Difference between revisions of "SGR1935+2154"
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==Presentations== | ==Presentations== | ||
| − | * 2023-06-05 LST Analysis Call (reco meeting): https://indico.cta-observatory.org/event/4919/contributions/40145/attachments/23853/34369/SGR1935+2154withLST1.pdf | + | * 2023-06-05 LST Analysis Call (reco meeting): [https://indico.cta-observatory.org/event/4919/contributions/40145/attachments/23853/34369/SGR1935+2154withLST1.pdf link to pdf] |
| − | * 2023-06-19 LST General Meeting: https://indico.cta-observatory.org/event/4727/contributions/40419/attachments/23955/34570/SGR1935+2154withLST1.pdf | + | * 2023-06-19 '''LST General Meeting''': [https://indico.cta-observatory.org/event/4727/contributions/40419/attachments/23955/34570/SGR1935+2154withLST1.pdf link to pdf] |
| − | * 2023-07-21 LST Galactic Group Meeting: https://indico.cta-observatory.org/event/5033/contributions/40844/attachments/24208/34981/SGR1935+2154status.pdf | + | * 2023-07-21 LST Galactic Group Meeting: [https://indico.cta-observatory.org/event/5033/contributions/40844/attachments/24208/34981/SGR1935+2154status.pdf link to pdf] |
==Data-taking Information== | ==Data-taking Information== | ||
Revision as of 16:12, 7 September 2023
Note: Under construction
Contents
General Information
- Name of the source: SGR 1935+2154
- Brief description of the source:
- Object type : Soft Gamma Repeater, Galactic Magnetar
- Other relevant information: Its simultaneous X-ray bursts and Fast radio Bursts on April 28th, 2020 suggest that FRB can be created by magnetars.
- RA: 19 35 00.0 (hh mm ss), Dec: +21 53 59.1 (dd mm ss)
- RA, Dec in deg (ICRS): 293.75, 21.90
- Galactic Coordinates l=57.26, b=0.81
People involved
- Gabriele Panebianco (gabriele.panebianco@inaf.it)
- Rubén López-Coto (rlopezcoto@iaa.es)
- Andrea Bulgarelli
Presentations
- 2023-06-05 LST Analysis Call (reco meeting): link to pdf
- 2023-06-19 LST General Meeting: link to pdf
- 2023-07-21 LST Galactic Group Meeting: link to pdf
Data-taking Information
To be added
Data analysis Information
To be added
