Difference between revisions of "Transient Working Group"
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[https://indico.cta-observatory.org/event/3560/ 30/06/2021 General Meeting] | [https://indico.cta-observatory.org/event/3560/ 30/06/2021 General Meeting] | ||
Revision as of 21:32, 30 October 2023
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:
- Alice Donini (Leader), INAF OAR, Italy, alice.donini@inaf.it
- Monica Seglar-Arroyo (Deputy), IFAE, Spain, mseglar@ifae.es
Past Coordinators:
- Armand Fiasson (Leader), LAPP, France, armand.fiasson@lapp.in2p3.fr
Mailing list and slack channels
Join our mailing list here!
We have several channel in the CTA North Slack Workspace:
- #lst1-alert-followup to discuss the received alerts or any interesting event
- #lst1-transient-analysis to discuss the analysis of the observed events
Main topics
Agenda 2022
Papers in advanced stage:
Published / Accepted
Resubmitted
Submitted
Nearing submission (internal review)
Papers in progress:
Meetings
List of transient group meetings per year:
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
