papers

Publications (66)

gr-qc2011

Search for gravitational waves from binary black hole inspiral, merger and ringdown

The LIGO Scientific Collaboration, the Virgo Collaboration, J. Abadie +721

We present the first modeled search for gravitational waves using the complete binary black hole gravitational waveform from inspiral through the merger and ringdown for binaries w…

astro-ph2006

The frontier of darkness: the cases of GRB 040223, GRB 040422, GRB 040624

P. D'Avanzo, P. Filliatre, P. Goldoni +23

Understanding the reasons for the faintness of the optical/near-infrared afterglows of the so-called dark bursts is essential to assess whether they form a subclass of GRBs, and he…

astro-ph.HE2012

Search for gravitational waves associated with gamma-ray bursts during LIGO science run 6 and Virgo science runs 2 and 3

The LIGO Scientific Collaboration, Virgo Collaboration, J. Abadie +807

We present the results of a search for gravitational waves associated with 154 gamma-ray bursts (GRBs) that were detected by satellite-based gamma-ray experiments in 2009-2010, dur…

astro-ph2005

The weak INTEGRAL bursts GRB040223 and GRB040624: an emerging population of dark afterglows

P. Filliatre, S. Covino, P. D'Avanzo +18

We report here gamma-ray, X-ray and near-infrared observations of GRB040223 along with gamma-ray and optical observations of GRB040624. GRB040223 was detected by INTEGRAL close to…

astro-ph.CO2011

Planck early results. III. First assessment of the Low Frequency Instrument in-flight performance

A. Mennella, M. Bersanelli, R. C. Butler +158

The scientific performance of the Planck Low Frequency Instrument (LFI) after one year of in-orbit operation is presented. We describe the main optical parameters and discuss photo…

astro-ph2007

Polarisation studies of the prompt gamma-ray emission from GRB 041219a using the Spectrometer aboard INTEGRAL

S. McGlynn, D. J. Clark, A. J. Dean +6

The spectrometer aboard INTEGRAL, SPI, has the capability to detect the signature of polarised emission from a bright gamma-ray source. GRB 041219a is the most intense burst locali…

gr-qc2010

Sensitivity to Gravitational Waves from Compact Binary Coalescences Achieved during LIGO's Fifth and Virgo's First Science Run

The LIGO Scientific Collaboration, the Virgo Collaboration, J. Abadie +707

We summarize the sensitivity achieved by the LIGO and Virgo gravitational wave detectors for compact binary coalescence (CBC) searches during LIGO's fifth science run and Virgo's f…

astro-ph.IM2012

Planck Early Results. II. The thermal performance of Planck

Planck Collaboration, P. A. R. Ade, N. Aghanim +225

The performance of the Planck instruments in space is enabled by their low operating temperatures, 20K for LFI and 0.1K for HFI, achieved through a combination of passive radiative…

astro-ph.CO2009

The INTEGRAL view of Gamma-Ray Bursts

P. Ubertini, A. Corsi, S. Foley +3

After more than six and half years in orbit, the ESA space observatory INTEGRAL has provided new, exciting results in the soft gamma-ray energy range (from a few keV to a few MeV).…

gr-qc2012

The characterization of Virgo data and its impact on gravitational-wave searches

J. Aasi, J. Abadie, B. P. Abbott +798

Between 2007 and 2010 Virgo collected data in coincidence with the LIGO and GEO gravitational-wave (GW) detectors. These data have been searched for GWs emitted by cataclysmic phen…

astro-ph.HE2010

Searches for gravitational waves from known pulsars with S5 LIGO data

The LIGO Scientific Collaboration, The Virgo Collaboration, B. P. Abbott +678

We present a search for gravitational waves from 116 known millisecond and young pulsars using data from the fifth science run of the LIGO detectors. For this search ephemerides ov…

astro-ph2005

Outshining the quasars at reionisation: The X-ray spectrum and lightcurve of the redshift 6.29 Gamma-Ray Burst GRB050904

D. Watson, J. N. Reeves, J. Hjorth +7

Gamma-ray burst (GRB) 050904 is the most distant X-ray source known, at z=6.295, comparable to the farthest AGN and galaxies. Its X-ray flux decays, but not as a power-law; it is d…

astro-ph.HE2013

A First Search for coincident Gravitational Waves and High Energy Neutrinos using LIGO, Virgo and ANTARES data from 2007

The ANTARES Collaboration, the LIGO Scientific Collaboration, the Virgo Collaboration +959

