Difference between revisions of "Galactic Working Group"
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== Introduction == | == Introduction == | ||
| − | The Galactic | + | The Galactic Working Group focuses on the spectral and morphological study of Galactic gamma-ray sources and their time properties at VHE gamma-rays. |
'''Current Coordinators''': Pol Bordas (Leader), Jakub Jurysek (Deputy) | '''Current Coordinators''': Pol Bordas (Leader), Jakub Jurysek (Deputy) | ||
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'''Past Coordinators''': Ruben Lopez-Coto | '''Past Coordinators''': Ruben Lopez-Coto | ||
| − | === | + | == Members == |
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| + | '''Mailing list: '''[https://ctaoobservatory.sharepoint.com/sites/help/SitePages/Mailing-lists.aspx?csf=1&web=1&e=t3Db5z CTA sharepoint] | ||
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| + | '''Slack channel in CTA North workspace: '''[https://app.slack.com/client/T4GSUFW6M/C056T8WJMNV?selected_team_id=T4GSUFW6M] | ||
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== Meetings == | == Meetings == | ||
Revision as of 13:39, 5 May 2023
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Back to Data Analysis
Introduction
The Galactic Working Group focuses on the spectral and morphological study of Galactic gamma-ray sources and their time properties at VHE gamma-rays.
Current Coordinators: Pol Bordas (Leader), Jakub Jurysek (Deputy)
Past Coordinators: Ruben Lopez-Coto
Members
Mailing list: CTA sharepoint
Slack channel in CTA North workspace: [1]
Meetings
Ongoing Projects
RS Oph
- PI: Team:
- Abstract:
- Link: Project Webpage
Galactic Center
- PI: Team:
- Abstract:
- Link: Project Webpage
Crab Nebula Performance
- PI: Team:
- Abstract:
- Link: Project Webpage
Crab Pulsar
- PI: Team:
- Abstract:
- Link: Project Webpage
Publications
Observed Galactic Sources
Full up-to-date list of all observed sources: Sources observed with LST-1
Data collected (4 May 2023):
Crab: 301.4 hours, LHAASOJ2108+5157: 93.7 hours, GalacticCenter: 50.3 hours, G106.3+2.7: 49.6 hours, Geminga: 40.4 hours, SGR1935+2154: 31.8 hours LHAASOJ0341+5258: 28.7 hours, Nova_RS_Oph: 15.0 hours, U_Sco: 10.9 hours, LHAASOJ1956+2845: 6.9 hours, PSRJ1402+13: 5.7 hours, PSRJ2021+3651: 5.7 hours, HESS1857+026: 4.7 hours, LSV+4417: 4.6 hours, N-Her_2021: 4.4 hours, LSI+61: 4.0 hours, Cyg-X3: 3.9 hours, Cygnus_XNorth: 3.4 hours, V1405Cas: 3.3 hours, AGLJ2114+6249: 2.4 hours, G17.8+16.7: 2.2 hours, 4FGLJ1723.5-0501e: 1.6 hours PSRJ2229+6114: 1.4 hours, MAXIJ1848-015: 1.3 hours, PSRJ2032: 1.1 hours, HESS J1848-018: 0.3 hours, Nova_V1405_Cas: 0.3 hours,
Proposals
File:LST MAGIC Engineering proposal CycleXVII.pdf
Conferences
Please refer to the LSTCOS webpage for a list of upcoming 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
