Difference between revisions of "Transient Working Group"
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The Transient Science Group focuses on the analysis of detection, spectra, and time variability of transient sources such as GRBs. | The Transient Science Group focuses on the analysis of detection, spectra, and time variability of transient sources such as GRBs. | ||
| − | '''Current Coordinators''': Armand Fiasson (Leader), Alice Donini (Deputy) | + | '''Current Coordinators''': |
| + | * Armand Fiasson (Leader), LAPP, France, [mailto:armand.fiasson@lapp.in2p3.fr armand.fiasson@lapp.in2p3.fr] | ||
| + | * Alice Donini (Deputy), INAF OAR, Italy, [mailto:alice.donini@inaf.it alice.donini@inaf.it] | ||
'''Past Coordinators''': NA | '''Past Coordinators''': NA | ||
| − | ===Members=== | + | === Members === |
'''Join us!''' Mailing list: [https://portal.cta-observatory.org/_layouts/people.aspx?MembershipGroupId=3277 join here] | '''Join us!''' Mailing list: [https://portal.cta-observatory.org/_layouts/people.aspx?MembershipGroupId=3277 join here] | ||
Revision as of 09:46, 1 March 2022
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Contents
Introduction
The Transient Science Group focuses on the analysis of detection, spectra, and time variability of transient sources such as GRBs.
Current Coordinators:
- Armand Fiasson (Leader), LAPP, France, armand.fiasson@lapp.in2p3.fr
- Alice Donini (Deputy), INAF OAR, Italy, alice.donini@inaf.it
Past Coordinators: NA
Members
Join us! Mailing list: join here
Agenda 2022
Papers in advanced stage:
Published / Accepted
Resubmitted
Submitted
Nearing submission (internal review)
Papers in progress:
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
