2005ANU Open Research (Australian National University)Open access

Supernova Cosmology and the ESSENCE project

J. Sollerman, Claudio Aguilera, Andy Becker, S. Blondin, P. Challis, A. Clocchiatti, Alex Filippenko, R. J. Foley, P. Garnavich, M. Hicken, Saurabh W. Jha, R. Kirshner, K. Krisciunas, B. Leibundgut, Weidong Li, T. Matheson, G. Miknaitis, A. Rest, Adam G. Riess, M. Salvo, B. Schmidt, Chris Smith, J. Spyromilio, C. W. Stubbs, N. B. Suntzeff, J. Tonry, Michael Wood-Vasey, B. Barris, T. M. Davis, Edvard Mörtsell

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Abstract

The proper usage of Type Ia supernovae (SNe Ia) as distance indicators has revolutionized cosmology, and added a new dominant component to the energy density of the Universe, dark energy. Following the discovery and confirmation era, the currently ongoing SNe Ia surveys aim to determine the properties of the dark energy. ESSENCE is a five year ground-based supernova survey aimed at finding and characterizing 200 SNe Ia in the redshift domain z=[0.2-0.8]. The goal of the project is to put constraints on the equation of state parameter, w, of the dark energy with an accuracy of <10%. This paper presents these ongoing efforts in the context of the current developments in observational cosmology.

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The proper usage of Type Ia supernovae (SNe Ia) as distance indicators has revolutionized cosmology, and added a new dominant component to the energy density of the Universe, dark energy. Following the discovery and confirmation era, the currently ongoing SNe Ia surveys aim to determine the properties of the dark energy. ESSENCE is a five year ground-based supernova survey aimed at finding and characterizing 200 SNe Ia in the redshift domain z=[0.2-0.8]. The goal of the project is to put constraints on the equation of state parameter, w, of the dark energy with an accuracy of <10%. This paper presents these ongoing efforts in the context of the current developments in observational cosmology.

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Available abstract

The proper usage of Type Ia supernovae (SNe Ia) as distance indicators has revolutionized cosmology, and added a new dominant component to the energy density of the Universe, dark energy. Following the discovery and confirmation era, the currently ongoing SNe Ia surveys aim to determine the properties of the dark energy. ESSENCE is a five year ground-based supernova survey aimed at finding and characterizing 200 SNe Ia in the redshift domain z=[0.2-0.8]. The goal of the project is to put constraints on the equation of state parameter, w, of the dark energy with an accuracy of <10%. This paper presents these ongoing efforts in the context of the current developments in observational cosmology.

Key concepts: Dark energy, Cosmology, Supernova, Physics, Redshift, Context (archaeology), Astrophysics, Observational cosmology

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