Extragalactic Working Group
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The Extragalactic Sources Science Group focuses on the analysis of spectra, time variability, searches for periodicity, and cosmological aspects (EBL) of sources outside of our Galaxy.
Current Coordinators: Seiya Nozaki (Leader), Jorge Otero Santos (Deputy)
Past Coordinators: David Sanchez, Mireia Nievas Rosillo
(since April 2024)
Contents
Members
Join us!
Mailing lists:
Slack channels:
EGAL Meeting
Next meetings:
(always check the calendar and indico for last-minute changes)
Date | Meeting | Indico | Minutes
|
---|---|---|---|
Dec 20, 2023 | Egal | [3] | [4] |
Dec 12, 2023 | AGN Zoo | [5] | [6] |
Nov 22, 2023 | Egal | [7] | [8] |
Oct 24, 2023 | AGN Zoo | [9] | [10] |
Oct 18, 2023 | Egal | [11] | [12] |
Sep 6, 2023 | AGN Zoo | [13] | [14] |
Sep 5, 2023 | Egal | [15] | [16] |
Aug 16, 2023 | AGN Zoo | [17] | cancelled |
Aug 11, 2023 | Egal | [18] | cancelled |
July 21, 2023 | AGN Zoo | [19] | [20] |
July 19, 2023 | Egal | [21] | [22] |
Full list of meetings : indico
Past Observation and Current studies
A wiki page devoted to collect the current studies made and the observations that might interest the group can be found here : EGAL_Observations_and_Studies
A list of the ToO can be found here : Logbook_of_ToO
Papers in preparation:
Other source analyses
Papers in advanced stage:
Published / Accepted
Resubmitted
Submitted
Nearing submission (internal review)
conferences
ICRC 2023:
- Ryuji: AGN Zoo - Seiya: BL Lac
TeVPA 2023:
- Joshua: AGN Zoo - Estelle: PG1553+113
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