Nijmegen / Tucson / Huntsville / Coventry / Leicester / Ferrara / Santiago / Bellingham / Amsterdam / Surrey / Reykjav´ık / New York / Copenhagen / St Petersburg / /
Company
L21 Starling R. L. C. / GRB 080721 R. L. C. / R. L. C. / L17 Starling R. L. C. / Starling R. L. C. / Isaac Newton Group / Newton Science Analysis Software / GE / JPO / Italy 11 Mullard Space Science Laboratory / /
Country
Netherlands / Norway / Iceland / Finland / Denmark / Italy / Sweden / Chile / Russia / United States / / /
Event
Person Communication and Meetings / /
Facility
Science Institute / University of Copenhagen / Ioffe Physico-Technical Institute / University of Warwick / European Southern Observatory / UCO/Lick Observatory / University of California / University Road / University College London / Paranal Observatory / University of Iceland / Roque de Los Muchachos Observatory / University of Leicester / University of Amsterdam / University of Nijmegen / Liverpool John Moores University / Niels Bohr Institute / University of Ferrara / /
IndustryTerm
energy constraint / rotation energy / high-energy spectral peak / energy bands / spectral peak energy / power-law spectral index / analysis software version / absorbed power-law extrapolation / power-law fits / rotational energy / measured energy limit / energy / observed total energy / power-law photon index / weakest detected metal line / power-law shape / energy budget / power-law models / power law / low-energy / prompt gamma-ray energy / final power-law decays / power-law index / electron energy distribution / overall energy requirements / temporal and spectral power-law models / Double and even triple jet systems / energy range / absorbed power law / metal-poor fast rotators / broken power law / high-energy photons / gamma-ray spectral energy distribution / energy reservoir / power-law decline / explosive energy / collimation-corrected energy / high isotropic energy / power-law decay / peak energy / high-energy spectral slope / isotropic energy / energy conversion / energy injection / power-law fit / power-law model / high-energy budget / reduced using the Swift analysis software version / /
MusicGroup
SED / D / X-ray / /
NaturalFeature
La Palma / /
Organization
University of Leicester / Liverpool John Moores University / UK Science and Technology Facilities Council / Physics Department / Russian Space Agency / Centre for Astrophysics and Cosmology / UK Swift Science Data Centre / University of Ferrara / University of Nijmegen / University of Amsterdam / VLT Antu / Department of Astrophysics / University of Warwick / Centre for Astrophysics / Icelandic Research Fund / Society of Photo-Optical Instrumentation Engineers / Department of Astronomy and Astrophysics / University College London / Department of Physics and Astronomy / Department of Physics / Laboratory for Experimental Astrophysics / Niels Bohr Institute / Instituto de Astrofisica de Canarias / University of California / Santa Cruz / Science Institute / Dark Cosmology Centre / National Aeronautics and Space Administration / Ioffe Physico-Technical Institute / University of Copenhagen / University of Iceland / /
Person
Della Valle / Edita Stonkute / Andrew Read / Nat / Racusin / Daniele Malesani / Juliane Maries Vej / Jenny Carter / Tayyaba Zafar / Birgitta Nordstrom / / /
Position
Butler / author / Schlegel D. J. / Marshall / /
Product
T-90 / Starling et al. / /
ProvinceOrState
Alabama / New York / Washington / California / Arizona / /
Mon. Not. R. Astron. Soc. 400, 90–[removed]doi:[removed]j[removed]15443.x Constraining the energy budget of GRB[removed]R. L. C. Starling,1 E. Rol,1,2 A. J. van der Horst,3 S.-C. Yoon,4 V. Pal’shin,5