Difference between revisions of "Extragalactic Working Group"
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Revision as of 09:19, 12 May 2022
Back to Main page
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 May 25, 10AM CEST : https://indico.cta-observatory.org/event/4138/
Papers in preparation:
Papers in advanced stage:
Published / Accepted
Resubmitted
Submitted
Nearing submission (internal review)
conferences
sign up for conferences
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
