Transient Working Group
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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:
- Monica Seglar-Arroyo (Lead), IFAE, Spain, mseglar@ifae.es
- Irene Burelli (Deputy), irene.burelli@gmail.com
Past Coordinators:
- Alice Donini, INAF OAR, Italy, alice.donini@inaf.it (lead convener in 2023)
- Armand Fiasson, LAPP, France, armand.fiasson@lapp.in2p3.fr (lead convener in 2022)
Mailing list and slack channels
Join our mailing list following these instructions: go the outlook webapp https://outlook.office.com/mail/ login with your <firstname>.<lastname>@cta-consortium.org account. Then, in the tab where there is the inbox, etc, scroll down to groups. There you can manage the mailing list to which you are subscribed.
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
Proposals
2024:
- TRAN01: Spotting the GRB counterpart to gravitational wave detections during the second half of O4 (PI: Monica Seglar-Arroyo)
- TRAN02: Gamma-ray bursts observations (PI: Edna Ruiz-Velasco)
- TRAN03: Follow-up Observations of Fast Radio Bursts (PI: Alessandro Carosi)
- TRAN04: Neutrino ToO (NToO) Observations (PI: Koji Noda)
2023:
- TRAN01: Follow-up of gravitational wave events
- TRAN02: Gamma-ray burst observations
- TRAN03: Tick-Tock: Monitoring of an inspiraling binary SMBH
Papers in progress:
Meetings
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