We present the results of the first search for gravitational wave bursts associated with high energy neutrinos. Together, these messengers could reveal new, hidden sources that are…

astro-ph.HE2013

Evidence for a Photospheric Component in the Prompt Emission of the Short GRB120323A and its Effects on the GRB Hardness-Luminosity Relation

S. Guiriec, F. Daigne, R. Hascoët +12

The short GRB 120323A had the highest flux ever detected with the Fermi/GBM. Here we study its remarkable spectral properties and their evolution using two spectral models: (i) a s…

astro-ph.HE2011

Fermi/GBM observations of the ultra-long GRB 091024: A burst with an optical flash

D. Gruber, T. Krühler, S. Foley +27

In this paper we examine gamma-ray and optical data of GRB 091024, a gamma-ray burst (GRB) with an extremely long duration of T90~1020 s, as observed with the Fermi Gamma-Ray Burst…

gr-qc2012

Search for Gravitational Waves from Intermediate Mass Binary Black Holes

the LIGO Scientific Collaboration, the Virgo Collaboration, J. Abadie +790

We present the results of a weakly modeled burst search for gravitational waves from mergers of non-spinning intermediate mass black holes (IMBH) in the total mass range 100--450 s…

astro-ph.HE2010

Search for gravitational-wave inspiral signals associated with short Gamma-Ray Bursts during LIGO's fifth and Virgo's first science run

The LIGO Scientific Collaboration, the Virgo Collaboration, J. Abadie +665

Progenitor scenarios for short gamma-ray bursts (short GRBs) include coalescenses of two neutron stars or a neutron star and black hole, which would necessarily be accompanied by t…

astro-ph.HE2011

Search for Gravitational Wave Bursts from Six Magnetars

J. Abadie, B. P. Abbott, R. Abbott +765

Soft gamma repeaters (SGRs) and anomalous X-ray pulsars (AXPs) are thought to be magnetars: neutron stars powered by extreme magnetic fields. These rare objects are characterized b…

gr-qc2011

All-sky Search for Periodic Gravitational Waves in the Full S5 LIGO Data

J. Abadie, B. P. Abbott, R. Abbott +794

We report on an all-sky search for periodic gravitational waves in the frequency band 50-800 Hz and with the frequency time derivative in the range of 0 through -6e-9 Hz/s. Such a…

astro-ph.CO2009

High energy emission and polarisation limits for the INTEGRAL burst GRB 061122

S. McGlynn, S. Foley, B. McBreen +6

(Abridged) GRB 061122 is one of the brightest GRBs detected within INTEGRAL's field of view to date. The two gamma-ray detectors on INTEGRAL were used to investigate the spectral c…

astro-ph.IM2018

The Sensitivity of the Advanced LIGO Detectors at the Beginning of Gravitational Wave Astronomy

D. V. Martynov, E. D. Hall, B. P. Abbott +261

The Laser Interferometer Gravitational Wave Observatory (LIGO) consists of two widely separated 4 km laser interferometers designed to detect gravitational waves from distant astro…

astro-ph.HE2013

Identifying the Location in the Host Galaxy of the Short GRB 111117A with the Chandra Sub-arcsecond Position

T. Sakamoto, E. Troja, K. Aoki +31

We present our successful Chandra program designed to identify, with sub-arcsecond accuracy, the X-ray afterglow of the short GRB 111117A, which was discovered by Swift and Fermi.…

astro-ph2008

GRB 070707: the first short gamma-ray burst observed by INTEGRAL

S. McGlynn, S. Foley, S. McBreen +4

INTEGRAL has observed 47 long-duration GRBs (T_90 > 2s) and 1 short-duration GRB (T_90 < 2s) in five years of observation since October 2002. This work presents the properties of t…

astro-ph.IM2012

Implementation and testing of the first prompt search for gravitational wave transients with electromagnetic counterparts

The LIGO Scientific Collaboration, Virgo Collaboration, J. Abadie +815

Aims. A transient astrophysical event observed in both gravitational wave (GW) and electromagnetic (EM) channels would yield rich scientific rewards. A first program initiating EM…

astro-ph.HE2011

Rest-frame properties of 32 gamma-ray bursts observed by the Fermi Gamma-Ray Burst Monitor

