Difference between revisions of "Extragalactic Working Group"
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==Useful Tools== | ==Useful Tools== | ||
Revision as of 13:53, 14 March 2022
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Back to Data Analysis
The Extragalactic Sources Science Group focuses on the analysis of spectra, time variability, and periodicity of sources outside of our Galaxy.
Current Coordinators: David Sanchez (Leader), Mireia Neivas Rosillo (Deputy)
Past Coordinators: NA
Contents
Members
Join us!
Mailing list: join here
Agenda 2022
all the meetings : indico
Next meeting Mach 24, 2PM : https://indico.cta-observatory.org/event/4007/
Papers in preparation:
Papers in advanced stage:
Published / Accepted
Resubmitted
Submitted
Nearing submission (internal review)
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
