JWST Spectroscopy of SN H0pe: Classification and Time Delays of a Triply Imaged Type Ia Supernova at z = 1.78

SN H0pe is a triply imaged supernova (SN) at redshift z = 1.78 discovered using the James Webb Space Telescope. In order to classify the SN spectroscopically and measure the relative time delays of its three images (designated A, B, and C), we acquired NIRSpec follow-up spectroscopy spanning 0.6–5 μ...

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Detaylı Bibliyografya
Asıl Yazarlar:	Wenlei Chen, Patrick L. Kelly, Brenda L. Frye, Justin Pierel, S. P. Willner, Massimo Pascale, Seth H. Cohen, Christopher J. Conselice, Michael Engesser, Lukas J. Furtak, Daniel Gilman, Norman A. Grogin, Simon Huber, Saurabh W. Jha, Joel Johansson, Anton M. Koekemoer, Conor Larison, Ashish K. Meena, Matthew R. Siebert, Rogier A. Windhorst, Haojing Yan, Adi Zitrin
Materyal Türü:	Artigo
Dil:	Inglês
Baskı/Yayın Bilgisi:	IOP Publishing 2024-01-01
Seri Bilgileri:	The Astrophysical Journal
Konular:	Type Ia supernovae Gravitational lensing Strong gravitational lensing Rich galaxy clusters Spectroscopy James Webb Space Telescope
Online Erişim:	https://doi.org/10.3847/1538-4357/ad50a5
Etiketler:	Etiketle Etiket eklenmemiş, İlk siz ekleyin!

JWST Spectroscopy of SN H0pe: Classification and Time Delays of a Triply Imaged Type Ia Supernova at z = 1.78

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