D. Gruber, J. Greiner, A. von Kienlin +27

Aims: In this paper we study the main spectral and temporal properties of gamma-ray bursts (GRBs) observed by Fermi/GBM. We investigate these key properties of GRBs in the rest-fra…

astro-ph.HE2012

Swift follow-up observations of candidate gravitational-wave transient events

P. A. Evans, J. K. Fridriksson, N. Gehrels +813

We present the first multi-wavelength follow-up observations of two candidate gravitational-wave (GW) transient events recorded by LIGO and Virgo in their 2009-2010 science run. Th…

astro-ph.IM2014

Localization of Gamma-Ray Bursts using the Fermi Gamma-Ray Burst Monitor

V. Connaughton, M. S. Briggs, A. Goldstein +25

The Fermi Gamma-ray Burst Monitor (GBM) has detected over 1400 Gamma-Ray Bursts (GRBs) since it began science operations in July, 2008. We use a subset of over 300 GRBs localized b…

gr-qc2013

A directed search for continuous Gravitational Waves from the Galactic Center

The LIGO Scientific Collaboration, The Virgo Collaboration, J. Aasi +871

We present the results of a directed search for continuous gravitational waves from unknown, isolated neutron stars in the Galactic Center region, performed on two years of data fr…

astro-ph.IM2011

Planck Early Results: The Planck mission

Planck Collaboration, P. A. R. Ade, N. Aghanim +272

The European Space Agency's Planck satellite was launched on 14 May 2009, and has been surveying the sky stably and continuously since 13 August 2009. Its performance is well in li…

astro-ph2007

Very different X-ray to optical column density ratios in gamma-ray burst afterglows: ionisation in GRB environments

D. Watson, J. Hjorth, J. P. U. Fynbo +4

We compare the HI column densities from Ly-alpha absorption to the metal column densities from X-ray absorption in gamma-ray burst (GRB) afterglows. Eight bursts of seventeen enter…

astro-ph2010

Photometry and spectroscopy of GRB 060526: A detailed study of the afterglow and host galaxy of a z=3.2 gamma-ray burst

C. C. Thöne, D. A. Kann, G. Jóhannesson +58

Aims: With this paper we want to investigate the highly variable afterglow light curve and environment of gamma-ray burst (GRB) 060526 at . Methods: We present one of the…

gr-qc2014

Application of a Hough search for continuous gravitational waves on data from the 5th LIGO science run

The LIGO Scientific Collaboration, The Virgo Collaboration, J. Aasi +876

We report on an all-sky search for periodic gravitational waves in the frequency range with the first derivative of frequency in the range $-8.9 \times 10^{-1…

astro-ph.HE2013

Search for long-lived gravitational-wave transients coincident with long gamma-ray bursts

The LIGO Scientific Collaboration, the Virgo Collaboration, J. Aasi +875

Long gamma-ray bursts (GRBs) have been linked to extreme core-collapse supernovae from massive stars. Gravitational waves (GW) offer a probe of the physics behind long GRBs. We inv…

gr-qc2010

A search for gravitational waves associated with the August 2006 timing glitch of the Vela pulsar

The LIGO Scientific Collaboration, J. Abadie, B. P. Abbott +499

The physical mechanisms responsible for pulsar timing glitches are thought to excite quasi-normal mode oscillations in their parent neutron star that couple to gravitational wave e…

astro-ph.HE2010

Search for gravitational-wave bursts associated with gamma-ray bursts using data from LIGO Science Run 5 and Virgo Science Run 1

LIGO Scientific Collaboration, Virgo Collaboration, B. P. Abbott +665

We present the results of a search for gravitational-wave bursts associated with 137 gamma-ray bursts (GRBs) that were detected by satellite-based gamma-ray experiments during the…

gr-qc2014

Searching for stochastic gravitational waves using data from the two co-located LIGO Hanford detectors

The LIGO Scientific Collaboration, the Virgo Collaboration, J. Aasi +873

Searches for a stochastic gravitational-wave background (SGWB) using terrestrial detectors typically involve cross-correlating data from pairs of detectors. The sensitivity of such…

astro-ph.HE2013

The First Pulse of the Extremely Bright GRB 130427A: A Test Lab for Synchrotron Shocks

R. Preece, J. Michael Burgess, A. von Kienlin +156

Gamma-ray burst (GRB) 130427A is one of the most energetic GRBs ever observed. The initial pulse up to 2.5 s is possibly the brightest well-isolated pulse observed to date. A fine…

gr-qc2012

Upper limits on a stochastic gravitational-wave background using LIGO and Virgo interferometers at 600-1000 Hz

