Difference between revisions of "Galactic Working Group"

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== Papers in progress: ==
 
== Papers in progress: ==
 
* [[RS Oph]]
 
* [[RS Oph]]
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==Useful Tools==
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* Coordinate converter http://heasarc.gsfc.nasa.gov/cgi-bin/Tools/convcoord/convcoord.pl
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* Distance converter http://www.convertworld.com/en/length/Parsec.html
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* Energy/frequency/wavelength converter  http://heasarc.gsfc.nasa.gov/cgi-bin/Tools/energyconv/energyConv.pl
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* A Date/Time Conversion Utility http://heasarc.gsfc.nasa.gov/cgi-bin/Tools/xTime/xTime.pl
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* Flux/count rate converter http://heasarc.gsfc.nasa.gov/Tools/w3pimms.html
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* Catalog of TeV source http://tevcat.uchicago.edu/
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* Publication of [https://www.mpi-hd.mpg.de/hfm/HESS/pages/publications/pubs_jour.shtml HESS], [https://magic.mpp.mpg.de/backend/publications/articles MAGIC] and [https://veritas.sao.arizona.edu/veritas-science/veritas-results-mainmenu-72 VERITAS]
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* To calculate source observability (you may have to introduce LST-1 coordinates 28.76195, -17.89005) [http://www.magic.iac.es/scheduler/ http://www.magic.iac.es/scheduler/] or [https://www.mpi-hd.mpg.de/hfm/HESS/public/Visibility.html https://www.mpi-hd.mpg.de/hfm/HESS/public/Visibility.html]

Revision as of 07:51, 3 February 2022

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The Galactic Sources Science Group focuses on the analysis of spectra, time variability, and periodicity of sources in our Galaxy.

Current Coordinators: XXX (Leader), XXX (Deputy)

Past Coordinators: NA

Members

Join us!

Mailing list: XXX

Archive of past emails: link


Agenda 2022

Papers in advanced stage:

Published / Accepted

Resubmitted

Submitted

Nearing submission (internal review)

Papers in progress:


Useful Tools