VERITAS is an imaging atmospheric Cherenkov telescope (IACT) array most sensitive to gamma rays in the very-high-energy (VHE) energy band (85 GeV - 30 TeV). As a part of its active galactic nuclei (AGN) program, VERITAS focuses on the identification and follow-up of AGN flares reported by other multiwavelength observatories. Between October 15th and October 19th, 2020, VERITAS followed up on the Fermi-LAT and MAGIC detections of a flare of the intermediate-frequency-peaked BL Lacertae (IBL) object, B2 1811+31, located at a redshift of z=0.117. In this work, we present preliminary scientific results from the analysis of B2 1811+31's 2020 flare, including the corresponding Fermi-LAT light curve and VERITAS detection analysis.Comment: 8 pages,...
We present results from an intensive VERITAS monitoring campaign of the high-frequency peaked BL Lac...
We report the detection of very high energy γ-ray emission from the intermediate-frequency-peaked BL...
We present multi-wavelength observations by Chandrayaan-2/XSM, SDO/AIA and Hinode/XRT of a B-class f...
The Galactic Center region hosts a variety of powerful astronomical sources and rare astrophysical p...
B2 1215+30 is a BL-Lac-type blazar that was first detected at TeV energies by the MAGIC atmospheric ...
3C 279 showed enhanced flux variations in Fermi-LAT {\gamma}-ray observations from January to June 2...
A decade after the discovery of TeV gamma-rays from the blazar Mrk 421 (Punch et al. 1992), the list...
We report the results from our study of the blazar S5 1803+784 carried out using the quasi-simultane...
International audienceB2 1215+30 is a BL-Lac-type blazar that was first detected at TeV energies by ...
High-frequency-peaked BL Lacs (HBLs) dominate the extragalactic TeV sky, with more than 50 objects d...
We present results from an intensive VERITAS monitoring campaign of the high-frequency peaked BL Lac...
B2 1215+30 is a BL-Lac-type blazar that was first detected at TeV energies by the MAGIC atmospheric ...
AbstractVERITAS is a ground-based gamma-ray observatory consisting of an array of four atmospheric C...
We discuss the key science motivations for observing these sources – including performing multiwavel...
M87 was discovered in the very-high-energy band (VHE, E > 100 GeV) with HEGRA in 2003, long before i...
We present results from an intensive VERITAS monitoring campaign of the high-frequency peaked BL Lac...
We report the detection of very high energy γ-ray emission from the intermediate-frequency-peaked BL...
We present multi-wavelength observations by Chandrayaan-2/XSM, SDO/AIA and Hinode/XRT of a B-class f...
The Galactic Center region hosts a variety of powerful astronomical sources and rare astrophysical p...
B2 1215+30 is a BL-Lac-type blazar that was first detected at TeV energies by the MAGIC atmospheric ...
3C 279 showed enhanced flux variations in Fermi-LAT {\gamma}-ray observations from January to June 2...
A decade after the discovery of TeV gamma-rays from the blazar Mrk 421 (Punch et al. 1992), the list...
We report the results from our study of the blazar S5 1803+784 carried out using the quasi-simultane...
International audienceB2 1215+30 is a BL-Lac-type blazar that was first detected at TeV energies by ...
High-frequency-peaked BL Lacs (HBLs) dominate the extragalactic TeV sky, with more than 50 objects d...
We present results from an intensive VERITAS monitoring campaign of the high-frequency peaked BL Lac...
B2 1215+30 is a BL-Lac-type blazar that was first detected at TeV energies by the MAGIC atmospheric ...
AbstractVERITAS is a ground-based gamma-ray observatory consisting of an array of four atmospheric C...
We discuss the key science motivations for observing these sources – including performing multiwavel...
M87 was discovered in the very-high-energy band (VHE, E > 100 GeV) with HEGRA in 2003, long before i...
We present results from an intensive VERITAS monitoring campaign of the high-frequency peaked BL Lac...
We report the detection of very high energy γ-ray emission from the intermediate-frequency-peaked BL...
We present multi-wavelength observations by Chandrayaan-2/XSM, SDO/AIA and Hinode/XRT of a B-class f...