Search Results - "Maccagni, D."
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The VIMOS Public Extragalactic Redshift Survey (VIPERS): galaxy segregation inside filaments at z ≃ 0.7
Published in Monthly notices of the Royal Astronomical Society (11-03-2017)“…We present the first quantitative detection of large-scale filamentary structure at z [not asymptotically =] 0.7 in the large cosmological volume probed by the…”
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Spectral Energy Distributions of Hard X-Ray Selected Active Galactic Nuclei in the XMM-Newton Medium Deep Survey
Published in The Astrophysical journal (01-07-2007)“…We present the SEDs of a hard X-ray selected sample containing 136 sources with F[SUB]2-10keV[/SUB]>10[SUP]-14[/SUP] erg cm[SUP]-2[/SUP] s[SUP]-1[/SUP] 132 are…”
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AGN-enhanced outflows of low-ionization gas in star-forming galaxies at 1.7 < z < 4.6
Published in Monthly notices of the Royal Astronomical Society (01-11-2017)“…Abstract Fast and energetic winds are invoked by galaxy formation models as essential processes in the evolution of galaxies. These outflows can be powered…”
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Clustering-based redshift estimation: application to VIPERS/CFHTLS
Published in Monthly notices of the Royal Astronomical Society (21-10-2016)“…We explore the accuracy of the clustering-based redshift estimation proposed by Ménard et al. when applied to VIMOS Public Extragalactic Redshift Survey…”
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An Investigation of Procedural Radiation Dose Level Awareness and Personal Training Experience in Communicating Ionizing Radiation Examinations Benefits and Risks to Patients in Two European Cardiac Centers
Published in Health physics (1958) (01-07-2019)“…PurposeCardiac interventional practitioners need to be appropriately informed regarding radiation dose quantities and risks. Communicating benefit-risk…”
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The VVDS Data‐Reduction Pipeline: Introducing VIPGI, the VIMOS Interactive Pipeline and Graphical Interface
Published in Publications of the Astronomical Society of the Pacific (01-11-2005)“…The VIMOS VLT Deep Survey (VVDS), designed to measure 150,000 galaxy redshifts, requires a dedicated data reduction and analysis pipeline to process in a…”
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The VIMOS-VLT Deep Survey: evolution in the halo occupation number since z∼ 1
Published in Monthly notices of the Royal Astronomical Society (01-08-2010)“…We model the evolution of the mean galaxy occupation of dark matter haloes over the range 0.1 < z < 1.3, using the data from the VIMOS-VLT Deep Survey. The…”
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The power spectrum from the angular distribution of galaxies in the CFHTLS-Wide fields at redshift ∼0.7
Published in Monthly notices of the Royal Astronomical Society (01-03-2012)“…We measure the real-space galaxy power spectrum on large scales at redshifts 0.5-1.2 using optical colour selected samples from the Canada-France-Hawaii…”
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The XMM-Large Scale Structure catalogue: X-ray sources and associated optical data. Version I
Published in Monthly notices of the Royal Astronomical Society (21-11-2007)“…Following the presentation of the XMM-Large Scale Structure (XMM-LSS) survey X-ray source detection package by Pacaud et al., we provide the source lists for…”
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The VIMOS-VLT Deep Survey: evolution in the halo occupation number since z similar to 1
Published in Monthly notices of the Royal Astronomical Society (01-08-2010)“…We model the evolution of the mean galaxy occupation of dark matter haloes over the range 0.1 < z < 1.3, using the data from the VIMOS-VLT Deep Survey. The…”
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The zCOSMOS-Bright survey: the clustering of early and late galaxy morphological types since z≃ 1
Published in Monthly notices of the Royal Astronomical Society (2011)“…We measure the spatial clustering of galaxies as a function of their morphological type at z≃ 0.8, for the first time in a deep redshift survey with full…”
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Bias in the estimation of global luminosity functions
Published in Monthly notices of the Royal Astronomical Society (21-06-2004)“…We discuss a bias present in the calculation of the global luminosity function (LF) which occurs when analysing faint galaxy samples. This effect exists as a…”
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The XMM Large-Scale Structure survey: a well-controlled X-ray cluster sample over the D1 CFHTLS area
Published in Monthly notices of the Royal Astronomical Society (21-10-2006)“…We present the XMM Large-Scale Structure Survey (XMM-LSS) cluster catalogue corresponding to the Canada–France–Hawaii Telescope Legacy Survey D1 area. The list…”
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The Very Large Telescope Visible Multi‐Object Spectrograph Mask Preparation Software
Published in Publications of the Astronomical Society of the Pacific (01-09-2005)“…VIMOS (Visible Multi‐Object Spectrograph) is a multiobject imaging spectrograph installed at the VLT (Very large Telescope) at the ESO (European Southern…”
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The VIMOS Integral Field Unit: Data‐Reduction Methods and Quality Assessment
Published in Publications of the Astronomical Society of the Pacific (01-11-2005)“…With the new generation of spectrographs, integral field spectroscopy is becoming a widely used observational technique. The Integral Field Unit (IFU) of the…”
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The XMM-LSS survey: the Class 1 cluster sample over the initial 5 deg2 and its cosmological modelling
Published in Monthly notices of the Royal Astronomical Society (11-12-2007)“…We present a sample of 29 galaxy clusters from the XMM-LSS survey over an area of some 5 deg2 out to a redshift of z= 1.05. The sample clusters, which…”
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The VIMOS-VLT Deep Survey: evolution in the halo occupation number since z∼ 1
Published in Monthly notices of the Royal Astronomical Society (01-08-2010)Get full text
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A test of the nature of cosmic acceleration using galaxy redshift distortions
Published in Nature (31-01-2008)“…Observations of distant supernovae indicate that the Universe is now in a phase of accelerated expansion the physical cause of which is a mystery. Formally,…”
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The VLT‐VIRMOS Mask Manufacturing Unit
Published in Publications of the Astronomical Society of the Pacific (01-04-2001)“…The VIRMOS Consortium had the task to design and manufacture two spectrographs for the ESO Very Large Telescope, VIMOS (Visible Multi‐Object Spectrograph) and…”
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