[vsnet-grb-info 24832] LIGO/Virgo S200129m: upper limits from AGILE/GRID observations
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Wed Jan 29 18:43:46 JST 2020
TITLE: GCN CIRCULAR
NUMBER: 26931
SUBJECT: LIGO/Virgo S200129m: upper limits from AGILE/GRID observations
DATE: 20/01/29 09:38:59 GMT
FROM: Carlotta Pittori at ASI SSDC, INAF-OAR <carlotta.pittori at ssdc.asi.it>
C. Pittori, F. Verrecchia (SSDC, and INAF/OAR), M. Tavani (INAF/IAPS, and
Univ. Roma Tor Vergata), M. Cardillo, C. Casentini, G. Piano, A. Ursi (INAF/IAPS),
F. Lucarelli (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 S200129m at T0 = 2020-01-29
06:54:58.435 (UT) a preliminary analysis of the AGILE exposure at T0 shows that
the Gamma-Ray Imaging Detector (GRID) exposure covered less than 10% of
the 90% c.l. localization region (LR) (due to 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
S200129m 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 8.3e-07 to 9.1e-06 erg cm^-2 s^-1, with exposure of about 51% of the LR over
the time interval ( T0 + 100s ; T0 + 200s );
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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