Difference between revisions of "Galactic Working Group"
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===Members=== | ===Members=== | ||
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== Meetings == | == Meetings == | ||
Revision as of 10:55, 24 February 2022
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: Rubén López-Coto (Leader), Pol Bordas (Deputy)
Past Coordinators: NA
Members
Join the mailing list in:join here
Meetings
Papers
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
