The supernova was studied with ultraviolet, optical, and near-infrared photometry as well as optical spectra, using the Magellan telescopes in Chile, the MMT telescope in Arizona, the Gemini and Keck telescopes in Hawaii, and NASA's Swift satellite.
The data were collected at Magellan telescopes in Chile, the MMT telescope in Arizona, the Gemini and Keck telescopes in Hawaii, and NASA's Swift satellite. The supernova was studied with ultraviolet, optical, and near-infrared photometry as well as optical spectra.
The supernova was studied with ultraviolet, optical, and near-infrared photometry as well as optical spectra. The data were collected at Magellan telescopes in Chile, the MMT telescope in Arizona, the Gemini and Keck telescopes in Hawaii, and NASA's Swift satellite.
The supernova was studied with ultraviolet, optical, and near-infrared photometry as well as optical spectra. The data were collected at Magellan telescopes in Chile, the MMT telescope in Arizona, the Gemini and Keck telescopes in Hawaii, and NASA's Swift satellite.