Difference between revisions of "Galactic ToO"
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This page is related to the project '''Target of Opportunity observations of Galactic Transient sources'''. | This page is related to the project '''Target of Opportunity observations of Galactic Transient sources'''. | ||
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| + | You can join the dedicated slack channel lst-galactic-transients: https://cta-north.slack.com/archives/C057YMBC4H5 | ||
==Proposals== | ==Proposals== | ||
* Cycle I: https://www.lst1.iac.es/wiki/index.php/GAL02 | * Cycle I: https://www.lst1.iac.es/wiki/index.php/GAL02 | ||
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| + | ==Teams and triggering== | ||
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| + | Triggers will be discussed within the whole list of co-Is and discussed in the project channels. People forming part of a team are responsible to issue these triggers. If they are not available, any LST member can trigger after discussing it with the aforementioned people. | ||
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| + | The different teams are formed by: | ||
| + | *Novae: A. Aguasca-Cabot, D. Green, H. Katagiri, Y. Kobayashi, R. López-Coto, A. López-Oramas | ||
| + | *Microquasars: P. Bordas, López-Oramas; | ||
| + | *Flares from gamma-ray binaries: P. Bordas, López-Oramas | ||
| + | *Magnetars: A. Carosi, R. López-Coto, A. López-Oramas, G. Panebianco, T. Saito | ||
| + | *Supernovae: A. Carosi, A. López-Oramas | ||
| + | *Flares from pulsar-wind nebulae: R. López-Coto, A. López-Oramas, G. Pirola, T. Saito | ||
| + | *Stellar superflares: A. Carosi, A. López-Oramas | ||
| + | *Other sources: A. Carosi, A. López-Oramas. | ||
Revision as of 10:58, 15 February 2024
This page is related to the project Target of Opportunity observations of Galactic Transient sources.
You can join the dedicated slack channel lst-galactic-transients: https://cta-north.slack.com/archives/C057YMBC4H5
Proposals
Teams and triggering
Triggers will be discussed within the whole list of co-Is and discussed in the project channels. People forming part of a team are responsible to issue these triggers. If they are not available, any LST member can trigger after discussing it with the aforementioned people.
The different teams are formed by:
- Novae: A. Aguasca-Cabot, D. Green, H. Katagiri, Y. Kobayashi, R. López-Coto, A. López-Oramas
- Microquasars: P. Bordas, López-Oramas;
- Flares from gamma-ray binaries: P. Bordas, López-Oramas
- Magnetars: A. Carosi, R. López-Coto, A. López-Oramas, G. Panebianco, T. Saito
- Supernovae: A. Carosi, A. López-Oramas
- Flares from pulsar-wind nebulae: R. López-Coto, A. López-Oramas, G. Pirola, T. Saito
- Stellar superflares: A. Carosi, A. López-Oramas
- Other sources: A. Carosi, A. López-Oramas.
