Shapiro delay of asteroids on LISA (2009)
Chauvineau, Bertrand, Pireaux, Sophie, Regimbau, Tania
In this paper, we examine the Shapiro delay caused by the close approach of an asteroid to the LISA constellation. We find that the probability that such an event occurs at a detectable level during...
Regimbau, Tania, Hughes, Scott A.
Increasing the sensitivity of a gravitational-wave (GW) detector improves our ability to measure the characteristics of detected sources. It also increases the number of weak signals that contribute...
LISACode : A scientific simulator of LISA (2008)
Petiteau, Antoine, Auger, G., Halloin, H., Jeannin, O., Plagnol, E., Pireaux, Sophie, ...
A new LISA simulator (LISACode) is presented. Its ambition is to achieve a new degree of sophistication allowing to map, as closely as possible, the impact of the different sub-systems on the...
LISACode : A scientific simulator of LISA (2008)
Petiteau, Antoine, Auger, G., Halloin, H., Jeannin, O., Plagnol, E., Pireaux, Sophie, ...
A new LISA simulator (LISACode) is presented. Its ambition is to achieve a new degree of sophistication allowing to map, as closely as possible, the impact of the different sub-systems on the...
LISACode : A scientific simulator of LISA (2008)
Petiteau, Antoine, Auger, G., Halloin, H., Jeannin, O., Plagnol, E., Pireaux, Sophie, ...
A new LISA simulator (LISACode) is presented. Its ambition is to achieve a new degree of sophistication allowing to map, as closely as possible, the impact of the different sub-systems on the...
LISACode : A scientific simulator of LISA (2008)
Petiteau, Antoine, Auger, G., Halloin, H., Jeannin, O., Plagnol, E., Pireaux, Sophie, ...
A new LISA simulator (LISACode) is presented. Its ambition is to achieve a new degree of sophistication allowing to map, as closely as possible, the impact of the different sub-systems on the...
Prospects for Stochastic Background Searches Using Virgo and LSC Interferometers (2007)
Cella, Giancarlo, Colacino, Carlo Nicola, Cuoco, Elena, Di Virgilio, Angela, Regimbau, Tania, Robinson, Emma L, ...
We consider the question of cross-correlation measurements using Virgo and the LSC Interferometers (LIGO Livingston, LIGO Hanford, and GEO600) to search for a stochastic gravitational-wave...
Prospects for Stochastic Background Searches Using Virgo and LSC Interferometers (2007)
Cella, Giancarlo, Colacino, Carlo Nicola, Cuoco, Elena, Di Virgilio, Angela, Regimbau, Tania, Robinson, Emma L., ...
We consider the question of cross-correlation measurements using Virgo and the LSC Interferometers (LIGO Livingston, LIGO Hanford, and GEO600) to search for a stochastic gravitational-wave...
Stochastic background from inspiralling double neutron stars (2006)
We review the contribution of extra galactic inspiralling double neutron stars, to the LISA astrophysical gravitational wave foreground. Using recent fits of the star formation rate, we show that...
Etoiles à neutrons et ondes gravitationnelles (2006)
Nous présentons des synthèses de populations permettant de retrouver les propriétés statistiques de la population réelle des pulsars radio galactiques à partir de l'échantillon observé...
Advanced VIRGO: detector optimization for gravitational waves by inspiralling binaries (2006)
Aoudia, Sofiane, Pacheco, Jose De Freitas, Frossati, Giorgio, Regimbau, Tania
For future configurations, we study the relation between the abatement of the noise sources and the Signal to Noise Ratio (SNR) for coalescing binaries. Our aim is not the proposition of a new...
Capture Rates of Compact Objects by Supermassive Black Holes (2006)
Filloux, Charline, Regimbau, Tania
Capture rates of compact objects were calculated by using a recent solution of the Fokker-Planck equation in energy-space, including two-body resonant effects. The fraction of compact objects (white...
Gravitational Wave Background from Magnetars (2006)
We investigate the gravitational wave background produced by magnetars. The statistical properties of these highly magnetized stars were derived by population synthesis methods and assumed to be also...
Coward, David, Regimbau, Tania
Key targets for gravitational wave (GW) observatories, such as LIGO and the next generation interferometric detector, Advanced LIGO, include core-collapse of massive stars and the final stage of...
Relativistic analysis of the LISA long range optical links (2006)
Chauvineau, Bertrand, Regimbau, Tania, Vinet, Jean-Yves, Pireaux, Sophie
The joint ESA/NASA LISA mission consists in three spacecraft on heliocentric orbits, flying in a triangular formation of 5 Mkm each side, linked by infrared optical beams. The aim of the mission is...
