LAT high-energy photons: other sources

Current trigger threshold: 3 photons above 30 GeV in a 24 hr window. (Blue line shows the most recent 24 hr at 30 GeV)

CrabNebula

T CrB

4FGL J1532.0+3016

PKS1217+02

TXS0836+182

SN2023ixf

4FGLJ1731.6+0630

SN2022jli

NGC4278

3C138

LS I +61 303

TXS1303+113

AGLJ2114+6249

AT2023cvb

AT2023clx

NuEm-230313A

GRB 221009A

4FGL J0816.9+2050

B3_2247+381

IceCube-211125A

4C+39p12

Fermi J0008+6829

4FGL J0009.2+6847

Fermi J0330.1+3743

SGR1935+2154

SN2020tcw

AT2019qwf

GRB190501A

CGRaBS_J0017_0512

B2_0200+30

CGRaBS_J0211+1051

CRATES_J0422_0643

1H_0323+342

4C_+56p27

4C_+06p21

PKS_0507+17

CLASS_J0517+0858

CLASS_J0713+1935

PKS_0736+01

SBS_0846+513

OJ_287

B2_0912+29

PMN_J0948+0022

M_82

4C_+55p17

3FGL_J1039

SBS_1150+497

3C264

M_87

NGC1218

PKS_1502+036

PKS_1509+022

PKS_1546+027

NRAO_512

CGRaBS_J1700+6830

PKS_1725+044

CRATES_J1818+0903

NVSS_J220941-045111

CGRaBS_J2334+0736

A detailed description of our Fermi-LAT analysis algorithms can be found here and here.

VERITAS research at Barnard is supported by the U.S. National Science Foundation.
This website was created by Manel Errando (errando (at) physics.wustl.edu), and maintained by Qi Feng (qifeng (at) nevis.columbia.edu).

Contact

Qi Feng
Nevis Labs / Barnard College / Columbia University
136 S Broadway, Irvington, NY 10533, USA
email: qifeng (at) nevis.columbia.edu