supernovae

Documents about supernovae

• Boxlib with tiling: an adaptive mesh refinement software framework#934558Koc University Digital Collections
• Core-collapse supernovae 2022prr, 2023ucy, and 2024ljc in the luminous infrared galaxy NGC 6745#1036132arXiv (All)
• AT 2024wpp: An extremely luminous fast ultraviolet transient powered by accretion onto a black hole#392138ISTA Publications
• Bianchi type-II models in the presence of perfect fluid and anisotropic dark energy#954722Koc University Digital Collections
• Updated 1.1% Precision Values of the Hubble Constant with Corrected Pantheon+ and Dark Energy Survey (DES)-DOVEKIE Type Ia Supernovae#1011171arXiv (All)
• Quantitative modelling of type Ia supernovae spectral time series II: Exploring the diversity of thermonuclear explosion scenarios#987655arXiv (All)
• A statistical study of the environmental age of core-collapse supernovae based on VLT/MUSE integral-field-unit spectroscopy#788731arXiv (OAI Expanded)
• A statistical study of the environmental age of core-collapse supernovae based on VLT/MUSE integral-field-unit spectroscopy#792731arXiv (All)
• Probing kinematics and fate of the universe with linearly time-varying deceleration parameter#954708Koc University Digital Collections
• Confronting Cold New Early Dark Energy and its Equation of State with Updated CMB and Supernovae Data#246721HAL (France)
• GRB 260310A/SN 2026fgk: a multiwavelength study of a nearby underluminous long GRB and SN with a complex afterglow#684918HAL (France)
• Photometric Selection of High-Redshift Type Ia Supernova Candidates#612128eScholarship
• Evidence of environmental dependencies of Type Ia supernovae from the Nearby Supernova Factory indicated by local Hα (Corrigendum)#491951eScholarship
• What nature already gives us a practical source hypothesis for wormholes and time difference#456782Figshare
• H 0 without the sound horizon (or supernovae): A 2% measurement in DESI DR1#780520eScholarship
• <em>H</em>₀ without the sound horizon (or supernovae): A 2% measurement in DESI DR1#495567OSTI.gov
• Constraining High-energy Neutrino Emission from Supernovae with IceCube#491804eScholarship
• Study of Key ⁵⁷Ni ⁢(𝑝,𝛾)⁢ ⁵⁸Cu Resonances to Understand ⁴⁴Ti Nucleosynthesis in Supernovae#626283OSTI.gov
• The Type Ia Supernova Rate at z ≈ 0.5 from the Supernova Legacy Survey**Based on observations obtained with MegaPrime/MegaCam, a joint project of the Canada-France-Hawaii Telescope (CFHT) and CEA/DAPNIA, at CFHT, which is operated by the National Research Council (NRC) of Canada, the Institut National des Sciences de l’Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii. This work is based in part on data products produced at the Canadian Astronomy Data Centre as part of the Canada-France-Hawaii Telescope Legacy Survey, a collaborative project of NRC and CNRS. This work is also based on observations obtained at the European Southern Observatory using the Very Large Telescope on the Cerro Paranal (ESO Large Program 171.A-0486), and on observations (programs GN-2004A-Q-19, GS-2004A-Q-11, GN-2003B-Q-9, and GS-2003B-Q-8) obtained at the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperati#612022eScholarship