Advanced VIRGO: detector optimization for gravitational waves by inspiralling binaries (2006)
Aoudia, Sofiane, Pacheco, Jose De Freitas, Frossati, Giorgio, Regimbau, Tania
For future configurations, we study the relation between the abatement of the noise sources and the Signal to Noise Ratio (SNR) for coalescing binaries. Our aim is not the proposition of a new...
Relativistic analysis of the LISA long range optical links (2006)
Chauvineau, Bertrand, Regimbau, Tania, Vinet, Jean-Yves, Pireaux, Sophie
The joint ESA/NASA LISA mission consists in three spacecraft on heliocentric orbits, flying in a triangular formation of 5 Mkm each side, linked by infrared optical beams. The aim of the mission is...
Levinson, Amir, Lee, Hyun Kyu, Regimbau, Tania, Punturo, Michele, Harry, Gregory M.
Gamma-ray bursts are believed to originate in core-collapse of massive stars. This produces an active nucleus containing a rapidly rotating Kerr black hole surrounded by a uniformly magnetized torus...
Searching Gravitational Waves from Pulsars, Using Laser Beam Interferometers (2006)
We use recent population synthesis results to investigate the distribution of pulsars in the frequency space, having a gravitational strain high enough to be detected by the future generations of...
Observational evidence for a correlation between peak-luminosities and beaming in GRBs (2006)
We calculate the unseen-but-true GRB-event rate from a current flux-limited sample of 33 GRBs with individually measured redshifts. We consider a GRB-event rate which is proportional to the...
Coward, David, Regimbau, Tania
Key targets for gravitational wave (GW) observatories, such as LIGO and the next generation interferometric detector, Advanced LIGO, include core-collapse of massive stars and the final stage of...
Capture Rates of Compact Objects by Supermassive Black Holes (2006)
Filloux, Charline, Regimbau, Tania
Capture rates of compact objects were calculated by using a recent solution of the Fokker-Planck equation in energy-space, including two-body resonant effects. The fraction of compact objects (white...
Capture Rates of Compact Objects by Supermassive Black Holes (2006)
Filloux, Charline, Regimbau, Tania
Capture rates of compact objects were calculated by using a recent solution of the Fokker-Planck equation in energy-space, including two-body resonant effects. The fraction of compact objects (white...
Capture Rates of Compact Objects by Supermassive Black Holes (2006)
Filloux, Charline, Regimbau, Tania
Capture rates of compact objects were calculated by using a recent solution of the Fokker-Planck equation in energy-space, including two-body resonant effects. The fraction of compact objects (white...
Gravitational Wave Background from Magnetars (2006)
We investigate the gravitational wave background produced by magnetars. The statistical properties of these highly magnetized stars were derived by population synthesis methods and assumed to be also...
Gravitational Wave Background from Magnetars (2006)
We investigate the gravitational wave background produced by magnetars. The statistical properties of these highly magnetized stars were derived by population synthesis methods and assumed to be also...
Coward, David, Regimbau, Tania
Key targets for gravitational wave (GW) observatories, such as LIGO and the next generation interferometric detector, Advanced LIGO, include core-collapse of massive stars and the final stage of...
Coward, David, Regimbau, Tania
Key targets for gravitational wave (GW) observatories, such as LIGO and the next generation interferometric detector, Advanced LIGO, include core-collapse of massive stars and the final stage of...
Relativistic analysis of the LISA long range optical links (2005)
Chauvineau, Bertrand, Pireaux, Sophie, Regimbau, Tania, Vinet, Jean-Yves
The joint ESA/NASA LISA mission consists in three spacecraft on heliocentric orbits, flying in a triangular formation of 5 Mkm each side, linked by infrared optical beams. The aim of the mission is...
Relativistic analysis of the LISA long range optical links (2005)
Chauvineau, Bertrand, Regimbau, Tania, Vinet, Jean-Yves, Pireaux, Sophie
The joint ESA/NASA LISA mission consists in three spacecraft on heliocentric orbits, flying in a triangular formation of 5 Mkm each side, linked by infrared optical beams. The aim of the mission is...
Relativistic analysis of the LISA long range optical links (2005)
Chauvineau, Bertrand, Pireaux, Sophie, Regimbau, Tania, Vinet, Jean-Yves
The joint ESA/NASA LISA mission consists in three spacecraft on heliocentric orbits, flying in a triangular formation of 5 Mkm each side, linked by infrared optical beams. The aim of the mission is...
Gravitational Wave Background from Magnetars (2005)
We investigate the gravitational wave background produced by magnetars. The statistical properties of these highly magnetized stars were derived by population synthesis methods and assumed to be also...
Advanced VIRGO: detector optimization for gravitational waves by inspiralling binaries (2005)
Aoudia, Sofiane, Pacheco, Jose De Freitas, Frossati, Giorgio, Regimbau, Tania
For future configurations, we study the relation between the abatement of the noise sources and the Signal to Noise Ratio (SNR) for coalescing binaries. Our aim is not the proposition of a new...
