The Large-Sized Telescope (LST-1) is the first prototype telescope for the future Cherenkov Telescope Array Observatory (CTAO) northern site, located in the Roque de los Muchachos in La Palma. The telescope detected the Very High Energy (VHE) gamma ray signal from BL Lacertae, the namesake for the AGN-blazar class, in 2021 and has since then collected many observations of the object. This has allowed us to study extreme levels of VHE variability in an unprecedented flare of the source. The analysis and results will become the base of one of the very first scientific results from the LST collaboration. We will present the results of the BL Lac 2021 observational campaign, including the VHE gamma-ray lightcurve of BL Lacertae detected by the ...
The recent detection of a very high energy (VHE) emission from Gamma-Ray Bursts (GRBs) above 100 GeV...
We present evidence for the first detection of gamma rays from the extragalactic object BL Lacertae....
A very high energy gamma-ray signal has been detected at the 5.5sigma level from H1426+ 428, an X-ra...
38th International Cosmic Ray Conference (ICRC2023), 26 July - 3 August, 2023, Nagoya, Japan.Seiya N...
The Large-Sized Telescope prototype (LST-1) of the future Cherenkov Telescope Array (CTA) Observator...
The first Large-Sized Telescope (LST-1) of the future Cherenkov Telescope Array (CTA) is located in ...
Since about 2002 the current-generation imaging air Cherenkov telescopes have discovered more than 5...
The low-frequency peaked BL Lac (LBL) object BL Lacertae was observed with the MAGIC telescope from ...
The MAGIC collaboration observed BL Lacertae for 22.2 hr during 2005 August to December and for 26 h...
The MAGIC collaboration observed BL Lacertae for 22.2 hr during 2005 August to December and for 26 h...
The MAGIC collaboration observed BL Lacertae for 22.2 hr during 2005 August to December and for 26 h...
BL Lacertae is a blazar at the redshift of z = 0.069, eponym of the BL Lac blazar type. It is also a...
The recent detection of a very high energy (VHE) emission from Gamma-Ray Bursts (GRBs) above 100 GeV...
We present evidence for the first detection of gamma rays from the extragalactic object BL Lacertae....
A very high energy gamma-ray signal has been detected at the 5.5sigma level from H1426+ 428, an X-ra...
38th International Cosmic Ray Conference (ICRC2023), 26 July - 3 August, 2023, Nagoya, Japan.Seiya N...
The Large-Sized Telescope prototype (LST-1) of the future Cherenkov Telescope Array (CTA) Observator...
The first Large-Sized Telescope (LST-1) of the future Cherenkov Telescope Array (CTA) is located in ...
Since about 2002 the current-generation imaging air Cherenkov telescopes have discovered more than 5...
The low-frequency peaked BL Lac (LBL) object BL Lacertae was observed with the MAGIC telescope from ...
The MAGIC collaboration observed BL Lacertae for 22.2 hr during 2005 August to December and for 26 h...
The MAGIC collaboration observed BL Lacertae for 22.2 hr during 2005 August to December and for 26 h...
The MAGIC collaboration observed BL Lacertae for 22.2 hr during 2005 August to December and for 26 h...
BL Lacertae is a blazar at the redshift of z = 0.069, eponym of the BL Lac blazar type. It is also a...
The recent detection of a very high energy (VHE) emission from Gamma-Ray Bursts (GRBs) above 100 GeV...
We present evidence for the first detection of gamma rays from the extragalactic object BL Lacertae....
A very high energy gamma-ray signal has been detected at the 5.5sigma level from H1426+ 428, an X-ra...