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Observing GRB afterglows, SNe and their host galaxies with the 10.4 m Gran Telescopio Canarias (GTC)

Published online by Cambridge University Press:  22 July 2013

J. Gorosabel
Affiliation:
Unidad Asociada Grupo Ciencia Planetarias UPV/EHU-IAA/CSIC, Departamento de Física Aplicada I, E.T.S. Ingeniería, Universidad del PaísVasco UPV/EHU, Alameda de Urquijo s/n, 48013 Bilbao, Spain Ikerbasque, Basque Foundation for Science, Alameda de Urquijo 36-5, 48008 Bilbao, Spain
A.J. Castro-Tirado
Affiliation:
Instituto de Astrofísica de Andalucía (IAA-CSIC), Glorieta de la Astronomía s/n, 18008, Granada, Spain
A. de Ugarte Postigo
Affiliation:
Instituto de Astrofísica de Andalucía (IAA-CSIC), Glorieta de la Astronomía s/n, 18008, Granada, Spain Dark Cosmology Centre, Niels Bohr Institute, Juliane Maries Vej 30, 2100, Copenhagen Ø, Denmark
C.C. Thöne
Affiliation:
Instituto de Astrofísica de Andalucía (IAA-CSIC), Glorieta de la Astronomía s/n, 18008, Granada, Spain
R. Sánchez-Ramírez
Affiliation:
Instituto de Astrofísica de Andalucía (IAA-CSIC), Glorieta de la Astronomía s/n, 18008, Granada, Spain
D. Peréz-Ramírez
Affiliation:
Departamento de Física, Universidad de Jaén, Campus Las Lagunillas, 23071 Jaén, Spain
J.C. Tello
Affiliation:
Instituto de Astrofísica de Andalucía (IAA-CSIC), Glorieta de la Astronomía s/n, 18008, Granada, Spain
M. Jelínek
Affiliation:
Instituto de Astrofísica de Andalucía (IAA-CSIC), Glorieta de la Astronomía s/n, 18008, Granada, Spain
S. Guziy
Affiliation:
Instituto de Astrofísica de Andalucía (IAA-CSIC), Glorieta de la Astronomía s/n, 18008, Granada, Spain Astronomical Observatory, Nikolaev National University, Nikolaev, Ukraine
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Abstract

We summarize the results of our programs started in 2009 with the 10.4 m Gran Telescopio Canarias (GTC) telescope. Since then its instruments have been subject of a continuous upgrade, making the GTC a competitive telescope for the GRB field. So far (Dec. 2012) the GTC have followed up 25 GRBs, measuring 10 redshifts, and discovering two SNe associated to GRBs. The new generation of instruments foreseen for the coming years will contribute substantially to enhance the knowledge of these puzzling explosions.

Type
Research Article
Copyright
© EAS, EDP Sciences 2013

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