Difference between revisions of "WR140"
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:- RA: (hh mm ss), Dec: (dd mm ss) | :- RA: (hh mm ss), Dec: (dd mm ss) | ||
:- RA, Dec in deg (ICRS): | :- RA, Dec in deg (ICRS): | ||
| − | * Proposal: dedicated proposal (GAL05) | + | * Proposal: dedicated LST-1 proposal (GAL08), also joint MAGIC+LST-1 proposal (GAL05 in MAGIC) |
==People involved== | ==People involved== | ||
| − | + | Analyzers by alphabetical order: Arnau Aguasca-Cabot, Fernando Frías (LST analysis), Alessandro Carosi & Alicia López-Oramas (PI) (MAGIC Analysis) | |
| − | |||
==Presentations== | ==Presentations== | ||
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== Data analysis == | == Data analysis == | ||
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| + | === Analysis by Fernando Frías === | ||
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| + | [[File:myfile.png | 600 px]] | ||
Latest revision as of 12:27, 21 November 2024
Contents
General information[edit]
- 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 LST-1 proposal (GAL08), also joint MAGIC+LST-1 proposal (GAL05 in MAGIC)
People involved[edit]
Analyzers by alphabetical order: Arnau Aguasca-Cabot, Fernando Frías (LST analysis), Alessandro Carosi & Alicia López-Oramas (PI) (MAGIC Analysis)
Presentations[edit]
None yet
Data-taking information[edit]
- 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:
