Difference between revisions of "PG 1553+113"
(→General information) |
|||
| Line 1: | Line 1: | ||
==General information== | ==General information== | ||
* '''Name of the source''': PG 1553+113 | * '''Name of the source''': PG 1553+113 | ||
| − | * '''Brief description of the source''': This is a BL Lac | + | * '''Brief description of the source''': This is a BL Lac object subject of an intense multi-year, multi-wavelenght campaign by MAGIC. Starting from 2023, LST has a program aimed at searching for intra-night variability during high state (PI E. Prandini). The program was triggered in April 2023. |
:- Object type : BL Lac | :- Object type : BL Lac | ||
:- Redshift : z=0.43 (Dorigo Jones+ 2021) | :- Redshift : z=0.43 (Dorigo Jones+ 2021) | ||
:- TeVCat page [http://tevcat.uchicago.edu/?mode=1&showsrc=102 link] | :- TeVCat page [http://tevcat.uchicago.edu/?mode=1&showsrc=102 link] | ||
| − | |||
== Analysis == | == Analysis == | ||
Revision as of 08:30, 24 April 2024
General information
- Name of the source: PG 1553+113
- Brief description of the source: This is a BL Lac object subject of an intense multi-year, multi-wavelenght campaign by MAGIC. Starting from 2023, LST has a program aimed at searching for intra-night variability during high state (PI E. Prandini). The program was triggered in April 2023.
- - Object type : BL Lac
- - Redshift : z=0.43 (Dorigo Jones+ 2021)
- - TeVCat page link
Analysis
