Isuru Gunawardhana
ORCID:
0000-0001-5583-0499
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About
Contact & Profiles
Research Areas
- Astrophysics and Cosmic Phenomena
- Radio Astronomy Observations and Technology
- Particle physics theoretical and experimental studies
- Particle Detector Development and Performance
- Dark Matter and Cosmic Phenomena
University of Utah
2018
A. U. Abeysekara
W. Benbow
R. Bird
T. Brantseg
Robert Brose
and 72
more
M. Buchovecky
J. H. Buckley
V. Bugaev
M. P. Connolly
Wei Cui
M. K. Daniel
A. Falcone
Q. Feng
J. P. Finley
L. Fortson
A. Furniss
G. H. Gillanders
Isuru Gunawardhana
Moritz Hütten
D. Hanna
O. Hervet
J. Holder
G. Hughes
T. B. Humensky
C. A. Johnson
P. Kaaret
P. Kar
M. Kertzman
F. Krennrich
M. J. Lang
T. T. Y. Lin
S. McArthur
P. Moriarty
R. Mukherjee
S. O’Brien
R. A. Ong
A. N. Otte
N. Park
A. Petrashyk
M. Pohl
E. Pueschel
J. Quinn
K. Ragan
P. T. Reynolds
G. T. Richards
E. Roache
C. B. Rulten
I. Sadeh
M. Santander
G. H. Sembroski
K. Shahinyan
S. P. Wakely
A. J. Weinstein
R. M. Wells
P. Wilcox
D. A. Williams
B. Zitzer
S. G. Jorstad
Alan P. Marscher
M. L. Lister
Y. Y. Kovalev
A. B. Pushkarev
T. Savolainen
I. Agudo
S. N. Molina
José L. Gómez
V. M. Larionov
Г. А. Борман
A. A. Mokrushina
M. Tornikoski
A. Lähteenmäki
Wara Chamani
S. Enestam
S. Kiehlmann
T. Hovatta
Paul S. Smith
P. Pontrelli
Combined with very-long-baseline interferometry measurements, the observations of fast TeV gamma-ray flares probe structure and emission mechanism blazar jets. However, only a handful such have been detected to date, within last few years these observed from lower-frequency-peaked BL~Lac objects flat-spectrum radio quasars. We report on flare BL~Lacertae by VERITAS, rise time $\sim$2.3~hr decay $\sim$36~min. The peak flux above 200 GeV is $(4.2 \pm 0.6) \times 10^{-6} \;\text{photon}...
10.3847/1538-4357/aab35c
article
EN
The Astrophysical Journal
2018-03-28
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