GCN Circular 24617

S. Nakahira (RIKEN),  A. Yoshida, T. Sakamoto, V. Pal'shin,
S. Sugita (AGU), Y. Kawakubo (LSU), K. Yamaoka (Nagoya U),
Y. Asaoka, S. Ozawa, S. Torii (Waseda U), Y. Shimizu,
T. Tamura (Kanagawa U), N. Cannady (GSFC/UMBC),
M. L. Cherry (LSU), S. Ricciarini (U of Florence),
P. S. Marrocchesi (U of Siena),
and the CALET collaboration:

The CALET Gamma-ray Burst Monitor (CGBM) was operating at the
trigger time of S190519bj T0 = 2019-05-19 15:35:44.398  UT (The
LIGO Scientific Collaboration and Virgo Collaboration, GCN Circ.
24598
Not found
 
 
).

No CGBM on-board trigger occurred around the event time.  Based
on the LIGO-Virgo localization sky map, most of the high  probability
area was within the field-of-view of the CGBM SGM.  The summed
LIGO probabilities inside the CGBM HXM (7-3000 keV) and SGM
(40 keV - 28 MeV)  fields of view are 32% and 87%, respectively
(and 100% credible region of the initial localization map was above
the horizon).  The HXM and SGM fields of view were centered at
RA = 244.6 deg, Dec = 61.1 deg and  RA = 243.1 deg, Dec = 51.1 deg
at T0, respectively.

Based on the analysis of the light curve data with 0.125 sec
time resolution from T0-60 sec to T0+60 sec, we found no
significant excess (signal-to-noise ratio >= 7) around the trigger
time in either the HXM or the SGM data.

The CALET Calorimeter (CAL) was operating in the high energy
trigger mode at the trigger time of S190519bj. Using CAL data,
we have searched for gamma-ray events in the 10-100 GeV
band from -60 sec to +60 sec from the GW trigger time and
found no candidates. There is no significant overlap with the LVC
location probability map.  The CAL FOV was centered
at RA=243.1 deg, Dec=51.1 deg at T0.

[GCN OPS NOTE(21may19): Per author's request, "S190519bj" was edded
to the Subject line.]