M. Diaz
University of Texas at Austin
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The Astrophysical Journal | 2017
M. Diaz; Lucas M. Macri; D. García Lambas; C. Mendes de Oliveira; J. L. Nilo Castellón; T. Ribeiro; B. Sanchez; W. Schoenell; L. R. Abramo; S. Akras; J. S. Alcaniz; Rodolfo L. Artola; Martin Beroiz; S. Bonoli; J. Cabral; R. Camuccio; M. Castillo; V. Chavushyan; P. Coelho; C. Colazo; M. V. Costa-Duarte; H. Cuevas Larenas; D. L. DePoy; M. Domínguez Romero; D. Dultzin; D. Fernández; J. García; C. Girardini; D. R. Gonçalves; Thiago S. Gonçalves
We present the results of prompt optical follow-up of the electromagnetic counterpart of the gravitational-wave event GW170817 by the Transient Optical Robotic Observatory of the South Collaboration. We detected highly significant dimming in the light curves of the counterpart (Delta g= 0.17 +/- 0.03 mag, Delta r = 0.14 +/- 0.02 mag, Delta i = 0.10 +/- 0.03 mag) over the course of only 80 minutes of observations obtained similar to 35 hr after the trigger with the T80- South telescope. A second epoch of observations, obtained similar to 59 hr after the event with the EABA 1.5 m telescope, confirms the fast fading nature of the transient. The observed colors of the counterpart suggest that this event was a blue kilonova relatively free of lanthanides.