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The XMM Large Scale Structure Survey and its multi-lambda follow-up

The XMM Large Scale Structure Survey and its multi-lambda follow-up

... X-ray survey is coupled with an extensive follow-up programme of ra- dio, optical and IR ...of the current range of European and other observa- tional facilities to observe ... Voir le document complet

5

The XMM large scale structure survey: optical vs. X-ray classifications of active galactic nuclei and the unified scheme

The XMM large scale structure survey: optical vs. X-ray classifications of active galactic nuclei and the unified scheme

... only up to a few percent of the X-ray absorbed sources with broad emission lines are identified as a BAL QSO: none of our 7 X-ray sources have an optical spec- trum consistent with a BAL QSO ...among ... Voir le document complet

24

The XXL Survey: I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme

The XXL Survey: I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme

... of the evolution of cluster properties, the de- tectability of such objects is, however, prone to very large un- certainties in any ...currently the subject of many search campaigns not only ... Voir le document complet

18

The XMM-LSS survey. Survey design and first results

The XMM-LSS survey. Survey design and first results

... 1.4. The goals of the XMM-LSS Each new generation of instruments brings major improvements over its ...While the BCS sample presented hints of structure in the sky ... Voir le document complet

35

Multi-scale navigation of large trace data: A survey

Multi-scale navigation of large trace data: A survey

... items and links. Data Correspondence One important issue in multi-level visualization is deciding about managing and representing the correspondence be- tween ...organize and visualize ... Voir le document complet

21

Angular Clustering of X-ray Point-Like Sources in the XMM Large Scale Structure Survey

Angular Clustering of X-ray Point-Like Sources in the XMM Large Scale Structure Survey

... present the log(N)-log(S) diagram and an angular clustering analysis of point-like X-ray sources for the XMM-Newton Large Scale Structure (XMM-LSS) Sur- ...study ... Voir le document complet

2

The XMM Large-Scale Structure survey: a well-controlled X-ray cluster sample over the D1 CFHTLS area

The XMM Large-Scale Structure survey: a well-controlled X-ray cluster sample over the D1 CFHTLS area

... to the deepest serendipitous ROSAT surveys (Rosati et ...However, XMM observations possess a narrower PSF (FWHM ∼ 6 ′′ for XMM vs ∼ 20 ′′ for the ROSAT PSPC) which suggests that the ... Voir le document complet

12

The XMM-LSS survey - First high redshift galaxy clusters: Relaxed and collapsing systems

The XMM-LSS survey - First high redshift galaxy clusters: Relaxed and collapsing systems

... from the XMM Large-Scale Structure Survey ...in the XMM ...of the velocity dispersion is possible: XLSSC 001 at z = 0.613 and σ V = 867 +80 −60 km s ... Voir le document complet

11

The XMM Large-Scale Structure survey: the X-ray pipeline and survey selection function

The XMM Large-Scale Structure survey: the X-ray pipeline and survey selection function

... regards the C1 sample, only genuine extended X- ray sources are detected, as expected, with no additional ...contamination. The majority (≈85%) of the extended C1 sources are clusters, the ... Voir le document complet

16

The XMM-LSS survey: the Class 1 cluster sample over the initial 5 deg(2) and its cosmological modelling

The XMM-LSS survey: the Class 1 cluster sample over the initial 5 deg(2) and its cosmological modelling

... from the XMM-LSS survey over an area of some 5 deg 2 out to a redshift of z = ...1.05. The sample clusters, which represent about half of the X-ray clusters identified in the ... Voir le document complet

20

The XMM-LSS survey - The XMDS/VVDS 4 sigma catalogue

The XMM-LSS survey - The XMDS/VVDS 4 sigma catalogue

... for the HELLAS2XMM survey. We refer to the latter paper for the formalism and procedure, and only mention here the main points and the few di ...used ... Voir le document complet

16

Probing Cosmology with the homogeneity scale of the Universe through large scale structure surveys.

Probing Cosmology with the homogeneity scale of the Universe through large scale structure surveys.

... on the redshift information z of the celestial ...Fluctuations The solutions of the Boltzmann-Einstein equations depend on the choice of the initial ...conditions. The ... Voir le document complet

214

D.1.1 – Survey on Weak Consistency Approaches for Large-Scale Systems

D.1.1 – Survey on Weak Consistency Approaches for Large-Scale Systems

... In survey presented by Shapiro, Preguiça, Baquero, and Zawirski distinguished between state-based and operation- based ...CDRDTs. The simpler form, state-based CRDTs are formally defined on ... Voir le document complet

20

Large-scale survey of lithium concentrations in marine organisms

Large-scale survey of lithium concentrations in marine organisms

... Hg, and Zn have been widely investigated in marine ecotoxicological studies considering their bioaccumulation, transfer along trophic webs, and the risks they pose to ecosystems and human ... Voir le document complet

46

Precision cosmology with the large-scale structure of the universe

Precision cosmology with the large-scale structure of the universe

... determine the light path In practice, what we did to determine the light path between a source and an observer is to start from the observer (assumed to stand in the Friedmann-Lemaˆıtre ... Voir le document complet

240

Bayesian large-scale structure inference and cosmic web analysis

Bayesian large-scale structure inference and cosmic web analysis

... 4 and 5 , (see Jasche & Wandelt , 2013a ; Jasche, Leclercq & Wandelt , 2015 ), the borg inference framework possesses a high degree of control on observational systematic and statistical ... Voir le document complet

238

The XMM-Newton view of Plaskett's star and its surroundings

The XMM-Newton view of Plaskett's star and its surroundings

... in the RGS spectra (see Fig. 1(b)) despite the large ISM ...observed and the nitrogen tends to disappear. Actually, the power law component with γ ∼ ...for the bump at 0.5 ... Voir le document complet

4

Renal function assessment is part of endovascular aortic aneurysm repair and its follow up.

Renal function assessment is part of endovascular aortic aneurysm repair and its follow up.

... Charles and al reported in their 9 years follow up study yearly drop of eGFR of ...[7]. The decline seems to be steeper the first year after EVAR ...diabetes and prior history of ... Voir le document complet

2

Multi-observation PET image analysis for patient follow-up quantitation and therapy assessment.

Multi-observation PET image analysis for patient follow-up quantitation and therapy assessment.

... during the treatment. Such measurements do not reflect overall tumour volume and radiotracer uptake ...variations. The proposed approach is based on multi-observation image analysis for ... Voir le document complet

14

Response function of the large-scale structure of the universe to the small scale inhomogeneities

Response function of the large-scale structure of the universe to the small scale inhomogeneities

... infer the impact of the small-scale physics to the large-scale properties of the universe, we use a series of cosmological N-body simulations of self-gravitating matter ... Voir le document complet

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