Difference between revisions of "Transient Working Group"
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== Useful Tools == | == Useful Tools == | ||
Revision as of 21:48, 4 April 2022
Back to Main page
Back to Data Analysis
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
Mailing list
Main topics
- Gamma-Ray Bursts (GRBs)
- Gravitational Waves (GWs)
- Neutrino Observations
Agenda 2022
Papers in advanced stage:
Published / Accepted
Resubmitted
Submitted
Nearing submission (internal review)
Papers in progress:
Meetings
List of transient group meetings.
07/04/2022 Transient WG Meeting
18/03/2022 Transient WG Meeting
Documentation
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
