Difference between revisions of "WR140"
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==People involved== | ==People involved== | ||
Alphabetical order: Arnau Aguasca-Cabot, Fernando Frías (LST analysis), Alessandro Carosi & Alicia López-Oramas (PI) (MAGIC Analysis) | Alphabetical order: Arnau Aguasca-Cabot, Fernando Frías (LST analysis), Alessandro Carosi & Alicia López-Oramas (PI) (MAGIC Analysis) | ||
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| + | ==Presentations== | ||
| + | None yet | ||
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| + | ==Data-taking information== | ||
* '''Dates of data-taking (yyyymmdd)''': June to November 2024 | * '''Dates of data-taking (yyyymmdd)''': June to November 2024 | ||
Revision as of 09:04, 19 November 2024
Contents
General information
- Name of the source: WR 140
- Brief description of the source:
- - Object type : Colliding Wind Binary
- - Distance (pc) : (Galactic source)
- - Other relevant information: Monitoring of the periastron approach (Nov 23, 2024)
- - RA: (hh mm ss), Dec: (dd mm ss)
- - RA, Dec in deg (ICRS):
- Proposal: dedicated proposal (GAL05)
People involved
Alphabetical order: Arnau Aguasca-Cabot, Fernando Frías (LST analysis), Alessandro Carosi & Alicia López-Oramas (PI) (MAGIC Analysis)
Presentations
None yet
Data-taking information
- Dates of data-taking (yyyymmdd): June to November 2024
- - Date [yyyymmdd] (time of observation h): 20230520 (X.XX)
- ELOG link: [1]
- ZD range (deg): [XX, XX]
- AZ range (deg): [XX, XX]
- Transmission9km: 0.5-0.9
- Runs: 1
- Joint observations with MAGIC? : Yes
- Comments:
