Difference between revisions of "PG 1553+113"
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== Analysis == | == Analysis == | ||
| + | * [[AGN_paper_LST1#PG_1553.2B113 | AGN zoo paper]] - commissioning data (2021-2022) | ||
| + | * [[PG 1553 - 2023 ToO data analysis]] - Cycle1 data, dedicated proposal triggered | ||
| + | * [[PG 1553 - redshift]] | ||
| − | + | == Publications and Conferences == | |
| − | + | * PG1553 2021-2022 data are part of the AGN zoo paper | |
| + | * Planned: we plan a publication on 2023 flare (Prandini & Luciani) | ||
Latest revision as of 15:40, 2 December 2024
General information[edit]
- 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. LST observed the source since the beginning of its commissioning. Starting from Cycle 1, 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 (HBL)
- - Redshift : z=0.43 (Dorigo Jones+ 2021)
- - TeVCat page link
Analysis[edit]
- AGN zoo paper - commissioning data (2021-2022)
- PG 1553 - 2023 ToO data analysis - Cycle1 data, dedicated proposal triggered
- PG 1553 - redshift
Publications and Conferences[edit]
- PG1553 2021-2022 data are part of the AGN zoo paper
- Planned: we plan a publication on 2023 flare (Prandini & Luciani)
