Characterization of the LIGO detectors during their sixth science run - Test2 - elhamkhani - TriplyDB

Characterization of the LIGO detectors during their sixth science run

Characterization of the LIGO detectors during their sixth science run

http://www.wikidata.org/entity/Q56977510

about

All-sky search for long-duration gravitational wave transients with initial LIGO Terrestrial Gravity Fluctuations.LIGO and the opening of a unique observational window on the universe.The Advanced LIGO photon calibrators.Electromagnetic evidence that SSS17a is the result of a binary neutron star merger.An instrument to measure mechanical up-conversion phenomena in metals in the elastic regime.Effects of transients in LIGO suspensions on searches for gravitational waves.Maximum Redshift of Gravitational Wave Merger Events.Stochastic Gravitational-Wave Background due to Primordial Binary Black Hole Mergers.Effects of Neutron-Star Dynamic Tides on Gravitational Waveforms within the Effective-One-Body Approach.Digging Deeper: Observing Primordial Gravitational Waves below the Binary-Black-Hole-Produced Stochastic Background.Search of the Orion spur for continuous gravitational waves using a loosely coherent algorithm on data from LIGO interferometers High-precision timing of 42 millisecond pulsars with the European Pulsar Timing Array Equation of state effects on gravitational waves from rotating core collapse The Mario Schenberg Gravitational Wave Antenna The unpolarized macronova associated with the gravitational wave event GW 170817 First targeted search for gravitational-wave bursts from core-collapse supernovae in data of first-generation laser interferometer detectors Local-oscillator noise coupling in balanced homodyne readout for advanced gravitational wave detectors Robust semicoherent searches for continuous gravitational waves with noise and signal models including hours to days long transients Binary black hole merger rates inferred from luminosity function of ultra-luminous X-ray sources Merging binary black holes formed through chemically homogeneous evolution in short-period stellar binaries Updated constraints and forecasts on primordial tensor modes

P2860

Q27012477-4628624C-E918-46BA-8BDA-075FD1167B3D Q30363978-FE23CF77-F653-44F1-B201-38FC721577EF Q36304926-1918DEBC-594D-420B-8277-68B9A7C9D02B Q45952444-D23DF94C-40A2-4030-BB27-F9E94E52C32D Q46296995-13469B50-5E9F-4948-8DAD-A39FEC73FE3F Q46688431-0086B1B5-46E2-46E9-830C-D3FB1B15210B Q47230785-00396EB6-9D1C-4ACF-BD2F-5E93E60020C9 Q49495129-5DF7A458-958E-40AC-9D49-D2237CDD5249 Q50859324-35CD37AE-F624-417E-9D02-77BC69284353 Q53095812-F345F3F9-EA4F-4DA6-805F-167B306CE0D2 Q53113007-515D6679-5AD9-46CA-92FA-0E33FDAA0379 Q56977458-21402096-A8B4-49F6-9164-0461628FFDE0 Q57201111-2F7E0572-A640-4458-94C9-4D7BE7464199 Q57426809-4D82B71E-50A1-453F-9D5A-FD5E0F3729D4 Q57483875-6CB2283A-D871-4DF0-A2FB-E1CCA34C5983 Q57559635-F0E26C8D-6AE2-423F-B632-5CAD9ACEF0DE Q57562025-0D893617-F8E1-406B-8676-C198A6312198 Q57591062-076BF99C-F5C2-487D-9A7D-3584B981212C Q57692543-E028839D-AC23-43B0-BEDE-F191DF7808B9 Q58907512-A9AA151C-BD7F-4269-B58E-8CABB0EC8F99 Q59093335-8FC89F52-B956-49B4-B076-3CECDD8FCB02 Q59237380-A3166CEA-4936-4191-A355-BF76EF157E14