J. Abadie, B. P. Abbott, R. Abbott +782

A stochastic background of gravitational waves is expected to arise from a superposition of many incoherent sources of gravitational waves, of either cosmological or astrophysical…

astro-ph.CO2014

Planck 2013 results. I. Overview of products and scientific results

Planck Collaboration, P. A. R. Ade, N. Aghanim +398

The ESA's Planck satellite, dedicated to studying the early Universe and its subsequent evolution, was launched 14 May 2009 and has been scanning the microwave and submillimetre sk…

astro-ph.HE2012

Implications For The Origin Of GRB 051103 From LIGO Observations

The LIGO Scientific Collaboration, J. Abadie, B. P. Abbott +568

We present the results of a LIGO search for gravitational waves (GWs) associated with GRB 051103, a short-duration hard-spectrum gamma-ray burst (GRB) whose electromagnetically det…

astro-ph2005

The soft X-ray blast in the apparently sub-luminous GRB 031203

D. Watson, S. A. Vaughan, R. Willingale +11

GRB031203 was a very low apparent luminosity gamma-ray burst (GRB). It was also the first GRB with a dust-scattered X-ray halo. The observation of the halo allowed us to infer the…

astro-ph.HE2011

GRIPS - Gamma-Ray Imaging, Polarimetry and Spectroscopy

J. Greiner, K. Mannheim, F. Aharonian +65

We propose to perform a continuously scanning all-sky survey from 200 keV to 80 MeV achieving a sensitivity which is better by a factor of 40 or more compared to the previous missi…

astro-ph2008

The Spectral Lag of GRB060505: A Likely Member of the Long Duration Class

S. McBreen, S. Foley, D. Watson +7

Two long gamma-ray bursts, GRB 060505 and GRB 060614, occurred in nearby galaxies at redshifts of 0.089 and 0.125 respectively. Due to their proximity and durations, deep follow-up…

astro-ph2005

The galaxies in the field of the nearby GRB980425/SN1998bw

S. Foley, D. Watson, J. Gorosabel +5

We present spectroscopic observations of ESO 184-G82, the host galaxy of GRB980425/SN1998bw, and six galaxies in its field. A host redshift of z=0.0087+/-0.0006 is derived, consist…

astro-ph.IM2013

First Searches for Optical Counterparts to Gravitational-wave Candidate Events

The LIGO Scientific Collaboration, the Virgo Collaboration, J. Aasi +904

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 even…

astro-ph.HE2010

Gamma-Ray Bursts Overview

B. McBreen, S. Foley, L. Hanlon

It is now more than 40 years since the discovery of gamma-ray bursts (GRBs) and in the last two decades there has been major progress in the observations of bursts, the afterglows…

gr-qc2010

First search for gravitational waves from the youngest known neutron star

LIGO Scientific Collaboration, J. Abadie, B. P. Abbott +537

We present a search for periodic gravitational waves from the neutron star in the supernova remnant Cassiopeia A. The search coherently analyzes data in a 12-day interval taken fro…

astro-ph.CO2010

Searching for differences in Swift's intermediate GRBs

A. de Ugarte Postigo, I. Horváth, P. Veres +16

Gamma-ray bursts are usually classified through their high-energy emission into short-duration and long-duration bursts, which presumably reflect two different types of progenitors…

astro-ph.CO2011

Directional limits on persistent gravitational waves using LIGO S5 science data

J. Abadie, B. P. Abbott, R. Abbott +712

The gravitational-wave (GW) sky may include nearby pointlike sources as well as astrophysical and cosmological stochastic backgrounds. Since the relative strength and angular distr…

gr-qc2014

Constraints on cosmic strings from the LIGO-Virgo gravitational-wave detectors

J. Aasi, J. Abadie, B. P. Abbott +873

Cosmic strings can give rise to a large variety of interesting astrophysical phenomena. Among them, powerful bursts of gravitational waves (GWs) produced by cusps are a promising o…

gr-qc2012

All-sky search for gravitational-wave bursts in the second joint LIGO-Virgo run

the LIGO Scientific Collaboration, the Virgo Collaboration, J. Abadie +786

We present results from a search for gravitational-wave bursts in the data collected by the LIGO and Virgo detectors between July 7, 2009 and October 20, 2010: data are analyzed wh…

gr-qc2014

Characterization of the LIGO detectors during their sixth science run

The LIGO Scientific Collaboration, The Virgo Collaboration, J. Aasi +867

In 2009-2010, the Laser Interferometer Gravitational-wave Observa- tory (LIGO) operated together with international partners Virgo and GEO600 as a network to search for gravitation…

astro-ph.HE2011

Beating the spin-down limit on gravitational wave emission from the Vela pulsar

The LIGO Scientific Collaboration, the Virgo Collaboration, J. Abadie +747

We present direct upper limits on continuous gravitational wave emission from the Vela pulsar using data from the Virgo detector's second science run. These upper limits have been…

gr-qc2013

Search for Gravitational Waves from Binary Black Hole Inspiral, Merger and Ringdown in LIGO-Virgo Data from 2009-2010

