about
Methods and results of a search for gravitational waves associated with gamma-ray bursts using the GEO 600, LIGO, and Virgo detectorsSearch for gravitational radiation from intermediate mass black hole binaries in data from the second LIGO-Virgo joint science runImproved Upper Limits on the Stochastic Gravitational-Wave Background from 2009–2010 LIGO and Virgo DataSearch for Gravitational Waves Associated with γ -ray Bursts Detected by the Interplanetary NetworkDirected search for gravitational waves from Scorpius X-1 with initial LIGO dataNarrow-band search of continuous gravitational-wave signals from Crab and Vela pulsars in Virgo VSR4 dataMultimessenger search for sources of gravitational waves and high-energy neutrinos: Initial results for LIGO-Virgo and IceCubeFirst all-sky search for continuous gravitational waves from unknown sources in binary systemsObservation of Gravitational Waves from a Binary Black Hole MergerSearch for transient gravitational waves in coincidence with short-duration radio transients during 2007–2013All-sky search for long-duration gravitational wave transients with initial LIGOGW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole CoalescenceGW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO and Advanced Virgo.Astrophysical Implications of the Binary Black-hole Merger GW150914GW150914: Implications for the Stochastic Gravitational-Wave Background from Binary Black HolesGW150914: The Advanced LIGO Detectors in the Era of First DiscoveriesGW150914: First results from the search for binary black hole coalescence with Advanced LIGOCalibration of the Advanced LIGO detectors for the discovery of the binary black-hole merger GW150914Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914Directly comparing GW150914 with numerical solutions of Einstein's equations for binary black hole coalescenceHigh-energy neutrino follow-up search of gravitational wave event GW150914 with ANTARES and IceCubeImproved Analysis of GW150914 Using a Fully Spin-Precessing Waveform ModelLocalization and Broadband Follow-up of the Gravitational-wave Transient GW150914Observing gravitational-wave transient GW150914 with minimal assumptionsProperties of the Binary Black Hole Merger GW150914Tests of General Relativity with GW150914The basic physics of the binary black hole merger GW150914GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral.Testing the Binary Black Hole Nature of a Compact Binary Coalescence.GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence.Directional Limits on Persistent Gravitational Waves from Advanced LIGO's First Observing Run.Upper Limits on the Stochastic Gravitational-Wave Background from Advanced LIGO's First Observing Run.Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817AAll-sky search for periodic gravitational waves in the O1 LIGO dataAll-sky search for short gravitational-wave bursts in the first Advanced LIGO runSupplement: "Localization and broadband follow-up of the gravitational-wave transient GW150914" (2016, ApJL, 826, L13)Results of the deepest all-sky survey for continuous gravitational waves on LIGO S6 data running on the Einstein@Home volunteer distributed computing projectSearch for High-energy Neutrinos from Binary Neutron Star Merger GW170817 with ANTARES, IceCube, and the Pierre Auger ObservatoryOn the Progenitor of Binary Neutron Star Merger GW170817
P50
Q21651192-F428CE99-C4F9-40BA-BA1C-BAC7102A159AQ21651199-62A0CBDB-96E2-4886-B6D6-D4EA396C8E05Q21706450-A7C9E793-477F-415F-988D-988B3315A8E5Q21706456-25E0370C-6E5D-4794-8955-A90445E2D17FQ21706633-62394981-7A92-4E06-A6D9-F2395562B4F3Q21706636-5D719028-4C17-412F-A50D-2249E0D4B575Q21706639-697321D0-30D2-488E-9EB8-75D0323397F0Q21706727-EA836F32-F44D-4417-B295-E0CD856B5127Q22683203-FB066746-EFD7-4010-806A-565C55B06E68Q27012407-2D633291-B5E8-4575-9EE9-7EE1F882331EQ27012477-8302239F-792D-48A5-80F6-224611C8DB8DQ28276820-C616C177-4BA9-46F9-AC68-580E890AB56CQ30105981-E5CA82C5-142B-453F-8EC8-FDC1BEB1418DQ37599384-196FCACB-C7A0-4454-9C26-6C57F7A17387Q40872682-CEB22E79-D7F6-46C8-B393-16BFAEB43643Q40889477-CEDE7684-93DA-4547-8529-94074824E5ADQ40895055-518C8F1B-2D45-41C0-97AD-AFE1684E4257Q40905577-34FAAE16-B786-4FC7-9B85-685C1308A5E2Q40906231-55389183-64F6-4F10-873A-B4C40ED9C762Q40906734-FF6D508D-3E1E-4652-80D1-996F643FE771Q40907000-E5BF301D-2FD9-43BA-84A0-59C3B5B4CC78Q40907274-026D3E33-BE01-47FE-9026-FC3AE5ADDD18Q40907552-4458BD9E-03F8-40EA-A76C-D00C50381E52Q40907824-E6933FBB-4783-4648-8335-5A88BB959A8BQ40908135-446EF551-1514-4F3F-981A-E8089244A67CQ40908347-22EADE4E-33A1-4F75-8446-470642CF548EQ40908744-91549EBD-A57E-4D33-945D-30AB617F60B9Q40909180-972E043D-1CBA-4910-8182-1D1C3DA9BF87Q42119679-AC010883-7299-40ED-B1FC-E23576050E7DQ49828294-F0BFDF77-885E-41EB-A2A8-F2D0E149CF9FQ50101879-0446C0EE-7C91-400A-91C0-B379A02E0CF1Q50204272-45675E64-615A-47BC-9E16-4F9D2FF50775Q50204280-11E92CCC-A50B-4AA0-A208-58CEA314B849Q51786082-AFA08931-3CCB-4AA1-A002-4C652D90D88EQ54935716-28814BB0-0A68-405C-AA07-514ED90C5C7EQ55031754-3BD7B9C1-2601-47AC-BE40-B88FFDF8FA93Q55450887-0D2069EE-09B0-4BBA-9BF8-C0F888F83F45Q56475490-2258A50F-679B-4CF5-B19A-5D43E8B1AC89Q56595381-AE16D551-5BF6-4880-B7EE-550C8E1F1AD0Q56854744-6446FBDC-CDAE-487D-8E35-9DD8DABC2160
P50
description
hulumtues
@sq
onderzoeker
@nl
researcher
@en
հետազոտող
@hy
name
C. Mishra
@nl
C. Mishra
@sl
Chandra Kant Mishra
@en
Chandra Kant Mishra
@es
type
label
C. Mishra
@nl
C. Mishra
@sl
Chandra Kant Mishra
@en
Chandra Kant Mishra
@es
altLabel
C Mishra
@en
C. Mishra
@en
Mishra C
@en
prefLabel
C. Mishra
@nl
C. Mishra
@sl
Chandra Kant Mishra
@en
Chandra Kant Mishra
@es
P106
P1153
36195865100
P21
P31
P496
0000-0002-8115-8728