Difference between revisions of "Galactic Working Group"
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== Meetings == | == Meetings == | ||
Revision as of 11:06, 11 April 2023
Back to Main page
Back to Data Analysis
Introduction
The Galactic Sources Science Group focuses on the analysis of spectra, time variability, and periodicity of sources in our Galaxy.
Current Coordinators: Pol Bordas (Leader), Jakub Jurysek (Deputy)
Past Coordinators: Ruben Lopez-Coto
Members
Join the mailing list in: CTA sharepoint
Meetings
Publications
Proposals
File:LST MAGIC Engineering proposal CycleXVII.pdf
Conferences
Please refer to the LSTCOS webpage for conferences attended by LST members.
Useful Tools
- Coordinate converter http://heasarc.gsfc.nasa.gov/cgi-bin/Tools/convcoord/convcoord.pl
- Distance converter http://www.convertworld.com/en/length/Parsec.html
- Energy/frequency/wavelength converter http://heasarc.gsfc.nasa.gov/cgi-bin/Tools/energyconv/energyConv.pl
- A Date/Time Conversion Utility http://heasarc.gsfc.nasa.gov/cgi-bin/Tools/xTime/xTime.pl
- Flux/count rate converter http://heasarc.gsfc.nasa.gov/Tools/w3pimms.html
- Catalog of TeV source http://tevcat.uchicago.edu/
- Publication of HESS, MAGIC and VERITAS
- To calculate source observability (you may have to introduce LST-1 coordinates 28.76195, -17.89005) http://www.magic.iac.es/scheduler/ or https://www.mpi-hd.mpg.de/hfm/HESS/public/Visibility.html
