[vsnet-grb-info 22843] LIGO/Virgo S190630ag: No counterpart candidates in AGILE-GRID observations
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Tue Jul 2 01:08:49 JST 2019
TITLE: GCN CIRCULAR
NUMBER: 24942
SUBJECT: LIGO/Virgo S190630ag: No counterpart candidates in AGILE-GRID observations
DATE: 19/07/01 16:07:45 GMT
FROM: Carlotta Pittori at ASI SSDC, INAF-OAR <carlotta.pittori at ssdc.asi.it>
C. Pittori (SSDC, and INAF/OAR), A. Ursi (INAF/IAPS), M. Tavani
(INAF/IAPS, and Univ. Roma Tor Vergata), M. Cardillo, C. Casentini, G.
Piano (INAF/IAPS), F. Lucarelli, F. Verrecchia (SSDC, and INAF/OAR),
A. Bulgarelli, V. Fioretti, N. Parmiggiani (INAF/OAS-Bologna), M.
Pilia (INAF/OA-Cagliari), F. Longo (Univ. Trieste, and INFN Trieste),
report on behalf of the AGILE Team:
In response to the LIGO-Virgo GW event S190630ag at T0 = 2019-06-30 18:52:05.180
UTC a preliminary analysis of the AGILE exposure at T0 shows that
the Gamma-Ray Imaging Detector (GRID) exposure covered less than 20%
of the 90% c.l. localization region (LR) (due to Earth occultation
and Solar Panel constraints).
We performed an analysis of the GRID data in the energy range 50 MeV
-10 GeV over time intervals before and after T0, where good exposure of
the S190630ag 90% c.l. LR was available.
No candidate gamma-ray transient was detected.
The following preliminary GRID values of 3-sigma upper limit (UL) are obtained:
from 5.9e-08 to 5.5e-06 erg cm^-2 s^-1, with exposure of about 42% of the LR
over the time interval ( T0 -200s ; T0 -100s ).
These measurements were obtained with AGILE observing a large portion of
the sky in spinning mode. Additional analysis of AGILE data is in progress.
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