GRBSpec and GRBPhot: Social networks to share gamma ray burst data

Publikation: Bidrag til bog/antologi/rapportKonferencebidrag i proceedingsForskningfagfællebedømt

  • Martin Blazek
  • A. De Ugarte Postigo
  • D. A. Kann
  • C. C. Thöne
  • J. F. Agüĺ Fernández
  • Izzo, Luca

GRBSpec and GRBPhot are two databases designed for the storage and analysis of gamma-ray burst (GRB) data. GRBSpec is devoted to spectroscopic observations, GRBPhot to photometric data. Both databases have a detailed search engine and offer online graphical tools for plotting and data analysis. They aim to publicly share these specialised data among the astronomical community and provide quick online measurements and plots. The databases can be accessed through http://grbpsec.iaa.es and http://grbphot.iaa.es, respectively. As of November 2020, the database already contained 2013 files belonging to 810 spectra of 268 different GRBs.

OriginalsprogEngelsk
TitelSoftware and Cyberinfrastructure for Astronomy VI
RedaktørerJuan C. Guzman, Jorge Ibsen
Antal sider8
ForlagSPIE - International Society for Optical Engineering
Publikationsdato2020
Artikelnummer1145218
ISBN (Elektronisk)9781510636910
DOI
StatusUdgivet - 2020
BegivenhedSoftware and Cyberinfrastructure for Astronomy VI 2020 - Virtual, Online, USA
Varighed: 14 dec. 202018 dec. 2020

Konference

KonferenceSoftware and Cyberinfrastructure for Astronomy VI 2020
LandUSA
ByVirtual, Online
Periode14/12/202018/12/2020
SponsorThe Society of Photo-Optical Instrumentation Engineers (SPIE)
NavnProceedings of SPIE - The International Society for Optical Engineering
Vol/bind11452
ISSN0277-786X

Bibliografisk note

Funding Information:
GRBSpec and GRBPhot have been made possible through the generous contribution of a 2016 Leonardo Grant for Researchers and Cultural Creators, BBVA Foundation. AdUP and CT acknowledge support from Ramón y Cajal fellowships (RyC-2012-09975, RyC-2012-09984). MB acknowledges funding associated to a personal técnico de apoyo fellowship (PTA2016-13192-I). DAK acknowledges support from Spanish National Research Project RTI2018-098104-J-I00 (GRBPhot). LI was supported by grants from VILLUM FONDEN (project number 16599 and 25501). JFAF acknowledge financial support from Ministerio de Ciencia, Innovación y Universidades fellowship (PRE2018-086507).

Publisher Copyright:
© 2020 SPIE.

ID: 271558832