Now showing items 1-4 of 4

    • Pan, Y. C.; Foley, R. J.; Smith, M.; González Gaitán, Santiago (Oxford University Press, 2017)
      We present the Dark Energy Survey (DES) discovery of DES15E2mlf, the most distant superluminous supernova (SLSN) spectroscopically confirmed to date. The light curves and Gemini spectroscopy of DES15E2mlf indicate that it ...
    • Sepúlveda, S.; Gaete Vásquez, Ximena; Rocha, A.; Smith, M. (Karger, 2016)
    • Smith, M.; Sullivan, M.; Nichol, R. C.; González Gaitán, Santiago (IOP Publishing Ltd, 2018)
      We present observations of DES16C2nm, the first spectroscopically confirmed hydrogen-free superluminous supernova (SLSN-I) at redshift z approximate to 2. DES16C2nm was discovered by the Dark Energy Survey (DES) Supernova ...
    • de Jaeger, T.; Galbany, L.; Gonzalez-Gaitan, S.; Kessler, R.; Filippenko, A. V.; Forster Burón, Francisco; Hamuy, M.; Brown, P. J.; Davis, T. M.; Gutierrez, C. P.; Inserra, C.; Lewis, G. F.; Moller, A.; Scolnic, D.; Smith, M.; Brout, D.; Carollo, D.; Foley, R. J.; Glazebrook, K.; Hinton, S. R.; Macaulay, E.; Nicho, B.; Sako, M.; Sommer, N. E.; Tucker, B. E.; Abbott, T. M. C.; Aguena, M.; Allam, S.; Annis, J.; Avila, S.; Bertin, E.; Bhargava, S.; Brooks, D.; Burke, D. L.; Rosell, A. Carnero; Carrasco Kind, M.; Carretero, J.; Costanzi, M.; Crocce, M.; da Costa, L. N.; De Vicente, J.; Desai, S.; Dieh, H. T.; Doe, P.; Drlica-Wagner, A.; Eifler, T. F.; Garcia-Bellido, J.; Gaztanaga, E.; Gruen, D.; Gruend, R. A.; Gschwend, J.; Gutierrez, G.; Hartley, W. G.; Hollowood, D. L.; Honscheid, K.; James, D. J.; Kuehn, K.; Kuropatkin, N.; Li, T. S.; Lima, M.; Maia, M. A. G.; Menanteau, F.; Mique, R.; Palmese, A.; Paz-Chinchon, F.; Plazas, A. A.; Romer, A. K.; Roodman, A.; Sanchez, E.; Scarpine, V.; Schubne, M.; Serrano, S.; Sevilla-Noarbe, I.; Soares-Santos, M.; Suchyta, E.; Swanson, M. E. C.; Thomas, D.; Tucker, D. L.; Varga, T. N.; Walker, A. R.; Weller, J.; Wilkinson, R. (Oxford University Press, 2020)
      Despite vast improvements in the measurement of the cosmological parameters, the nature of dark energy and an accurate value of the Hubble constant (H-0) in the Hubble-Lemaitre law remain unknown. To break the current ...