P2860

Characterization of the LIGO detectors during their sixth science run

http://www.wikidata.org/entity/Q56977510

description

2015 nî lūn-bûn

@nan

2015年の論文

@ja

2015年学术文章

@wuu

2015年学术文章

@zh

2015年学术文章

@zh-cn

2015年学术文章

@zh-hans

2015年学术文章

@zh-my

2015年学术文章

@zh-sg

2015年學術文章

@yue

2015年學術文章

@zh-hant

name

Characterization of the LIGO detectors during their sixth science run

@en

Characterization of the LIGO detectors during their sixth science run

@nl

type

label

Characterization of the LIGO detectors during their sixth science run

@en

Characterization of the LIGO detectors during their sixth science run

@nl

prefLabel

Characterization of the LIGO detectors during their sixth science run

@en

Characterization of the LIGO detectors during their sixth science run

@nl

P1433

Q56977510-65EB4189-F4BE-402D-854A-D801FA9962DE

P1476

Q56977510-7774948A-3C5E-47FB-A89F-8A422543D55E

P2093

Q56977510-00756FC6-7416-47F1-B7F2-02AF2FEF8B70

Q56977510-009841A6-07A9-4504-8920-06FE77D81580

Q56977510-00985863-D615-435F-89B7-B1370EAA5DA4

Q56977510-009DAF04-D426-40CB-A086-B3E55D404909

Q56977510-01312D8F-66E2-415C-8C6E-6586D1E66089

Q56977510-0180F3C6-298B-49E7-8AA2-288749CC211D

Q56977510-01D53087-F4EE-4592-8B98-03D4C8D7E62E

Q56977510-0295B06E-0914-4987-B9E3-175182924448

Q56977510-02D0955D-8DD2-42AF-AFB5-B72156156C46

Q56977510-02D7E91D-6066-45CE-ADAA-4710F45399FB

P304

Q56977510-D497D013-676A-4882-A771-38CD9DD07884

P31

Q56977510-7A20F60D-23E0-4B68-8E4A-7DFF58EEF784

P356

Q56977510-678EACB5-5B71-4C12-9D22-E26AB1394030

P407

Q56977510-C35A94EB-2261-4262-9162-3289F2B8A266

P433

Q56977510-87E952F3-158C-47DC-A6DB-B2E9097EC1C6

P478

Q56977510-85F1D84C-26C5-479D-92E3-6656B32D2A48

P50

Q56977510-05675DD9-6BDF-40E4-8CDA-883D2C5FB6E8

Q56977510-0DCD6085-C679-4578-A806-EAD0AD1F3D82

Q56977510-113A2111-4B07-43AF-A414-6E9E8919FAF2

Q56977510-116222EA-F859-452F-B75D-0605C31F10A6

Q56977510-1504E753-127C-4DCA-B70A-EEEB954AE125

Q56977510-1531F8B3-ED77-4AFA-8C5A-4BD9D7514E4F

Q56977510-1A68A9E9-14DA-4936-956A-86E9FB5116B5

Q56977510-1C998371-D944-4346-B23C-F8DC8E2DCF37

Q56977510-1D1BF489-CE8C-4BE2-835F-30AF8CBCA4BC

Q56977510-21F8F2EF-DCD9-4517-85E2-C288F627FE74

P577

Q56977510-D89E78AC-A983-4E90-8681-DAAABB91103C

P818

Q56977510-9B338A72-2517-45A3-ABB8-AFE28D6ED129

P356

P1433

Classical and Quantum Gravity

P1476

Characterization of the LIGO detectors during their sixth science run

@en

P2093

A A van Veggel

http://www.w3.org/2001/XMLSchema#string

A Allocca

http://www.w3.org/2001/XMLSchema#string

A Basti

http://www.w3.org/2001/XMLSchema#string

A Brillet

http://www.w3.org/2001/XMLSchema#string

A Buonanno

http://www.w3.org/2001/XMLSchema#string

A C Lin

http://www.w3.org/2001/XMLSchema#string

A Castiglia

http://www.w3.org/2001/XMLSchema#string

A Chiummo

http://www.w3.org/2001/XMLSchema#string

A Colla

http://www.w3.org/2001/XMLSchema#string

A Conte

http://www.w3.org/2001/XMLSchema#string

P304

115012

http://www.w3.org/2001/XMLSchema#string

P31

scholarly article

P356

10.1088/0264-9381/32/11/115012

http://www.w3.org/2001/XMLSchema#string

P407

P433

11

http://www.w3.org/2001/XMLSchema#string

P478

32

http://www.w3.org/2001/XMLSchema#string

P50

Karsten Danzmann

David McClelland

Andrea Chincarini

P577

2015-05-13T00:00:00Z

http://www.w3.org/2001/XMLSchema#dateTime

P818

1410.7764

http://www.w3.org/2001/XMLSchema#string