The LIGO Scientific Collaboration, the Virgo Collaboration, J. Aasi +800

We report a search for gravitational waves from the inspiral, merger and ringdown of binary black holes (BBH) with total mass between 25 and 100 solar masses, in data taken at the…

astro-ph2005

INTEGRAL and XMM-Newton observations of the low-luminosity and X-ray rich burst GRB 040223

S. McGlynn, S. McBreen, L. Hanlon +6

GRB 040223 was observed by INTEGRAL and XMM-Newton. GRB 040223 has a peak flux of (1.6+/-0.13) x10^-8 ergs cm^-2 s^-1, a fluence of (4.4+/-0.4)x10^-7 ergs cm^-2 and a steep photon…

astro-ph2008

Global characteristics of GRBs observed with INTEGRAL and the inferred large population of low-luminosity GRBs

S. Foley, S. McGlynn, L. Hanlon +2

INTEGRAL has two sensitive gamma-ray instruments that have detected 46 gamma-ray bursts (GRBs) up to July 2007. We present the spectral, spatial, and temporal properties of the bur…

astro-ph.HE2014

Gravitational waves from known pulsars: results from the initial detector era

J. Aasi, J. Abadie, B. P. Abbott +892

We present the results of searches for gravitational waves from a large selection of pulsars using data from the most recent science runs (S6, VSR2 and VSR4) of the initial generat…

gr-qc2012

Search for Gravitational Waves from Low Mass Compact Binary Coalescence in LIGO's Sixth Science Run and Virgo's Science Runs 2 and 3

the LIGO Scientific Collaboration, the Virgo Collaboration, J. Abadie +796

We report on a search for gravitational waves from coalescing compact binaries using LIGO and Virgo observations between July 7, 2009 and October 20, 2010. We searched for signals…

astro-ph2006

Observations of the intense and ultra-long burst GRB041219a with the Germanium Spectrometer on INTEGRAL

S. McBreen, L. Hanlon, S. McGlynn +5

GRB041219a is the brightest burst localised by INTEGRAL. The intense burst occurred about ~250s after the precursor and the long delay enabled optical and near infrared telescopes…

astro-ph.HE2010

Predictions for the Rates of Compact Binary Coalescences Observable by Ground-based Gravitational-wave Detectors

LIGO Scientific Collaboration, Virgo Collaboration, J. Abadie +709

We present an up-to-date, comprehensive summary of the rates for all types of compact binary coalescence sources detectable by the Initial and Advanced versions of the ground-based…

astro-ph.IM2018

In-flight measurement of Planck telescope emissivity

F. Cuttaia, L. Terenzi, G. Morgante +19

The Planck satellite in orbit mission ended in October 2013. Between the end of Low Frequency Instrument (LFI) routine mission operations and the satellite decommissioning, a dedic…

gr-qc2012

Einstein@Home all-sky search for periodic gravitational waves in LIGO S5 data

J. Aasi, J. Abadie, B. P. Abbott +794

This paper presents results of an all-sky searches for periodic gravitational waves in the frequency range [50, 1190] Hz and with frequency derivative ranges of [-2 x 10^-9, 1.1 x…

gr-qc2013

Parameter estimation for compact binary coalescence signals with the first generation gravitational-wave detector network

the LIGO Scientific Collaboration, the Virgo Collaboration, J. Aasi +801

Compact binary systems with neutron stars or black holes are one of the most promising sources for ground-based gravitational wave detectors. Gravitational radiation encodes rich i…

astro-ph2009

In search of progenitors for supernova-less GRBs 060505 and 060614: re-examination of their afterglows

D. Xu, R. L. C. Starling, J. P. U. Fynbo +6

GRB060505 and GRB060614 are nearby long-duration gamma-ray bursts (LGRBs) without accompanying supernovae (SNe) down to very strict limits. They thereby challenge the conventional…

gr-qc2010

Calibration of the LIGO Gravitational Wave Detectors in the Fifth Science Run

LIGO Scientific Collaboration, J. Abadie, B. P. Abbott +538

The Laser Interferometer Gravitational Wave Observatory (LIGO) is a network of three detectors built to detect local perturbations in the space-time metric from astrophysical sourc…

physics.ins-det2016

Seismic isolation of Advanced LIGO: Review of strategy, instrumentation and performance

F. Matichard, B. Lantz, R. Mittleman +49

Isolating ground-based interferometric gravitational wave observatories from environmental disturbances is one of the great challenges of the advanced detector era. In order to dir…