Due to the overwhelming background of atmospheric muons, the traditional IceCube point source search in the Southern Hemisphere is mainly sensitive to neutrinos with energies above 100TeV. A new approach focuses on events starting inside the instrumented volume. By utilizing different veto techniques we are able to significantly reduce the energy threshold and can now for the first time explore the entire Southern Hemisphere at neutrino energies as low as 100GeV. We present the results of two analyses targeting slightly different energy ranges. Both use one year of data taken with the completed IceCube detector in 2011/12
Observation of a point source of astrophysical neutrinos would be a "smoking gun" signature of a cos...
Observation of a point source of astrophysical neutrinos would be a“smoking gun”signature of a cosmi...
Observation of a point source of astrophysical neutrinos would be a “smoking gun” signature of a cos...
Due to the overwhelming background of atmospheric muons, the traditional IceCube point source search...
Due to the overwhelming background of atmospheric muons, the traditional IceCube point source search...
Due to the overwhelming background of atmospheric muons, the traditional IceCube point source search...
Due to the overwhelming background of atmospheric muons, the traditional IceCube point source search...
Due to the overwhelming background of atmospheric muons, the traditional IceCube point source search...
Due to the overwhelming background of atmospheric muons, the traditional IceCube point source search...
© 2019 Many Galactic sources of gamma rays, such as supernova remnants, are expected to produce neut...
© 2019 Many Galactic sources of gamma rays, such as supernova remnants, are expected to produce neut...
Many Galactic sources of gamma rays, such as supernova remnants, are expected to produce neutrinos w...
Many Galactic sources of gamma rays, such as supernova remnants, are expected to produce neutrinos w...
Many Galactic sources of gamma rays, such as supernova remnants, are expected to produce neutrinos w...
Many Galactic sources of gamma rays, such as supernova remnants, are expected to produce neutrinos w...
Observation of a point source of astrophysical neutrinos would be a "smoking gun" signature of a cos...
Observation of a point source of astrophysical neutrinos would be a“smoking gun”signature of a cosmi...
Observation of a point source of astrophysical neutrinos would be a “smoking gun” signature of a cos...
Due to the overwhelming background of atmospheric muons, the traditional IceCube point source search...
Due to the overwhelming background of atmospheric muons, the traditional IceCube point source search...
Due to the overwhelming background of atmospheric muons, the traditional IceCube point source search...
Due to the overwhelming background of atmospheric muons, the traditional IceCube point source search...
Due to the overwhelming background of atmospheric muons, the traditional IceCube point source search...
Due to the overwhelming background of atmospheric muons, the traditional IceCube point source search...
© 2019 Many Galactic sources of gamma rays, such as supernova remnants, are expected to produce neut...
© 2019 Many Galactic sources of gamma rays, such as supernova remnants, are expected to produce neut...
Many Galactic sources of gamma rays, such as supernova remnants, are expected to produce neutrinos w...
Many Galactic sources of gamma rays, such as supernova remnants, are expected to produce neutrinos w...
Many Galactic sources of gamma rays, such as supernova remnants, are expected to produce neutrinos w...
Many Galactic sources of gamma rays, such as supernova remnants, are expected to produce neutrinos w...
Observation of a point source of astrophysical neutrinos would be a "smoking gun" signature of a cos...
Observation of a point source of astrophysical neutrinos would be a“smoking gun”signature of a cosmi...
Observation of a point source of astrophysical neutrinos would be a “smoking gun” signature of a cos...