Search Results - "Lentati, Lindley"
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Deep CO(1-0) Observations of z = 1.62 Cluster Galaxies with Substantial Molecular Gas Reservoirs and Normal Star Formation Efficiencies
Published in The Astrophysical journal (01-11-2017)“…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)…”
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The intense starburst HDF 850.1 in a galaxy overdensity at z ≈ 5.2 in the Hubble Deep Field
Published in Nature (London) (14-06-2012)“…Using a millimetre-wave molecular line scan, a redshift has finally been determined for the extremely active star-forming galaxy HDF 850.1 in the Hubble Deep…”
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STAR FORMATION AND GAS KINEMATICS OF QUASAR HOST GALAXIES AT z ∼ 6: NEW INSIGHTS FROM ALMA
Published in The Astrophysical journal (10-08-2013)“…We present Atacama Large Millimeter/submillimeter Array (AT,MA) observations of the [CiII] 158 mu m fine structure line and dust continuum emission from the…”
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Contamination of the Epoch of Reionization power spectrum in the presence of foregrounds
Published in Monthly notices of the Royal Astronomical Society (01-11-2016)“…We construct foreground simulations comprising spatially correlated extragalactic and diffuse Galactic emission components and calculate the 'intrinsic'…”
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5
The intense starburst HDF850.1 in a galaxy overdensity at z [asymptotically =] 5.2 in the Hubble Deep Field
Published in Nature (London) (14-06-2012)“…The Hubble Deep Field provides one of the deepest multiwavelength views of the distant Universe and has led to the detection of thousands of galaxies seen…”
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6
European Pulsar Timing Array limits on continuous gravitational waves from individual supermassive black hole binaries
Published in Monthly notices of the Royal Astronomical Society (11-01-2016)“…We have searched for continuous gravitational wave (CGW) signals produced by individually resolvable, circular supermassive black hole binaries (SMBHBs) in the…”
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7
Contamination of the Epoch of Reionization power spectrum in the presence of foregrounds
Published 26-07-2016“…We construct foreground simulations comprising spatially correlated extragalactic and diffuse Galactic emission components and calculate the `intrinsic'…”
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8
Bayesian estimation of non-Gaussianity in pulsar timing analysis
Published 18-09-2014“…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,…”
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9
Deep CO(1-0) Observations of z=1.62 Cluster Galaxies with Substantial Molecular Gas Reservoirs and Normal Star Formation Efficiencies
Published 20-09-2017“…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)…”
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10
A Bayesian blind survey for cold molecular gas in the Universe
Published 15-08-2014“…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…”
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European Pulsar Timing Array limits on an isotropic stochastic gravitational-wave background
Published in Monthly notices of the Royal Astronomical Society (01-11-2015)“…We present new limits on an isotropic stochastic gravitational-wave background (GWB) using a six pulsar data set spanning 18 yr of observations from the 2015…”
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12
TempoNest: A Bayesian approach to pulsar timing analysis
Published 08-10-2013“…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…”
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13
Hyper-efficient model-independent Bayesian method for the analysis of pulsar timing data
Published 25-06-2013“…Physical Review D, vol. 87, Issue 10, id. 104021 05/2013 A new model independent method is presented for the analysis of pulsar timing data and the estimation…”
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14
European Pulsar Timing Array Limits on Continuous Gravitational Waves from Individual Supermassive Black Hole Binaries
Published 11-09-2015“…We have searched for continuous gravitational wave (CGW) signals produced by individually resolvable, circular supermassive black hole binaries (SMBHBs) in the…”
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15
European Pulsar Timing Array Limits On An Isotropic Stochastic Gravitational-Wave Background
Published 09-09-2015“…Monthly Notices of the Royal Astronomical Society 2015 453 (3): 2576-2598 We present new limits on an isotropic stochastic gravitational-wave background (GWB)…”
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16
Star Formation and Gas Kinematics of Quasar Host Galaxies at z~6: New insights from ALMA
Published 08-07-2013“…We present ALMA observations of the [C II] 158 micron fine structure line and dust continuum emission from the host galaxies of five redshift 6 quasars. We…”
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17
Variations in the Fundamental constants in the QSO Host J1148+5251 at z = 6.4 and the BR1202-0725 System at z = 4.7
Published 14-11-2012“…We use sensitive observations of three high redshift sources; [CII] fine structure and CO(2-1) rotational transitions for the z=6.4 Quasar host galaxy (QSO)…”
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18
The intense starburst HDF850.1 in a galaxy overdensity at z approximately 5.2 in the Hubble Deep Field
Published in Nature (London) (04-06-2012)“…The Hubble Deep Field provides one of the deepest multiwavelength views of the distant Universe and has led to the detection of thousands of galaxies seen…”
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19
Hyper-efficient model-independent Bayesian method for the analysis of pulsar timing data
Published in Physical review. D, Particles, fields, gravitation, and cosmology (20-05-2013)“…A new model-independent method is presented for the analysis of pulsar timing data and the estimation of the spectral properties of an isotropic gravitational…”
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20
How to take the interstellar weather with you in pulsar timing analysis
Published 09-12-2013“…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…”
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