to H0. Background rectangles indicate from left to right where Rung 1, Rung 2, and Rung 3 of a traditional distance ladder would fall. Graphic by Fabio Crameri, ISSI, based on original from Casertano et al. (2025). Figure available from https://s-ink.org/local-distance-network

Upcoming Game Changers Webinar

The Local Distance Network to measure the Hubble Constant at ~1% precision

Online Panel Discussion with Stefano Casertano, Richard I. Anderson, Eleonora Di Valentino, Adam Riess, and Licia Verde

Thursday, December 11, 2025
(17:00 CET | 11:00 EDT)

Please click here for the Zoom Session

Meeting ID: 852 6990 9362        Password: 459004

Abstract

The Hubble constant is widely acknowledged as a key test of our understanding of cosmology and the history of the Universe: its locally measured value differs from prevailing cosmological predictions with very high significance. The participants in a weeklong ISSI workshop in March have developed a new formalism, the Distance Network, to enable a rigorous analysis of a large, diverse set of distance measurements, yielding a more precise and robust value of the Hubble constant – and strengthening the discrepancy with cosmological predictions. The Distance Network formalism will be made publicly available and has the capability to incorporate future measurements as they become available.

About the Panellists

Stefano Casertano is an Observatory Scientist at the Space Telescope Science Institute in Baltimore.  He is an expert in distance scale and microlensing, as well as in space-based instrumentation and observations. He received his postgraduate degree from the Scuola Normale Superiore in Pisa.

Richard I. Anderson is an assistant professor at EPFL in Switzerland and PI of the ERC Starting Grant H1PStars. He is a leading expert in the astrophysics and distance applications of stellar standard candles. Prior to his current position, he obtained a PhD in Astrophysics from the University of Geneva and won two postdoctoral fellowships at Johns Hopkins University and the European Southern Observatory.

Eleonora Di Valentino is a Royal Society Dorothy Hodgkin Senior Research Fellow at the University of Sheffield specializing in cosmological tensions and the Hubble constant. She received her PhD from the University of Rome La Sapienza and previously held positions at the Institut d’Astrophysique de Paris (Lagrange Fellow), the University of Manchester (Postdoctoral Researcher), and Durham University’s Institute of Advanced Study (Addison-Wheeler Fellow).

Adam Riess is the  Bloomberg Distinguished Professor at Johns Hopkins University and the Space Telescope Science Institute. He is known for his research in using supernovae as cosmological probes. Riess shared both the 2006 Shaw Prize in Astronomy and the 2011 Nobel Prize in Physics with Saul Perlmutter and Brian Schmidt for providing evidence that the expansion of the universe is accelerating.

Licia Verde, ICREA professor at Instituto de Ciencias del Cosmos, Universitat de Barcelona (ICCUB) where she  leads the Cosmology & Large-Scale Structures research group. She is scientific director of the ICCUB and scientific director of JCAP. Her research focuses on the large-scale structure of the universe, the cosmic microwave background, galaxy surveys and statistical tools to analyse  and interpret cosmological data.

About The Webinars

NASA, ESA, CSA, S. Finkelstein (University of Texas)