Zobrazeno 1 - 10
of 28
pro vyhledávání: '"Lentati, Lindley"'
Autor:
Rudnick, Gregory, Hodge, Jacqueline, Walter, Fabian, Momcheva, Ivelina, Tran, Kim-Vy, Papovich, Casey, da Cunha, Elisabete, Decarli, Roberto, Saintonge, Amelie, Willmer, Christopher, Lotz, Jennifer, Lentati, Lindley
We present an extremely deep CO(1-0) observation of a confirmed z = 1.62 galaxy cluster. We detect two spectroscopically confirmed cluster members in CO(1-0) with signal-to-noise ratio >5. Both galaxies have log (M-star/M-circle dot) > 11 and are gas
Externí odkaz:
http://hdl.handle.net/10150/627107
http://arizona.openrepository.com/arizona/handle/10150/627107
http://arizona.openrepository.com/arizona/handle/10150/627107
Autor:
Rudnick, Gregory, Hodge, Jacqueline, Walter, Fabian, Momcheva, Ivelina, Tran, Kim-Vy, Papovich, Casey, da Cunha, Elisabete, Decarli, Roberto, Saintonge, Amelie, Willmer, Christopher, Lotz, Jennifer, Lentati, Lindley
We present an extremely deep CO(1-0) observation of a confirmed $z=1.62$ galaxy cluster. We detect two spectroscopically confirmed cluster members in CO(1-0) with $S/N>5$. Both galaxies have log(${\cal M_{\star}}$/\msol)$>11$ and are gas rich, with $
Externí odkaz:
http://arxiv.org/abs/1709.06963
Autor:
Sims, Peter H., Lentati, Lindley, Pober, Jonathan C., Carilli, Chris, Hobson, Michael P., Alexander, Paul, Sutter, Paul
We introduce a new method for performing robust Bayesian estimation of the three-dimensional spatial power spectrum at the Epoch of Reionization (EoR), from interferometric observations. The versatility of this technique allows us to present two appr
Externí odkaz:
http://arxiv.org/abs/1701.03384
We construct foreground simulations comprising spatially correlated extragalactic and diffuse Galactic emission components and calculate the `intrinsic' (instrument-free) two-dimensional spatial power spectrum and the cylindrically and spherically av
Externí odkaz:
http://arxiv.org/abs/1607.07628
Autor:
Babak, Stanislav, Petiteau, Antoine, Sesana, Alberto, Brem, Patrick, Rosado, Pablo A., Taylor, Stephen R., Lassus, Antoine, Hessels, Jason W. T., Bassa, Cees G., Burgay, Marta, Caballero, R. Nicolas, Champion, David J., Cognard, Ismael, Desvignes, Gregory, Gair, Jonathan R., Guillemot, Lucas, Janssen, Gemma H., Karuppusamy, Ramesh, Kramer, Michael, Lazarus, Patrick, Lee, K. J., Lentati, Lindley, Liu, Kuo, Mingarelli, Chiara M. F., Oslowski, Stefan, Perrodin, Delphine, Possenti, Andrea, Purver, Mark B., Sanidas, Sotiris, Smits, Roy, Stappers, Ben, Theureau, Gilles, Tiburzi, Caterina, van Haasteren, Rutger, Vecchio, Alberto, Verbiest, Joris P. W.
We have searched for continuous gravitational wave (CGW) signals produced by individually resolvable, circular supermassive black hole binaries (SMBHBs) in the latest EPTA dataset, which consists of ultra-precise timing data on 41 millisecond pulsars
Externí odkaz:
http://arxiv.org/abs/1509.02165
Autor:
Lentati, Lindley, Taylor, Stephen R., Mingarelli, Chiara M. F., Sesana, Alberto, Sanidas, Sotiris A., Vecchio, Alberto, Caballero, R. Nicolas, Lee, K. J., van Haasteren, Rutger, Babak, Stanislav, Bassa, Cees G., Brem, Patrick, Burgay, Marta, Champion, David J., Cognard, Ismael, Desvignes, Gregory, Gair, Jonathan R., Guillemot, Lucas, Hessels, Jason W. T., Janssen, Gemma H., Karuppusamy, Ramesh, Kramer, Michael, Lassus, Antoine, Lazarus, Patrick, Liu, Kuo, Osłowski, Stefan, Perrodin, Delphine, Petiteau, Antoine, Possenti, Andrea, Purver, Mark B., Rosado, Pablo A., Smits, Roy, Stappers, Ben, Theureau, Gilles, Tiburzi, Caterina, Verbiest, Joris P. W.
Publikováno v:
Monthly Notices of the Royal Astronomical Society 2015 453 (3): 2576-2598
We present new limits on an isotropic stochastic gravitational-wave background (GWB) using a six pulsar dataset spanning 18 yr of observations from the 2015 European Pulsar Timing Array data release. Performing a Bayesian analysis, we fit simultaneou
Externí odkaz:
http://arxiv.org/abs/1504.03692
Publikováno v:
MNRAS (October 1, 2014) 443 (4): 3741-3751
A new Bayesian method for performing an image domain search for line-emitting galaxies is presented. The method uses both spatial and spectral information to robustly determine the source properties, employing either simple Gaussian, or other physica
Externí odkaz:
http://arxiv.org/abs/1408.3585
Publikováno v:
MNRAS (November 11, 2014) 444 (4): 3863-3878
We introduce a method for performing a robust Bayesian analysis of non-Gaussianity present in pulsar timing data, simultaneously with the pulsar timing model, and additional stochastic parameters such as those describing red spin noise and dispersion
Externí odkaz:
http://arxiv.org/abs/1405.2460
Here we present a Bayesian method of including discrete measurements of dispersion measure due to the interstellar medium in the direction of a pulsar as prior information in the analysis of that pulsar. We use a simple simulation to show the efficac
Externí odkaz:
http://arxiv.org/abs/1312.2403
Autor:
Lentati, Lindley, Alexander, Paul, Hobson, Michael P., Feroz, Farhan, van Haasteren, Rutger, Lee, Kejia, Shannon, Ryan M.
A new Bayesian software package for the analysis of pulsar timing data is presented in the form of TempoNest which allows for the robust determination of the non-linear pulsar timing solution simultaneously with a range of additional stochastic param
Externí odkaz:
http://arxiv.org/abs/1310.2120