Galactic Working Group

Back to Main page
Back to Data Analysis

The Galaxy seen from both hemispheres. Credit: Petr Horálek/Juan Carlos Casado

Introduction

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

Current Coordinators: Rubén López-Coto (Leader), Pol Bordas (Deputy)

Past Coordinators: NA

Members

Join the mailing list in: CTA sharepoint

Meetings

Galactic calls (2022)

Publications

Papers Status

Conferences

Please refer to the LSTCOS webpage for conferences attended by LST members.

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