GCN Circular 18231
Subject
ANTARES neutrino detection and possible Swift X-ray counterpart
Date
2015-09-03T11:43:31Z (9 years ago)
From
Phil Evans at U of Leicester <pae9@leicester.ac.uk>
D. Dornic (CPPM), S. Basa (LAM), P.A. Evans (U. Leicester), J.A. Kennea
(PSU), J.P. Osborne (U. Leicester) and V. Lipunov (MSU) report on behalf
of the ANTARES Collaboration, the Swift-XRT team and MASTER team:
September 1st, 2015, at 07:38:25 UT, ANTARES has detected a bright
neutrino at a location of:
RA(J2000) = 16h 25m 42s
DEC (J2000) = -27d 23m 24s
with an uncertainty of 18 arcmin (radius, 50% containment)
A target of opportunity alert has been sent immediately to Swift. The
XRT onboard Swift followed the ANTARES error box 10 hours after the
neutrino detection. An uncatalogued X-ray source has been detected above
the limit of RASS, with the flux varying between 5e-13 and 1.4e-12 erg
cm^-2 s^-1 (0.3-10 keV), at location:
RA(J2000) = 16h 26m 2.12s
DEC (J2000) = -27d 18m 14.8s
with an uncertainty of 2.4 arcsec (radius, 90% containment).
The detected X-ray source seems to be variable. By contrast no
transient source in the visible domain with MASTER SAAO has been
observed so far until the magnitude 18.5 with a galactic extinction of
2 (Schlegel et al). Further Swift observations have been planned.
We encourage strongly further multi-wavelength observations to identify
this X-ray source.