Using late-time optical and near-infrared spectra to constrain Type Ia supernova explosion properties

Author:

Maguire K1ORCID,Sim S A1,Shingles L1ORCID,Spyromilio J2,Jerkstrand A3,Sullivan M4,Chen T-W5,Cartier R6,Dimitriadis G47,Frohmaier C8,Galbany L9ORCID,Gutiérrez C P4,Hosseinzadeh G1011,Howell D A1011,Inserra C4ORCID,Rudy R12,Sollerman J13

Affiliation:

1. Astrophysics Research Centre, School of Mathematics and Physics, Queen's University Belfast, Belfast BT7 1NN, UK

2. European Southern Observatory, Karl-Schwarzschild Strasse 2, D-85748 Garching bei München, Germany

3. Max-Planck Institut für Astrophysik, Karl-Schwarzschild Strasse 1, D-85748 Garching bei München, Germany

4. Department of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ, UK

5. Max-Planck-Institut für Extraterrestrische Physik, Giessenbachstrasse 1, D-85748 Garching bei München, Germany

6. Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatory, Casilla 603, La Serena, Chile

7. Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064, USA

8. Institute of Cosmology and Gravitation, University of Portsmouth, Portsmouth PO1 3FX, UK

9. PITT PACC, Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, PA 15260, USA

10. Las Cumbres Observatory, 6740 Cortona Dr Ste 102, Goleta, CA 93117-5575, USA

11. Department of Physics, University of California, Santa Barbara, CA 93106-9530, USA

12. Space Science Applications Laboratory, The Aerospace Corporation, PO Box 92957, Los Angeles, CA 90009, USA

13. The Oskar Klein Centre, Department of Astronomy, Stockholm University, AlbaNova, SE-10691 Stockholm, Sweden

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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