The comparison of the models with the DECam detection limits suggests good detection chances in two or three filters out to ∼230 Mpc under polar viewing angles ...
The GW candidate S190510g was discovered and initially classified as a binary neutron star (BNS) merger with 98% probability.
This Letter describes our DECam observations and our real-time analysis results, focusing in particular on the design and implementation of the observing ...
On 2019 May 10 02:59:39.292 UT the GW candidate S190510g was discovered and initially classified as a binary neutron star (BNS) merger with 98% probability. The ...
This Letter describes our DECam observations and our real-time analysis results, focusing in particular on the design and implementation of the observing ...
Dive into the research topics of 'GROWTH on S190510g: DECam Observation planning and follow-up of a distant binary neutron star merger candidate'. Together they ...
GROWTH acknowledges generous support of the NSF under PIRE Grant No 1545949. An optimized schedule was generated using the ToO marshal system (Coughlin et al.
GCN Circular 24493. Subject. LIGO/Virgo S190510g: KMTNet observation of DECam-GROWTH and DESGW candidates. Date. 2019-05-11T23:37:09Z (5 years ago). From.
Aug 9, 2019 ˇ On 2019 May 10 02:59:39.292 UT the GW candidate S190510g was discovered and initially classified as a binary neutron star (BNS) merger with 98% ...
Mar 11, 2020 ˇ Our infrastructure enabled us to conduct observations of two events during O3a, S190426c and S190510g. Furthermore, our analysis of deep ...
