W. Kells

Erratum: “Searches for Continuous Gravitational Waves from Nine Young Supernova Remnants” (2015, ApJ, 813, 39) *

J. Aasi, B. P. Abbott, R. Abbott, T. D. Abbott et autres

Equation (7) of the published article (Aasi et al. 2015) is in error; it should read (Equation presented). The upper limits on ò presented in the published article are unaffected by this error. Equation (8) of the published article is in error; …

us, it, fr, gb, de, nl, br, in, pl, ru, au, hu (code pays fourni par la source)

FIRST SEARCHES FOR OPTICAL COUNTERPARTS TO GRAVITATIONAL-WAVE CANDIDATE EVENTS

E. Chassande‐Mottin, M. Drago, E. K. Gustafson, L. Austin et autres

During the LIGO and Virgo joint science runs in 2009-2010, gravitational wave (GW) data from three interferometer detectors were analyzed within minutes to select GW candidate events and infer their apparent sky positions. Target coordinates were transmitted to several telescopes for follow-up …

Assessing accuracy of waveform models to best interpret GW150914

B. P. Abbott, Robert Abbott, T. D. Abbott, M. R. Abernathy et autres

We report here the non-detection of gravitational waves from the merger of binary neutron star systems and neutron-star--black-hole systems during the first observing run of Advanced LIGO. In particular we searched for gravitational wave signals from binary neutron star systems with component …

de (code pays fourni par la source)

Sensitivity of the Advanced LIGO detectors at the beginning of gravitational wave astronomy

Д. В. Мартынов, E. D. Hall, B. P. Abbott, R. Abbott et autres

The Laser Interferometer Gravitational Wave Observatory (LIGO) consists of two widely separated 4 km laser interferometers designed to detect gravitational waves from distant astrophysical sources in the frequency range from 10 Hz to 10 kHz. The first observation run of the Advanced …

us, gb, au, de, it (code pays fourni par la source)

Searching for stochastic gravitational waves using data from the two colocated LIGO Hanford detectors

J. Aasi, J. Abadie, B. P. Abbott, R. Abbott et autres

Searches for a stochastic gravitational-wave background (SGWB) using terrestrial detectors typically involve cross-correlating data from pairs of detectors. The sensitivity of such cross-correlation analyses depends, among other things, on the separation between the two detectors: the smaller the separation, the better the …

us, fr, it, gb, de, nl, br, ru, au (code pays fourni par la source)

A gravitational wave observatory operating beyond the quantum shot-noise limit

J. Abadie, B. P. Abbott, R. Abbott, T. D. Abbott et autres

us, gb, de, au, ru, ca, cn, kr (code pays fourni par la source)

Search for gravitational waves from compact binary coalescence in LIGO and Virgo data from S5 and VSR1

J. Abadie, B. P. Abbott, R. Abbott, M. R. Abernathy et autres

We report the results of the first search for gravitational waves from compact binary coalescence using data from the Laser Interferometer Gravitational-Wave Observatory and Virgo detectors. Five months of data were collected during the Laser Interferometer Gravitational-Wave Observatory's S5 and Virgo's VSR1 …

us, gb, fr, it, de, au, nl, ru, pl (code pays fourni par la source)