Accuracy of environmental tracers and consequences for determining the Type Ia supernova magnitude step

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作者
Briday, M. [1 ]
Rigault, M. [1 ]
Graziani, R. [1 ]
Copin, Y. [1 ]
Aldering, G. [3 ]
Amenouche, M. [2 ]
Brinnel, V. [5 ]
Kim, A.G. [3 ]
Kim, Y.-L. [1 ]
Lezmy, J. [1 ]
Nicolas, N. [1 ]
Nordin, J. [5 ]
Perlmutter, S. [4 ]
Rosnet, P. [2 ]
Smith, M. [1 ]
机构
[1] Univ Lyon, Univ Claude Bernard Lyon 1, CNRS, IP2I Lyon/IN2P3, IMR 5822, Villeurbanne,69622, France
[2] Université Clermont Auvergne, CNRS/IN2P3, Laboratoire de Physique de Clermont, Clermont-Ferrand,63000, France
[3] Lawrence Berkeley National Laboratory, 1 Cyclotron Rd., Berkeley,CA,94720, United States
[4] Department of Physics, University of California Berkeley, 366 LeConte Hall, MC 7300, Berkeley,CA,94720-7300, United States
[5] Institute of Physics, Humboldt-Universität zu Berlin, Newtonstr. 15, Berlin,12489, Germany
来源
Astronomy and Astrophysics | 2022年 / 657卷
基金
欧盟地平线“2020”; 美国国家航空航天局; 欧洲研究理事会;
关键词
Luminance - Uncertainty analysis - Galaxies;
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