Advanced VIRGO: detector optimization for gravitational waves by inspiralling binaries (2005)
Aoudia, Sofiane, Pacheco, Jose De Freitas, Frossati, Giorgio, Regimbau, Tania
For future configurations, we study the relation between the abatement of the noise sources and the Signal to Noise Ratio (SNR) for coalescing binaries. Our aim is not the proposition of a new...
Relativistic analysis of the LISA long range optical links (2005)
Chauvineau, Bertrand, Regimbau, Tania, Vinet, Jean-Yves, Pireaux, Sophie
The joint ESA/NASA LISA mission consists in three spacecraft on heliocentric orbits, flying in a triangular formation of 5 Mkm each side, linked by infrared optical beams. The aim of the mission is...
Relativistic analysis of the LISA long range optical links (2005)
Chauvineau, Bertrand, Regimbau, Tania, Vinet, Jean-Yves, Pireaux, Sophie
The joint ESA/NASA LISA mission consists in three spacecraft on heliocentric orbits, flying in a triangular formation of 5 Mkm each side, linked by infrared optical beams. The aim of the mission is...
Advanced VIRGO: detector optimization for gravitational waves by inspiralling binaries (2004)
Aoudia, Sofiane, Pacheco, Jose De Freitas, Frossati, Giorgio, Regimbau, Tania
For future configurations, we study the relation between the abatement of the noise sources and the Signal to Noise Ratio (SNR) for coalescing binaries. Our aim is not the proposition of a new...
Levinson, Amir, Lee, Hyun Kyu, Regimbau, Tania, Punturo, Michele, Harry, Gregory M.
Gamma-ray bursts are believed to originate in core-collapse of massive stars. This produces an active nucleus containing a rapidly rotating Kerr black hole surrounded by a uniformly magnetized torus...
Levinson, Amir, Lee, Hyun Kyu, Regimbau, Tania, Punturo, Michele, Harry, Gregory M.
Gamma-ray bursts are believed to originate in core-collapse of massive stars. This produces an active nucleus containing a rapidly rotating Kerr black hole surrounded by a uniformly magnetized torus...
Levinson, Amir, Lee, Hyun Kyu, Regimbau, Tania, Punturo, Michele, Harry, Gregory M.
Gamma-ray bursts are believed to originate in core-collapse of massive stars. This produces an active nucleus containing a rapidly rotating Kerr black hole surrounded by a uniformly magnetized torus...
Observational evidence for a correlation between peak-luminosities and beaming in GRBs (2003)
We calculate the unseen-but-true GRB-event rate from a current flux-limited sample of 33 GRBs with individually measured redshifts. We consider a GRB-event rate which is proportional to the...
Searching Gravitational Waves from Pulsars, Using Laser Beam Interferometers (2003)
We use recent population synthesis results to investigate the distribution of pulsars in the frequency space, having a gravitational strain high enough to be detected by the future generations of...
Searching Gravitational Waves from Pulsars, Using Laser Beam Interferometers (2003)
We use recent population synthesis results to investigate the distribution of pulsars in the frequency space, having a gravitational strain high enough to be detected by the future generations of...
Observational evidence for a correlation between peak-luminosities and beaming in GRBs (2003)
We calculate the unseen-but-true GRB-event rate from a current flux-limited sample of 33 GRBs with individually measured redshifts. We consider a GRB-event rate which is proportional to the...
Observational evidence for a correlation between peak-luminosities and beaming in GRBs (2003)
We calculate the unseen-but-true GRB-event rate from a current flux-limited sample of 33 GRBs with individually measured redshifts. We consider a GRB-event rate which is proportional to the...
Bose, Sukanta, Allen, Bruce, Landry, Michael, Lazzarini, Albert, Leonor, Isabel, Marka, Szabolcs, ...
We describe the utility of simulated-signal injection studies on earth-based gravitational-wave (GW) interferometric data toward obtaining bounds on the strength of a stochastic GW background. The...
Searching Gravitational Waves from Pulsars, Using Laser Beam Interferometers (2002)
We use recent population synthesis results to investigate the distribution of pulsars in the frequency space, having a gravitational strain high enough to be detected by the future generations of...
Etoiles à neutrons et ondes gravitationnelles (2001)
Nous présentons des synthèses de populations permettant de retrouver les propriétés statistiques de la population réelle des pulsars radio galactiques à partir de l'échantillon observé...
Etoiles à neutrons et ondes gravitationnelles (2001)
Nous présentons des synthèses de populations permettant de retrouver les propriétés statistiques de la population réelle des pulsars radio galactiques à partir de l'échantillon observé...
Etoiles à neutrons et ondes gravitationnelles (2001)
Nous présentons des synthèses de populations permettant de retrouver les propriétés statistiques de la population réelle des pulsars radio galactiques à partir de l'échantillon observé...